Electronic Devices and Circuits
Electronic Devices and Circuits
UNIT I 
                        PN DIODE AND ITS APPLICATIONS 
INTRODUCTION 
The  current-voltage  characteristics  is  of  prime  concern  in  the  study  of  semiconductor  devices 
with  light  entering  as  a  third  variable  in  optoelectronics  devices.The  external  characteristics  of 
the device is determined by the interplay of the following internal variables:  
1.  Electron and hole currents 
2.  Potential 
3.  Electron and hole density 
4.  Doping 
5.  Temperature  
Semiconductor equations 
 
The semiconductor equations relating these variables are given below: 
 
Carrier density: 
 
 
where  is the electron quasi Fermi level and  is the hole quasi Fermi level. These two 
equations lead to  
 
In equilibrium  =  = Constant 
 
Current:  
There are two components of current; electron current density and hole current density  . 
There are several mechanisms of current flow: 
(i) Drift 
(ii) Diffusion 
(iii) thermionic emission 
(iv) tunneling  
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The last two mechanisms are important often only at the interface of two different materials such 
as a metal-semiconductor junction or a semiconductor-semiconductor junction where the two 
semiconductors are of different materials. Tunneling is also important in the case of PN junctions 
where both sides are heavily doped.  
 
In the bulk of semiconductor , the dominant conduction mechanisms involve drift and diffusion.  
 
The current densities due to these two mechanisms can be written as 
 
where  are electron and hole mobilities respectively and  are their diffusion 
constants.  
 
Potential: 
 
The potential and electric field within a semiconductor can be defined in the following ways:  
 
 
All these definitions are equivalent and one or the other may be chosen on the basis of 
convenience.The potential is related to the carrier densities by the Poisson equation: -  
 
where the last two terms represent the ionized donor and acceptor density. 
 
Continuity equations 
 
These equations are basically particle conservation equations:  
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Where G and R represent carrier generation and recombination rates.Equations (1-8) will form 
the basis of most of the device analysis that shall be discussed later on. These equations require 
models for mobility and recombination along with models of contacts and boundaries.  
 
Analysis Flow 
 
Like most subjects, the analysis of semiconductor devices is also carried out by starting from 
simpler problems and gradually progressing to more complex ones as described below: 
(i) Analysis under zero excitation i.e. equilibrium. 
(ii) Analysis under constant excitation: in other words dc or static characteristics. 
(iii) Analysis under time varying excitation but with quasi-static approximation dynamic 
characteristics. 
(iv) Analysis under time varying excitation: non quasi-static dynamic characteristics.  
 
 
 
Even though there is zero external current and voltage in equilibrium, the situation inside the 
device is not so trivial. In general, voltages, charges and drift-diffusion current components at 
any given point within the semiconductor may not be zero. 
 
 
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Equilibrium in semiconductors implies the following:  
 
(i) steady state:   
Where Z is any physical quantity such as charge, voltage electric field etc 
 
(ii) no net electrical current and thermal currents: 
 
Since current can be carried by both electrons and holes, equilibrium implies zero values for both 
net electron current and net hole current. The drift and diffusion components of electron and hole 
currents need not be zero. 
 
(iii) Constant Fermi energy:   
 
The only equations that are relevant (others being zero!) for analysis in equilibrium are: 
Poisson Eq: 
 
  
 
In equilibrium, there is only one independent variable out of the three variables :   
If one of them is known, all the rest can be computed from the equations listed above. We shall 
take this independent variable to be potential. 
 
The analysis problem in equilibrium is therefore determination of potential or equivalently, 
energy band diagram of the semiconductor device. 
 
This is the reason why we begin discussions of all semiconductor devices with a sketch of its 
energy band diagram in equilibrium.  
 
 
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Energy Band Diagram 
 
This diagram in qualitative form is sketched by following the following procedure: 
1.  The  semiconductor  device  is  imagined  to  be  formed  by  bringing  together  the  various 
distinct semiconductor layers,  metals or insulators of which  it  is composed. The starting 
point is therefore the energy band diagram of all the constituent layers.  
2.  The  band  diagram  of  the  composite  device  is  sketched  using  the  fact  that  after 
equilibrium, the Fermi energy is the same everywhere in the system. The equalization of 
the Fermi energy is accompanied with transfer of electrons from regions of higher Fermi 
energy to region of lower Fermi energy and viceversa for holes.  
3.  The redistribution of charges results  in electric  field and creation of potential  barriers  in 
the  system.  These  effects  however  are  confined  only  close  to  the  interface  between  the 
layers.  The  regions  which  are  far  from  the  interface  remain  as  they  were  before  the 
equilibrium  
 
Analysis in equilibrium: Solution of Poissons Equation with appropriate boundary conditions -  
 
Non-equilibrium analysis: 
-  The electron and hole densities are no longer related together by the inverse relationship 
of Eq. (5) but through complex relationships involving all three variables Y , , p  
-  The three variables are in general independent of each other in the sense that a knowledge 
of two of them does not lead automatically to a knowledge of the third. 
-  The concept of Fermi energy is no longer valid but new quantities called the quasi-Fermi 
levels are used and these are not in general constant. 
-  For static or dc analysis, the  continuity equation  becomes time  independent so that only 
ordinary differential equations need to be solved. 
-  For  dynamic  analysis  however,  the  partial  differential  equations  have  to  be  solved 
increasing the complexity of the analysis.  
Analysis of Semiconductor Devices 
 
There are two complementary ways of studying semiconductor devices: 
 
(i) Through numerical simulation of the semiconductor equations. 
(ii) Through analytical solution of semiconductor equations. 
-  There are a  variety of techniques used  for device  simulation with some of them  starting 
from the drift diffusion formalism outlined earlier, while others take a more fundamental 
approach starting from the Boltzmann transport equation instead.  
-  In  general,  the  numerical  approach  gives  highly  accurate  results  but  requires  heavy 
computational effort also. 
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-  The output of device simulation in the form of numerical values for all internal variables 
requires  relatively  larger  effort to  understand  and  extract  important  relationships  among 
the device characteristics. 
 The electrons in the valence band are not capable of gaining energy from external electric field 
and  hence  do  not  contribute  to  the  current.  This  band  is  never  empty  but  may  be  partially  or 
completely with  electrons. On the contrary  in the  conduction  band, electrons are rarely present. 
But  it  is  possible  for  electrons  to  gain  energy  from  external  field  and  so  the  electrons  in  these 
bands contribute to the electric current. The forbidden energy gap is devoid of any electrons and 
this much energy is required by electrons to jump from valence band to the conduction band. 
In other words,  in the case of conductors and  semiconductors, as the temperature  increases, the 
valence electrons in the valence energy move from the valence band to conductance band. As the 
electron (negatively charged) jumps from valence band to conductance band, in the valence band 
there is a left out deficiency of electron that is called Hole (positively charged). 
Depending on the  value of E
gap
,  i.e., energy gap solids can  be classified as  metals (conductors), 
insulators and semi conductors. 
Semiconductors  
-  Conductivity in between those of metals and insulators. 
-  Conductivity can  be  varied over orders of  magnitude by  changes  in temperature, optical 
excitation, and impurity content (doping). 
-  Generally found in column IV and neighboring columns of the periodic table. 
-  Elemental semiconductors: Si, Ge. 
-  Compound semiconductors: 
 
Binary :  
  
GaAs,  AlAs,  GaP, 
etc. (III-V). 
  
ZnS, ZnTe, CdSe (II-
VI). 
  
SiC, SiGe (IV 
compounds). 
-  Ternary : GaAsP. 
Quaternary : InGaAsP. 
-  Si widely used for rectifiers, transistors, and ICs. 
-  III-V compounds widely used in optoelectronic and high-speed applications.  
 
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Applications  
-  Integrated circuits (ICs) SSI, MSI, LSI, and VLSI. 
-  Fluorescent materials used in TV screens II-VI (ZnS). 
-  Light detectors InSb, CdSe, PbTe, HgCdTe. 
-  Infrared and nuclear radiation detectors Si and Ge. 
-  Gunn diode (microwave device) GaAs, InP. 
-  Semiconductor LEDs GaAs, GaP. 
-  Semiconductor LASERs GaAs, AlGaAs.  
Energy Gap  
-  Distinguishing feature among metals, insulators, and semiconductors. 
-  Determines  the  absorption/emission  spectra,  the  leakage  current,  and  the  intrinsic 
conductivity. 
-  Unique value for each semiconductor (e.g. 1.12 eV for Si, 1.42 eV for GaAs) function of 
temperature.  
Impurities  
-  Can be added in precisely controlled amounts. 
-  Can change the electronic and optical properties. 
-  Used to vary conductivity over wide ranges. 
-  Can  even  change  conduction  process  from  conduction  by  negative  charge  carriers  to 
positive charge carriers and vice versa. 
-  Controlled addition of impurities doping. 
                                    Energy Bands and Charge Carriers in Semiconductors 
Bonding Forces and Energy Bands in Solids  
-  Electrons  are  restricted  to  sets  of  discrete  energy  levels  within  atoms,  with  large  gaps 
among them where no energy state is available for the electron to occupy. 
-  Electrons  in  solids  also  are  restricted  to  certain  energies  and  are  not  allowed  at  other 
energies. 
-  Difference  in the solid, the electron has a range (or band) of available energies. 
-  The discrete energy levels of the isolated atom spread into bands of energies in the solid 
because 
i)  in  the  solid,  the  wave  functions  of  electrons  in  neighboring  atoms  overlap,  thus,  it 
affects  the  potential  energy  term  and  the  boundary  conditions  in  the  
equation,  and  different  energies  are  obtained  in  the  solution,  and 
ii) an electron is not necessarily localized at a particular atom. 
-  The  influence  of  neighboring  atoms  on  the  energy  levels  of  a  particular  atom  can  be 
treated  as  a  small  perturbation,  giving  rise  to  shifting  and  splitting  of  energy  states  into 
energy bands.  
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Bonding Forces in Solids 
Ionic Bonding  
-  Example: NaCl. 
-  Na  (Z  =  11)  gives  up  its  outermost  shell  electron  to  Cl  (Z=17)  atom,  thus  the  crystal  is 
made up of ions with the electronic structures of the inert atoms Ne and Ar. 
-  Note: the  ions  have  net  electric  charges  after  the  electron  exchange   ion  has  a  net 
positive  charge,  having  lost  an  electron,  and  ion  has  a  net  negative  charge,  having 
acquired an electron. 
-  Thus, an electrostatic attractive force is established, and the balance is reached when this 
equals the net repulsive force. 
-  Note: all the electrons are tightly bound to the atom. 
-  Since there are no loosely bound electrons to participate in current flow  NaCl is a good 
insulator.  
Metallic Bonding  
-  In  metals,  the  outer  shell  is  filled  by  no  more  than  three  electrons  (loosely  bound  and 
given up easily) great chemical activity and high electrical conductivity. 
-  Outer  electron(s)  contributed  to  the  crystal  as  a  whole   solid  made  up  of  ions  with 
closed shells immersed in a sea of free electrons, which are free to move about the crystal 
under the influence of an electric field. 
-  Coulomb attraction force between the ions and the electrons hold the lattice together.  
Covalent Bonding  
-  Exhibited by the diamond lattice semiconductors. 
-  Each  atom  surrounded  by  four  nearest  neighbors,  each  having  four  electrons  in  the 
outermost orbit. 
-  Each atom shares its valence electrons with its four nearest neighbors. 
-  Bonding  forces  arise  from  a  quantum  mechanical  interaction  between  the  shared 
electrons. 
-  Both electrons belong to each bond, are indistinguishable, and have opposite spins. 
-  No  free  electrons  available  at  0  K,  however,  by  thermal  or  optical  excitation,  electrons 
can  be  excited  out  of  a  covalent  bond  and  can  participate  in  current  conduction
important feature of semiconductors.  
Mixed Bonding  
-  Shown by III-V compounds bonding partly ionic and partly covalent. 
-  Ionic  character  of  bonding  becomes  more  prominent  as  the  constituent  atoms  move 
further away in the periodic table, e.g., II-VI compounds.  
 
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Energy Bands  
-  As isolated atoms are brought together to form a solid, the electron wave functions begin 
to overlap. 
-  Various  interactions  occur,  and,  at  the  proper  interatomic  spacing  for  the  crystal,  the 
forces of attraction and repulsion find a balance. 
-  Due to Pauli exclusion principle, the discrete energy levels of individual atoms split into 
bands belonging to the pair instead of to individual atoms. 
-  In a solid, due to large number of atoms, the split energy levels for essentially  continuous 
bands of energy.  
 
 
Fig.2.1  Splitting  of  individual  energy  levels  to  energy  bands  as  atoms  are  brought  closer 
together.  
-  Imaginary formation of a diamond crystal from isolated carbon atoms . 
-  Each atom has two 1s states, two 2s states, six 2p states, and higher states. 
-  For  N  atoms,  the  numbers  of  states  are  2N,  2N,  and  6N  of  type  1s,  2s,  and  2p 
respectively. 
-  With a reduction  in the interatomic spacing, these energy levels split into bands, and the 
2s and 2p bands merge into a single band having 8N available states. 
-  As  the  interatomic  spacing  approaches  the  equilibrium  spacing  of  diamond  crystal,  this 
band  splits  into  two  bands  separated  by  an  energy  gap  ,  where  no  allowed  energy 
states for electrons exist  forbidden gap. 
-  The  upper  band  (called  the  conduction  band)  and  the  lower  band  (called  the  valence 
band) contain 4N states each. 
-  The  lower 1s band  is  filled with 2N electrons, however, the 4N electrons residing  in the 
original n = 2 state will now occupy states either in the valence band or in the conduction 
band. 
-  At 0 K, the electrons will occupy the lowest energy states available to them  thus, the 
4N  states  in  the  valence  band  will  be  completely  filled,  and  the  4N  states  in  the 
conduction band will be completely empty.  
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Metals, Semiconductors, and Insulators  
-  For  electrons  to  move  under  an  applied  electric  field,  there  must  be  states  available  to 
them. 
-  A completely filled  band cannot contribute to current transport; neither can a completely 
empty band. 
-  Thus, semiconductors at 0 K are perfect insulators. 
-  With  thermal  or  optical  excitation,  some  of  these  electrons  can  be  excited  from  the 
valence band to the conduction band, and then they can contribute to the current transport 
process. 
-  At  temperatures  other  than  0  K,  the  magnitude  of  the  band  gap  separates  an  insulator 
from a semiconductor, e.g., at 300 K,  (diamond) = 5 eV (insulator), and  (Silicon) = 
1.12 eV (semiconductor). 
-  Number of electrons available for conduction can be increased greatly in semiconductors 
by reasonable amount of thermal or optical energy. 
-  In  metals,  the  bands  are  either  partially  filled  or  they  overlap  thus,  electrons  and 
empty states coexist  great electrical conductivity.  
Direct and Indirect Semiconductors  
-  In  a  typical  quantitative  calculation  of  band  structures,  the  wave  function  of  a  single 
electron  traveling  through  a  perfectly  periodic  lattice  is  assumed  to  be  in  the  form  of  a 
plane  wave  moving  in  the  x-direction  (say)  with  propagation  constant  k,  also  called  a 
wave vector. 
-  In quantum mechanics, the electron momentum can be given by  
-  The  space  dependent  wave  function  for  the  electron  is 
(2.1)  
where the function  modulates the wave function according to the periodicity of the 
lattice.  
-  Allowed values of energy, while plotted as a function of k, gives the E-k diagram. 
-  Since the periodicity of most lattices is different in various directions, the E-k diagram is 
a complex surface, which is to be visualized in three dimensions.  
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Fig.2.2 Direct and indirect transition of electrons from the conduction band to the valence band: 
(a) direct - with accompanying photon emission, (b) indirect via defect level.  
-  Direct  band  gap  semiconductor: the  minima  of  the  conduction  band  and  the  maxima  of 
the valence band occur at the same value of k an electron making the smallest energy 
transition from the conduction band to the valence band can do so without a change in k 
(and, the momentum). 
-  Indirect band gap semiconductor: the minima of the conduction band and the maxima of 
the valence band occur for different values of k, thus, the smallest energy transition for an 
electron requires a change in momentum. 
-  Electron  falling  from  conduction  band  to  an  empty  state  in  valence  band 
recombination. 
-  Recombination  probability  for  direct  band  gap  semiconductors  is  much  higher  than  that 
for indirect band gap semiconductors. 
-  Direct band gap semiconductors give up the energy released during this transition (=  ) 
in the form of light  used for optoelectronic applications (e.g., LEDs and LASERs). 
-  Recombination  in  indirect  band  gap  semiconductors  occurs  through  some  defect  states 
within the band gap, and the energy is released in the form of heat given to the lattice.  
Variation of Energy Bands with Alloy Composition  
-  The  band  structures  of  III-V  ternary  and  quaternary  compounds  change  as  their 
composition is varied. 
-  There are three valleys in the conduction band:  (at k = 0), L, and X. 
-  In GaAs, the  valley has the minimum energy (direct with  = 1.43 eV) with very few 
electrons residing in L and X valleys (except for high field excitations). 
-  In AlAs, the X valley has minimum energy (indirect with  = 2.16 eV).  
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Fig.2.3 The E-k diagram of (a) GaAs and (b) AlAs, showing the three valleys (L,  , and X) in 
the conduction band. 
 
Charge Carriers in Semiconductors  
-  In  a  metal,  the  atoms  are  imbedded  in  a  "sea"  of  free  electrons,  and  these  electrons  can 
move as a group under the influence of an applied electric field. 
-  In  semiconductors  at  0  K,  all  states  in  the  valence  band  are  full,  and  all  states  in  the 
conduction band are empty. 
-  At T > 0 K, electrons get thermally excited from the valence band to the conduction band, 
and contribute to the conduction process in the conduction band. 
-  The empty states left in the valence band can also contribute to current conduction. 
-  Also,  introduction of  impurities  has an  important effect on the availability of the  charge 
carriers. 
-  Considerable flexibility in controlling the electrical properties of semiconductors.  
Electrons and Holes  
-  For T> 0 K, there would be some electrons in the otherwise empty conduction band, and 
some empty states in the otherwise filled valence band. 
-  The empty states in the valence band are referred to as holes. 
-  If  the  conduction  band  electron  and  the  valence  band  hole  are  created  by  thermal 
excitation  of  a  valence  band  electron  to  the  conduction  band,  then  they  are  called 
electron-hole pair (EHP). 
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-  After  excitation  to the  conduction  band,  an  electron  is  surrounded  by  a  large  number  of 
empty states, e.g., the equilibrium number of EHPs at 300 K in Si is  , whereas 
the Si atom density is  .  
-  Thus, the electrons in the conduction band are free to move about via the many available 
empty states. 
-  Corresponding problem of charge transport in the valence band is slightly more complex. 
-  Current transport in the valence band can be accounted for by keeping track of the holes 
themselves. 
-  In a filled band, all available energy states are occupied. 
-  For every electron moving with a given  velocity,  there is an equal and opposite electron 
motion somewhere else in the band. 
-  Under an applied electric  field, the net current is  zero, since  for every electron j  moving 
with a velocity  , there is a corresponding electron  moving with a velocity - . 
-  In  a  unit  volume,  the  current  density  J  can  be  given  by  
 
(filled  band)  (2.2) 
where N is the number of  in the band, and q is the electronic charge. 
-  Now, if the  electron is removed and a hole is created in the valence band, then the net 
current density 
 
 
-  Thus,  the  current  contribution  of  the  empty  state  (hole),  obtained  by  removing  the  jth 
electron, is equivalent to that of a positively charged particle with velocity  . 
-  Note  that  actually  this  transport  is  accounted  for  by  the  motion  of  the  uncompensated 
electron  having a charge of q and moving with a velocity  . 
-  Its  current  contribution  (-  q)(-  )  is  equivalent  to  that  of  a  positively  charged  particle 
with velocity + . 
-  For simplicity, therefore, the empty states  in the valence band are called holes, and they 
are assigned positive charge and positive mass. 
-  The  electron  energy  increases  as  one  moves  up  the  conduction  band,  and  electrons 
gravitate downward towards the bottom of the conduction band. 
-  On  the  other  hand,  hole  energy  increases  as  one  moves  down  the  valence  band  (since 
holes have positive charges), and holes gravitate upwards towards the top of the valence 
band. 
 
 
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Effective Mass  
-  The  "wave-particle"  motion  of  electrons  in  a  lattice  is  not  the  same  as  that  for  a  free 
electron, because of the interaction with the periodic potential of the lattice. 
-  To still be able to treat these particles as "free", the rest mass has to be altered to take into 
account the influence of the lattice. 
-  The  calculation  of  effective  mass  takes  into  account  the  shape  of  the  energy  bands  in 
three-dimensional k-space, taking appropriate averages over the various energy bands. 
-  The  effective  mass  of  an  electron  in  a  band  with  a  given  (E,k)  relation  is  given  by 
(2.4) 
 
 
EXAMPLE 2.1: Find the dispersion relation for a free electron, and, thus, observe the relation 
between its rest mass and effective mass. 
 
SOLUTION: For a free electron, the electron momentum is  . Thus, 
. Therefore, the dispersion relation, i.e., the E-k relation is 
parabolic. Hence,  . This is a very interesting relation, which states that for 
a free electron, the rest mass and the effective mass are one and the same, which is due to the 
parabolic band structure. Most materials have non-parabolic E-k relation, and, thus, they have 
quite different rest mass and effective mass for electrons. 
 
Note: for severely non-parabolic band structures, the effective mass may become a function of 
energy, however, near the minima of the conduction band and towards the maxima of the 
valence band, the band structure can be taken to be parabolic, and, thus, an effective mass, which 
is independent of energy, may be obtained. 
-  Thus, the effective mass is an inverse function of the curvature of the E-k diagram: weak 
curvature gives large mass, and strong curvature gives small mass. 
-  Note that in general, the effective mass is a tensor quantity, however, for parabolic bands, 
it is a constant. 
-  Another interesting feature is that the curvature  is positive at the conduction band 
minima, however, it is negative at the valence band maxima. 
-  Thus, the electrons near the top of the valence band have negative effective mass. 
-  Valence band electrons with negative charge and negative mass move in an electric field 
in the same direction as holes with positive charge and positive mass. 
-  Thus, the charge transport in the valence band can be fully accounted for by considering 
hole motion alone. 
-  The electron and hole effective masses are denoted by  and  respectively. 
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Intrinsic Material  
-  A perfect semiconductor crystal with no impurities or lattice defects. 
-  No carriers at 0 K, since the  valence  band  is completely  full and the  conduction band  is 
completely empty. 
-  For  T  >  0  K,  electrons  are  thermally  excited  from  the  valence  band  to  the  conduction 
band (EHP generation). 
-  EHP generation takes place due to breaking of covalent bonds  required energy = . 
-  The excited electron becomes free and leaves behind an empty state (hole). 
-  Since  these  carriers  are  created  in  pairs,  the  electron  concentration  ( )  is  always 
equal to the hole concentration ( ), and each of these is commonly referred to as the 
intrinsic carrier concentration ( ). 
-  Thus, for intrinsic material n = p = . 
-  These carriers are not localized in the lattice; instead they spread out over several lattice 
spacings, and are given by quantum mechanical probability distributions. 
-  Note: ni = f(T). 
-  To  maintain  a  steady-state  carrier  concentration,  the  carriers  must  also  recombine  at the 
same rate at which they are generated. 
-  Recombination  occurs  when  an  electron  from  the  conduction  band  makes  a  transition 
(direct or indirect) to an empty state in the valence band, thus annihilating the pair. 
-  At  equilibrium,   = ,  where  and  are  the  generation  and  recombination  rates 
respectively, and both of these are temperature dependent. 
-  (T) increases with temperature, and a new carrier concentration  ni  is established, such 
that the higher recombination rate  (T) just balances generation. 
-  At  any  temperature,  the  rate  of  recombination  is  proportional  to  the  equilibrium 
concentration  of  electrons  and  holes,  and  can  be  given  by (2.5) 
where   is  a  constant  of  proportionality  (depends  on  the  mechanism  by  which 
recombination takes place). 
Extrinsic Material  
-  In  addition  to  thermally  generated  carriers,  it  is  possible  to  create  carriers  in  the 
semiconductor by purposely introducing impurities into the crystal  doping. 
-  Most common technique for varying the conductivity of semiconductors. 
-  By doping, the crystal can be made to have predominantly electrons (n-type) or holes (p-
type). 
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-  When  a  crystal  is  doped  such  that  the  equilibrium  concentrations  of  electrons  (n0)  and 
holes (p0) are different from the intrinsic carrier concentration (ni), the material is said to 
be extrinsic. 
-  Doping creates additional levels within the band gap. 
-  In  Si,  column  V  elements  of  the  periodic  table  (e.g.,  P,  As,  Sb)  introduce  energy  levels 
very near (typically 0.03-0.06 eV) the conduction band. 
-  At 0 K, these levels are filled with electrons, and very little thermal energy (50 K to 100 
K) is required for these electrons to get excited to the conduction band. 
-  Since  these  levels  donate  electrons  to  the  conduction  band,  they  are  referred  to  as  the 
donor levels. 
-  Thus,  Si  doped  with  donor  impurities  can  have  a  significant  number  of  electrons  in  the 
conduction  band  even  when  the  temperature  is  not  sufficiently  high  enough  for  the 
intrinsic  carriers  to  dominate,  i.e.,  >>  ,  n-type  material,  with  electrons  as 
majority carriers and holes as minority carriers. 
-  In  Si,  column  III  elements  of  the  periodic  table  (e.g.,  B,  Al,  Ga,  In)  introduce  energy 
levels very near (typically 0.03-0.06 eV) the valence band. 
-  At 0 K, these levels are empty, and very little thermal energy (50 K to 100 K) is required 
for electrons in the valence band to get excited to these levels, and leave behind holes in 
the valence band. 
-  Since  these  levels  accept  electrons  from  the  valence  band,  they  are  referred  to  as  the 
acceptor levels. 
-  Thus,  Si  doped  with  acceptor  impurities  can  have  a  significant  number  of  holes  in  the 
valence  band  even  at  a  very  low  temperature,  i.e.,   >>   ,  p-type  material,  with 
holes as majority carriers and electrons as minority carriers. 
-  The  extra  electron  for  column  V  elements  is  loosely  bound  and  it  can  be  liberated  very 
easily ionization; thus, it is free to participate in current conduction. 
-  Similarly,  column  III  elements  create  holes  in  the  valence  band,  and  they  can  also 
participate in current conduction. 
-  Rough calculation of the ionization energy can be made based on the Bohr's model for 
atoms, considering the loosely bound electron orbiting around the tightly bound core 
electrons. Thus, 
 
(2.6)where  is the relative permittivity of Si.  
 
 
EXAMPLE2.2: Calculate the approximate donor binding energy for Si ( r = 11.7,  = 1.18
). 
 
SOLUTION: From Eq.(2.6), we have  
=  1.867  x  J  =  0.117  eV.  
 
Note:  The  effective  mass  used  here  is  an  average  of  the  effective  mass  in  different 
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crystallographic  directions,  and  is  called  the  "conductivity  effective  mass"  with  values  of  1.28
 (at 600 K), 1.18  (at 300 K), 1.08  (at 77 K), and 1.026  (at 4.2 K). 
-  In III-V compounds, column VI impurities (e.g., S, Se, Te) occupying column V sites act 
as  donors.  Similarly,  column  II  impurities  (e.g., Be,  Zn,  Cd)  occupying  column  III  sites 
act as acceptors. 
-  When  a  column  IV  material  (e.g.,  Si,  Ge)  is  used  to  dope  III-V  compounds,  then  they 
may substitute column III elements (and act as donors), or substitute column V elements 
(and act as acceptors) amphoteric dopants. 
-  Doping  creates  a  large  change  in  the  electrical  conductivity,  e.g.,  with  a  doping  of 
, the resistivity of Si changes from 2 x  -cm to 5  -cm.  
 
 
Carrier Concentrations  
-  For the calculation of semiconductor electrical properties and analyzing device behavior, 
it is necessary to know the number of charge carriers/cm3 in the material. 
-  The majority carrier concentration in a heavily doped material is obvious, since for each 
impurity atom, one majority carrier is obtained. 
-  However, the minority carrier concentration and the dependence of carrier concentrations 
on temperature are not obvious. 
-  To obtain the carrier concentrations, their distribution over the available energy states is 
required. 
-  These distributions are calculated using statistical methods.  
The Fermi Level  
-  Electrons in solids obey Fermi-Dirac (FD) statistics. 
-  This statistics accounts for the indistinguishability of the electrons, their wave nature, and 
the Pauli exclusion principle. 
-  The Fermi-Dirac distribution function f(E) of electrons over a range of allowed energy 
levels at thermal equilibrium can be given by  
 
(2.7)where k is Boltzmann's constant (= 8.62 x  eV/K = 1.38 x 
J/K). 
-  This  gives  the  probability  that  an  available  energy  state  at  E  will  be  occupied  by  an 
electron at an absolute temperature T.  
-  is called the Fermi level and is a measure of the average energy of the electrons in the 
lattice an extremely important quantity for analysis of device behavior. 
-  Note: for (E - ) > 3kT (known as Boltzmann approximation), f(E)  exp[- (E-  )/kT] 
this  is  referred  to  as  the  Maxwell-Boltzmann  (MB)  distribution  (followed  by  gas 
atoms). 
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-  The  probability  that  an  energy  state  at  will  be  occupied  by  an  electron  is  1/2  at  all 
temperatures. 
-  At  0  K,  the  distribution  takes  a  simple  rectangular  form,  with  all  states  below 
occupied, and all states above  empty. 
-  At  T  >  0  K,  there  is  a  finite  probability  of  states  above  to  be  occupied  and  states 
below  to be empty. 
-  The F-D distribution function is highly symmetric, i.e., the probability f(  +  ) that a 
state  E  above  is  filled  is  the  same  as  the  probability  [1-  f(   -  )]  that  a  state  E 
below  is empty. 
-  This  symmetry  about  EF  makes  the  Fermi  level  a  natural  reference  point  for  the 
calculation of electron and hole concentrations in the semiconductor. 
-  Note: f(E) is the probability of occupancy of an available state at energy E, thus, if there 
is  no  available  state  at  E  (e.g.,  within  the  band  gap  of  a  semiconductor),  there  is  no 
possibility of finding an electron there. 
-  For  intrinsic  materials,  the  Fermi  level  lies  close  to  the  middle  of  the  band  gap  (the 
difference  between  the  effective  masses  of  electrons  and  holes  accounts  for  this  small 
deviation from the mid gap). 
-  In  n-type  material,  the  electrons  in  the  conduction  band  outnumber  the  holes  in  the 
valence band, thus, the Fermi level lies closer to the conduction band. 
-  Similarly, in p-type material, the holes in the valence band outnumber the electrons in the 
conduction band, thus, the Fermi level lies closer to the valence band. 
-  The probability of occupation f(E) in the conduction band and the probability of vacancy 
[1- f(E)] in the valence band are quite small, however, the densities of available states in 
these  bands  are  very  large,  thus  a  small  change  in  f(E)  can  cause  large  changes  in  the 
carrier concentrations.  
 
 
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Fig.2.4  The  density  of  states  N(E),  the  Fermi-Dirac  distribution  function  f(E),  and  the  carrier 
concentration as functions of energy for (a) intrinsic, (b) n-type, and (c) p-type semiconductors at 
thermal equilibrium.  
-  Note:  since  the  function  f(E)  is  symmetrical  about  ,  a  large  electron  concentration 
implies a small hole concentration, and vice versa. 
-  In  n-type  material,  the  electron  concentration  in  the  conduction  band  increases  as  
moves closer to  ; thus, (  - ) gives a measure of n. 
-  Similarly, in p-type material, the hole concentration in the   valence band increases as  
moves closer to  ; thus, ( - ) gives a measure of p. 
 
Electron and Hole Concentrations at Equilibrium  
-  The  F-D  distribution  function  can  be  used  to  calculate  the  electron  and  hole 
concentrations  in  semiconductors,  if  the  densities  of  available  states  in  the  conduction 
and valence bands are known. 
-  In  equilibrium,  the  concentration  of  electrons  in  the  conduction  band  can  be  given  by 
 
(2.8) 
 
where N(E)dE is the density of available states/cm3 in the energy range dE. 
-  Note:  the  upper  limit  of  is  theoretically  not  proper,  since  the  conduction  band  does  not 
extend  to  infinite  energies;  however,  since  f(E)  decreases  rapidly  with  increasing  E,  the 
contribution to this integral for higher energies is negligible.  
-  Using the solution of  's wave equation under periodic boundary conditions, it 
can  be  shown  that  
 
(2.9)  
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-  Thus,  N(E)  increases  with  E,  however,  f(E)  decreases  rapidly  with  E,  thus,  the  product 
f(E)N(E)  decreases  rapidly  with  E,  and  very  few  electrons  occupy  states  far  above  the 
conduction  band  edge,  i.e.,  most  electrons  occupy  a  narrow  energy  band  near  the 
conduction band edge. 
-  Similarly,  the  probability  of  finding  an  empty  state  in  the  valence  band  [1  -  f(E)] 
decreases  rapidly  below  ,  and  most  holes  occupy  states  near  the  top  of  the  valence 
band. 
-  Thus, a mathematical simplification can be made assuming that all available states in the 
conduction  band  can  be  represented  by  an  effective  density  of  states  NC  located  at  the 
conduction  band  edge  and  using  Boltzmann  approximation.  
 
Thus, (2.10) 
 
where .  
-  Note: as (  -  ) decreases, i.e., the Fermi level moves closer to the conduction band, 
the electron concentration increases.  
-  By similar arguments,  
 
(2.11) 
 
where  is the effective density of states located at the valence band edge  . 
-  Note: the only terms separating the expressions for  and  are the effective masses of 
electrons (  ) and holes (  ) respectively, and since , hence,  . 
-  Thus,  as  (   -  )  decreases,  i.e.,  the  Fermi  level  moves  closer  to  the  valence  band 
edge, and the hole concentration increases. 
-  These equations  for  and  are valid  in  equilibrium,  irrespective of the  material  being 
intrinsic or doped. 
-  For  intrinsic  material  lies  at  an  intrinsic  level  (very  near  the  middle  of  the  band 
gap),  and  the  intrinsic  electron  and  hole  concentrations  are  given  by  
and (2.12)  
-  Note:  At  equilibrium,  the  product  is  a  constant  for  a  particular  material  and 
temperature,  even  though  the  doping  is  varied, 
 
i.e., (2.13) 
-  This equation gives an expression for the intrinsic carrier concentration ni as a function of 
,  , and temperature: 
 
(2.14) 
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-  These relations are extremely important, and are frequently used for calculations. 
-  Note: if  were to be equal to  , then  would have been exactly at mid gap (i.e.,  -
 =  -  = /2). 
-  However,  since  ,  is  displaced  slightly  from  mid  gap  (more  for  GaAs  than  that 
for Si). 
-  Alternate expressions for  and  : 
and (2.15) 
-  Note:  the  electron  concentration  is  equal  to  ni  when  is  at  ,  and  n0  increases 
exponentially as  moves away from  towards the conduction band. 
-  Similarly, the hole concentration  varies from  to larger values as  moves from 
towards the valence band.  
 
 
EXAMPLE 2.3: A Si sample is doped with  B  . What is the equilibrium electron 
concentration  n0  at  300  K?  Where  is  relative  to  ?  Assume  for  Si  at  300  K  =  1.5  x 
 
 
SOLUTION:  Since  B  (trivalent)  is  a  p-type  dopant  in  Si,  hence,  the  material  will  be 
predominantly  p-type,  and  since  >>  , therefore,  will  be  approximately  equal  to ,  and 
=  .  Also, 
.  The  resulting  band  diagram  is: 
 
 
 
Temperature Dependence of Carrier Concentrations  
-  The  intrinsic  carrier  concentration  has  a  strong  temperature  dependence,  given  by 
(2.16) 
-  Thus,  explicitly,  ni  is  proportional  to  T3/2  and  to  e  1/T,  however,  Eg  also  has  a 
temperature  dependence  (decreasing  with  increasing  temperature,  since  the  interatomic 
spacing  changes  with  temperature). 
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Fig.2.5 The intrinsic carrier concentration as a function of inverse temperature for Si, Ge, 
and GaAs. 
-  As  changes with temperature, so do  and  . 
-  With  and  T  given,  the  unknowns  are  the  carrier  concentrations  and  the  Fermi  level 
position with respect to  one of these quantities must be given in order to calculate the 
other. 
-  Example: Si doped with  donors ( ). 
-  At very  low temperature, negligible  intrinsic EHPs exist, and all the donor electrons are 
bound to the donor atoms. 
-  As  temperature  is  raised,  these  electrons  are  gradually  donated  to  the  conduction  band, 
and  at  about  100  K  (1000/T  =  10),  almost  all  these  electrons  are  donated  this 
temperature range is called the ionization region. 
Once all the donor atoms are ionized, the electron concentration  , since for each donor 
atom, one electron is obtained. 
 
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Fig.2.6 Variation of carrier concentration with inverse temperature clearly showing the three 
regions: ionization, extrinsic, and intrinsic. 
-  Thus,  remains  virtually  constant  with  temperature  for  a  wide  range  of  temperature 
(called  the  extrinsic  region),  until  the  intrinsic  carrier  concentration  ni  starts  to  become 
comparable to  . 
-  For  high  temperatures,  >>  ,  and  the  material  loses  its  extrinsic  property  (called  the 
intrinsic region). 
-  Note: in the intrinsic region, the device loses its usefulness => determines the maximum 
operable temperature range.  
Compensation and Space Charge Neutrality  
-  Semiconductors can be doped with both donors ( ) and acceptors ( ) simultaneously. 
-  Assume a material doped with  >  predominantly n-type  lies above 
acceptor  level  Ea  completely  full,  however,  with  above  ,  the  hole  concentration 
cannot be equal to  . 
-  Mechanism: 
o  Electrons are donated to the conduction band from the donor level   
o  An acceptor state gets filled by a valence band electron, thus creating a hole in the 
valence band. 
o  An electron from the conduction band recombines with this hole. 
o  Extending this logic, it is expected that the resultant concentration of electrons in 
the conduction band would be  instead of  . 
o  This process is called compensation. 
-  By compensation, an n-type material can be made intrinsic (by making  =  ) or even 
p-type (for  > ). 
 
Note: a semiconductor is neutral to start with, and, even after doping, it remains neutral 
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(since for all donated electrons, there are positively charged ions ( ); and for all 
accepted electrons (or holes in the valence band), there are negatively charged ions ( ).  
-  Therefore, the sum of positive charges  must equal the sum of  negative charges, and this 
governing  relation,  
given by  (2.17) is referred to as the equation for space charge neutrality. 
-  This  equation,  solved  simultaneously  with  the  law  of  mass  action  (given  by  ) 
gives  the  information  about  the  carrier  concentrations. 
Note: for ,  
Drift of Carriers in Electric and Magnetic Fields  
-  In  addition  to  the  knowledge  of  carrier  concentrations,  the  collisions  of  the  charge 
carriers  with  the  lattice  and  with  the  impurity  atoms  (or  ions)  under  electric  and/or 
magnetic  fields  must be accounted for, in order to compute the current flow through the 
device. 
-  These processes will affect the ease (mobility) with which carriers move within a lattice. 
-  These  collision  and  scattering  processes  depend  on  temperature,  which  affects  the 
thermal motion of the lattice atoms and the velocity of the carriers.  
Conductivity and Mobility  
-  Even at thermal equilibrium, the carriers are in a constant motion within the lattice.  
-  At room temperature, the thermal  motion of an  individual electron  may  be  visualized as 
random scattering from lattice atoms, impurities, other electrons, and defects. 
-  There  is  no  net  motion  of  the  group of  n  electrons/cm3  over  any  period  of 
time, since the scattering is random, and there is no preferred direction of motion for the 
group of electrons and no net current flow. 
-  However,  for  an  individual  electron,  this  is  not  true  the  probability  of  an  electron 
returning to its starting point after time t is negligibly small. 
-  Now, if an electric  field  is applied  in the  x-direction, each electron  experiences a  net 
force q  from the field. 
-  This  will  create  a  net  motion  of  group  in  the  x-direction,  even  though  the  force  may  be 
insufficient to appreciably alter the random path of an individual electron. 
-  If  is the x-component of the total momentum of the group, then the force of the field on 
the n  is 
(2.18) 
 
Note: this expression indicates a constant acceleration in the x-direction, which 
realistically cannot happen. 
-  In steady state, this acceleration is just balanced by the deceleration due to the collisions. 
-  Thus,  while  the  steady  field  does  produce  a  net  momentum  ,  for  steady  state 
current  flow,  the  net  rate  of  change  of  momentum  must  be  zero  when  collisions  are 
included. 
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-  Note:  the  collision  processes  are  totally  random,  thus,  there  is  a  constant  probability  of 
collision at any time for each electron. 
-  Consider a group of  electrons at time t = 0, and define N(t) as the number of electrons 
that have not undergone a collision by time t 
 
 
Fig.2.7 The random thermal motion of an individual electron, undergoing random 
scattering.  
-  The rate of decrease of N(t) at any time t is proportional to the number left unscattered at 
t,  i.e. 
 
(2.19) 
 
where  is the constant of proportionality. 
-  The solution is an exponential function 
(2.20) 
 
and  represents the mean time between scattering events, called the mean free time. 
-  The probability that any electron has a collision in time interval dt is dt/  , thus, the 
differential change in  due to collisions in time dt is 
(2.21) 
-  Thus,  the  rate  of  change  of  due  to  the  decelerating  effect  of  collisions  is 
(2.22) 
-  For  steady  state,  the  sum  of  acceleration  and  deceleration  effects  must  be  zero,  thus, 
(2.23) 
-  The  average  momentum  per  electron  (averaged  over  the  entire  group  of  electrons)  is 
(2.24) 
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-  Thus, as expected for steady state, the electrons would have on the average a constant net 
velocity in the -x-direction 
(2.25) 
-  This speed is referred to as the drift speed, and, in general, it is usually much smaller than 
the random speed due to thermal motion  . 
-  The current density resulting from this drift 
(2.26) 
-  This is the familiar Ohm's law with  being the conductivity of the sample, which 
can  also  be  written  as  ,  with is  defined  as  the  electron  mobility 
(in  ),  and  it  describes  the  ease  with  which  electrons  drift  in  the  material. 
 
-  The  mobility  can  also  be  expressed  as  the  average  drift  velocity  per  unit  electric  field, 
thus  with  the  negative  sign  denoting  a  positive  value  for  mobility  since 
electrons drift opposite to the direction of the electric field. 
-  The  total  current  density  can  be  given  by  (2.27)  when  both  electrons 
and  holes  contribute  to the  current  conduction;  on  the  other  hand,  for  predominantly  n-
type  or  p-type  samples,  respectively  the  first  or  the  second  term  of  the  above  equation 
dominates. 
 
Note:  both  electron  and  hole  drift  currents  are  in  the  same  direction,  since  holes  (with 
positive  charges)  move  along  the  direction  of  the  electric  field,  and  electrons  (with 
negative charges) drift opposite to the direction of the electric field. 
-  Since  GaAs  has  a  strong  curvature  of  the  E-k  diagram  at  the  bottom  of  the  conduction 
band, the electron effective mass in GaAs is very small  the electron mobility in GaAs 
is very high since  is inversely proportional to  . 
-  The  other  parameter  in  the  mobility  expression,  i.e.,  (the  mean  free  time  between 
collisions)  is  a  function  of  temperature  and  the  impurity  concentration  in  the 
semiconductor. 
-  For  a  uniformly  doped  semiconductor  bar  of  length  L,  width  w,  and  thickness  t,  the 
resistance R of the bar can be given by  where  is the resistivity.  
 
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Effects of Temperature and Doping on Mobility  
-  The  two  main  scattering  events  that  influence  electron  and  hole  motion  (and,  thus, 
mobility) are the lattice scattering and the impurity scattering. 
-  All lattice atoms vibrate due to temperature and can scatter carriers due to collisions. 
-  These  collective  vibrations  are  called  phonons,  thus  lattice  scattering  is  also  known  as 
phonon scattering. 
-  With increasing temperature, lattice vibrations increase, and the mean free time between 
collisions decreases  mobility decreases (typical dependence  ). 
-  Scattering from crystal defects and ionized impurities dominate at low temperatures. 
-  Since  carriers  moving  with  low  velocity  (at  low  temperature)  can  get  scattered  more 
easily  by  ionized  impurities, this kind of scattering causes a decrease  in  carrier  mobility 
with decreasing temperature (typical dependence  ). 
-  Note:  the  scattering  probability  is  inversely  proportional  to  the  mean  free  time  (and  to 
mobility),  hence,  the  mobilities  due  to  two  or  more  scattering  events  add  inversely: 
(2.28) 
-  Thus, the mechanism causing the lowest mobility value dominates. 
-  Mobility  also  decreases  with  increasing  doping,  since  the  ionized  impurities  scatter 
carriers  more  (e.g.,  for  intrinsic  Si  is  1350  at  300  K,  whereas  with  a  donor 
doping of  , n drops to 700  ).  
High Field Effects  
-  For  small  electric  fields,  the  drift  current  increases  linearly  with  the  electric  field,  since 
is a constant. 
-  However,  for  large  electric  fields  (typically  >  ),  the  current  starts  to  show  a 
sublinear dependence on the electric field and eventually saturates for very high fields.  
-  Thus, becomes a function of the electric field, and this is known as the hot carrier effect, 
when the carrier drift velocity becomes comparable to its thermal velocity. 
-  The  maximum  carrier  drift  velocity  is  limited  to  its  mean  thermal  velocity  (typically 
), beyond which the added energy imparted by the electric field is absorbed by 
the lattice (thus generating heat) instead of a corresponding increase in the drift velocity.  
2.4.4 The Hall Effect  
-  An extremely important measurement procedure for determining the majority carrier 
concentration and mobility. 
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Fig.2.8 The experimental setup for the Hall Effect measurement. 
-  If a magnetic field is applied perpendicular to the direction of carrier flow, the path of the 
carriers get deflected due to the Lorentz force experienced  by the carriers, which can  be 
given  by 
F = q(E + v x B) (2.29) 
-  Thus, the holes will get deflected towards the  -y-direction, and establish an electric field 
along the y-direction, such that in steady state   
-  The  establishment  of  this  electric  field  is  known  as  the  Hall  effect,  and  the  resulting 
voltage  is called the Hall voltage. 
-  Using  the  expression  for  the  drift  current,  is  called  the 
Hall coefficient. 
-  A  measurement  of  the  Hall  voltage  along  with  the  information  for  magnetic  field  and 
current density gives the majority carrier concentration   
-  Also,  the  majority  carrier  mobility  can  be  obtained  from  a  measurement  of 
the resistivity   
-  This  experiment  can  be  performed  to  obtain  the  variation  of  majority  carrier 
concentration and mobility as a function of temperature. 
-  For n-type samples, the Hall  voltage and the Hall coefficient are negative  a common 
diagnostic tool for obtaining the sample type. 
-  Note: caution should be exercised for near intrinsic samples.  
 
 
EXAMPLE  2.4:  A  sample  of  Si  is  doped  with  In  .  What  will  be  the  measured 
value  of  its  resistivity?  What  is  the  expected  Hall  voltage  in  a  150  m  thick  sample  if 
? 
 
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SOLUTION:  
 
 
 
Equilibrium Condition 
-  In  equilibrium,  there  is  no  external  excitation  except  a  constant  temperature,  no  net 
transfer of energy, no net carrier motion, and no net current transport. 
-  An important condition for equilibrium is that no discontinuity or gradient can arise in the 
equilibrium Fermi level EF. 
-  Assume  two  materials  1  and  2  (e.g.,  n-  and  p-type  regions,  dissimilar  semiconductors, 
metal and semiconductor, two adjacent regions in a nonuniformly doped semiconductor) 
in intimate contact such that electron can move between them. 
-  Assume materials 1 and 2 have densities of state N1(E) and N2(E), and F-D distribution 
functions  f1(E)  and  f2(E)  respectively  at  any  energy  E. 
 
 
-  The  rate  of  electron  motion  from  1  to  2  can  be  given  byrate  from  1  to  2  N1(E)f1(E)  . 
N2(E)[1 f2(E)] (2.30)and the rate of electron motion from 2 to 1 can be given byrate from 
2 to 1 N2(E)f2(E) . N1(E)[1 f1(E)] (2.31)" At equilibrium, these two rates must be equal, 
which gives f1(E) = f2(E) => EF1 = EF2 => dEF/dx = 0; thus, the Fermi level is constant 
at  equilibrium,  or,  in  other  words,  there  cannot  be  any  discontinuity  or  gradient  in  the 
Fermi level at equilibrium.  
 
Practice Problems  
2.1  Electrons  move  in  a  crystal  as  wave  packets  with  a  group  velocity  where 
is the angular  frequency. Show that in a given electric  field, these wave packets obey 
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Newton's second  law of  motion,  i.e., the  force F  =  m*a, where  m*  is the  effective  mass 
and a is the acceleration.  
2.2 Some semiconductors of interest have the dependence of its energy E with respect to 
the wave vector k, given by  is the effective mass for E = 
0,  k  is  the  wave  vector,  and  is  a  constant.  Calculate  the  dependence  of  the  effective 
mass  on energy. 
2.3  Determine  the  equilibrium  recombination  constant  r  for  Si  and  GaAs,  having 
equilibrium  thermal  generation  rates  of 
respectively, and  intrinsic carrier concentrations of 
respectively. Comment on the answers. Will  change with doping at equilibrium? 
2.4  The  relative  dielectric  constant  for  GaP  is  10.2  and  the  electron  effective  mass  is 
Calculate the approximate ionization energy of a donor atom in GaP. 
2.5 Show that the probability that a state  above the Fermi level  is occupied is the 
same as the probability that a state  below  is empty. 
2.6 Derive an expression relating the intrinsic level  to the center of the band gap 
and  compute  the  magnitude  of  this  displacement  for  Si  and  GaAs  at  300  K.  Assume 
respectively. 
2.7  Show  that  in  order  to  obtain  maximum  resistivity  in  a  GaAs  sample 
it  has  to  be 
doped slightly p-type. Determine this doping  concentration.  Also, determine the ratio of 
the maximum resistivity to the intrinsic resistivity. 
2.8  A  GaAs  sample  (use  the  date  given  in  Problem  2.7)  is  doped  uniformly  with 
out of  which  70%  occupy  Ga  sites,  and  the  rest  30%  occupy  As  sites. 
Assume  100%  ionization  and  T  =  300  K. 
a)  Calculate  the  equilibrium  electron  and  hole  concentrations   
b)  Clearly  draw  the  equilibrium  band  diagram,  showing  the  position  of  the  Fermi  level 
with  respect  to  the  intrinsic  level  ,  assuming  that  lies  exactly  at  midgap. 
c)  Calculate  the  percentage  change  in  conductivity  after  doping  as  compared  to  the 
intrinsic case. 
2.9 A Si sample is doped with  donor atoms. Determine the minimum 
temperature at which the sample becomes intrinsic. Assume that at this minimum 
temperature, the free electron concentration does not exceed by more than 1% of the 
donor concentration (beyond its extrinsic value). For 
 
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2.10 Since the event of collision of an electron in a lattice is a truly random process, thus 
having  a constant probability of collision  at any  given time, the  number of particles  left 
unscattered  at  time  t, 
Hence,  show  that  if  there  are  a  total  of  i  number  of  scattering  events,  each  with  a  mean 
free time of  then the net electron mobility  can be given by  where 
is the mobility due to the ith scattering event. 
2.11  A  Ge  sample  is  oriented  in  a  magnetic  field  (refer  to 
Fig.2.8).  The  current  is  4  mA,  and  the  sample  dimensions  are  w  =  0.25  mm,   
t  =  50  m,  and  L  =  2.5  mm.  The  following  data  are  taken: 
Find  the  type  and  concentration  of  the  majority 
carrier, and its mobility. Hence, compute the net relaxation time for the various scattering 
events, assuming   
2.12 In the Hall effect experiment, there is a chance that the Hall Probes A and B (refer to 
Fig.2.8) are not perfectly aligned, which may give erroneous Hall voltage readings. Show 
that  the  true  Hall  voltage   can  be  obtained  from  two  measurements  of  with  the 
magnetic field first in the +z-direction, and then in the z-direction. 
 
 
Metals 
 
or  
 
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In metals, either the conduction band is partially filled or overlaps with valence band. There is no 
forbidden  energy  gap  in  between.  Even  if  a  small  electric  field  is  applied,  free  electrons  start 
moving in a direction opposite to field and hence a good conductor of electricity.  
Insulators 
Here  the  valency  bands  are  completely  filled  and  conduction  band  is  empty  and  the  forbidden 
gap  is  quite  large.  For  example  in  diamond  E
gap
  is  6eV.  Even  if  an  electric  field  is  applied,  no 
electron is able to go from valence band to conduction band. 
Semiconductors 
The valence band is completely filled and conduction band is empty. The E
gap
 is also less i.e., of 
the  order  of  few  eV.  At  zero  kelvin,  electrons  are  not  able  to  cross  this  forbidden  gap  and  so 
behave  like  insulators.  But  as  temperature  is  increased,  electrons  in  valence  band  (VB)  gain 
thermal  energy  and  jump  to  conduction  band  (CB)  and  acquire  small  conductivity  at  room 
temperature and so behave like conductors. Hence they are called semiconductors. 
 
Charge carriers in semiconductors 
At  high  temperature,  electrons  move  from  valance  band  to  conduction  band  and  as  a  result  a 
vacancy is created in the valence band at a place where an electron was present before shifting to 
conduction  band. The  valency  is a  hole and  is seat of positive charge  having the  same  value of 
electron. Therefore the electrical  conduction  in  semiconductors is due to motion of electrons  in 
conduction band and also due to motion of holes in valence band. 
 
 
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Semiconductor Basics 
If  Resistors  are  the  most  basic  passive  component  in  electrical  or  electronic  circuits,  then  we 
have to consider the Signal Diode as being the most basic "Active" component. However, unlike 
a  resistor,  a  diode  does  not  behave  linearly  with  respect  to  the  applied  voltage  as  it  has  an 
exponential I-V relationship and therefore can not be described simply by using Ohm's law as we 
do for resistors. Diodes are unidirectional  semiconductor devices that will only allow current to 
flow through them  in one direction only, acting  more  like  a one way electrical  valve, (Forward 
Biased Condition). But, before we have a look at how signal or power diodes work we first need 
to understand their basic construction and concept. 
Diodes are made from a single piece of Semiconductor material which has a positive "P-region" 
at one end  and a  negative "N-region" at the other, and which  has a resistivity  value  somewhere 
between  that  of  a  conductor  and  an  insulator.  But  what  is  a  "Semiconductor"  material?,  firstly 
let's look at what makes something either a Conductor or an Insulator. 
Resistivity 
The electrical Resistance of an electrical or electronic component or device is generally defined 
as  being  the  ratio  of  the  voltage  difference  across  it  to  the  current  flowing  through  it,  basic 
Ohms  Law  principals.  The  problem  with  using  resistance  as  a  measurement  is  that  it  depends 
very  much  on  the  physical  size  of  the  material  being  measured  as  well  as  the  material  out  of 
which  it  is  made.  For  example,  If  we  were  to  increase  the  length  of  the  material  (making  it 
longer)  its  resistance  would  also  increase.  Likewise,  if  we  increased  its  diameter  (making  it 
fatter) its resistance would then decrease. So we  want to be able to define the material in such a 
way as to indicate its ability to either conduct or oppose the flow of electrical current through it 
no matter what its size or shape happens to be. The quantity that is used to indicate this specific 
resistance  is  called  Resistivity  and  is  given  the  Greek  symbol  of  ,  (Rho).  Resistivity  is 
measured in Ohm-metres, ( -m ) and is the inverse to conductivity. 
If the resistivity of various materials is compared, they can be classified into three main groups, 
Conductors, Insulators and Semi-conductors as shown below. 
 
 
 
 
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Resistivity Chart 
 
    
Notice  also  that  there  is  a  very  small 
margin  between  the  resistivity  of  the 
conductors  such  as  silver  and  gold, 
compared to a much  larger  margin  for 
the  resistivity  of  the  insulators 
between  glass  and  quartz.  The 
resistivity  of  all  the  materials  at  any 
one  time  also  depends  upon  their 
temperature. 
Conductors 
From  above  we  now  know  that  Conductors  are  materials  that  have  a  low  value  of  resistivity 
allowing  them  to  easily  pass  an  electrical  current  due  to  there  being  plenty  of  free  electrons 
floating  about  within  their  basic  atom  structure. When  a  positive  voltage  potential  is  applied  to 
the  material  these  "free  electrons"  leave  their  parent  atom  and  travel  together  through  the 
material  forming  an  electron  drift.  Examples  of  good  conductors  are  generally  metals  such  as 
Copper, Aluminium, Silver or non metals such as Carbon because these materials have very few 
electrons in their outer "Valence Shell" or ring, resulting in them being easily knocked out of the 
atom's  orbit.  This  allows  them  to  flow  freely  through  the  material  until  they  join  up  with  other 
atoms, producing a "Domino Effect" through the material thereby creating an electrical current. 
Generally  speaking,  most  metals  are  good  conductors  of  electricity,  as  they  have  very  small 
resistance  values,  usually  in  the  region  of  micro-ohms  per  metre  with  the  resistivity  of 
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conductors  increasing  with  temperature  because  metals  are  also  generally  good  conductors  of 
heat. 
Insulators 
Insulators  on  the  other  hand  are  the  exact  opposite  of  conductors.  They  are  made  of  materials, 
generally non-metals, that have very few or no "free electrons" floating about within their basic 
atom  structure  because  the  electrons  in  the  outer  valence  shell  are  strongly  attracted  by  the 
positively  charged  inner  nucleus.  So  if  a  potential  voltage  is  applied  to  the  material  no  current 
will  flow  as  there  are  no  electrons  to  move  and  which  gives  these  materials  their  insulating 
properties.  Insulators  also  have  very  high  resistances,  millions  of  ohms  per  metre,  and  are 
generally not affected by normal temperature changes (although at very high temperatures wood 
becomes  charcoal  and  changes  from  an  insulator  to  a  conductor).  Examples  of  good  insulators 
are marble, fused quartz, p.v.c. plastics, rubber etc. 
Insulators  play  a  very  important  role  within  electrical  and  electronic  circuits,  because  without 
them electrical circuits would short together and not work. For example, insulators made of glass 
or  porcelain  are  used  for  insulating  and  supporting  overhead  transmission  cables  while  epoxy-
glass resin materials are used to make printed circuit boards, PCB's etc. 
Semiconductor Basics 
Semiconductors  materials  such  as  silicon  (Si),  germanium  (Ge)  and  gallium  arsenide  (GaAs), 
have  electrical  properties  somewhere  in  the  middle,  between  those  of  a  "conductor"  and  an 
"insulator".  They  are  not  good  conductors  nor  good  insulators  (hence  their  name  "semi"-
conductors).  They  have  very  few  "fee  electrons"  because  their  atoms  are  closely  grouped 
together  in  a  crystalline  pattern  called  a  "crystal  lattice".  However,  their  ability  to  conduct 
electricity  can  be  greatly  improved  by  adding  certain  "impurities"  to  this  crystalline  structure 
thereby,  producing  more  free  electrons  than  holes  or  vice  versa.  By  controlling  the  amount  of 
impurities  added  to  the  semiconductor  material  it  is  possible  to  control  its  conductivity.  These 
impurities are called donors or acceptors depending on whether they produce electrons or holes. 
This process of adding impurity atoms to semiconductor atoms (the order of 1 impurity atom per 
10 million (or more) atoms of the semiconductor) is called Doping. 
The most commonly used semiconductor material by far is  silicon. It has four valence electrons 
in  its  outer  most  shell  which  it  shares  with  its  adjacent  atoms  in  forming  covalent  bonds.  The 
structure of the bond between two silicon atoms is such that each atom shares one electron with 
its neighbour making the bond very stable. As there are very few free electrons available to move 
from  place  to  place  producing  an  electrical  current,  crystals  of  pure  silicon  (or  germanium)  are 
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therefore  good  insulators,  or  at  the  very  least  very  high  value  resistors.  Silicon  atoms  are 
arranged in a definite symmetrical pattern making them a crystalline solid structure. A crystal of 
pure  silicon  (silicon  dioxide  or  glass)  is  generally  said  to  be  an  intrinsic  crystal  (it  has  no 
impurities). 
 
 
The  diagram  above  shows  the  structure  and  lattice  of  a  'normal'  pure  crystal 
of Silicon. 
N-type Semiconductor Basics 
In order for our silicon crystal to conduct electricity, we need to introduce an impurity atom such 
as Arsenic, Antimony or Phosphorus into the crystalline structure making it extrinsic (impurities 
are added). These atoms have five outer electrons in their outermost co-valent bond to share with 
other  atoms  and  are  commonly  called  "Pentavalent"  impurities.  This  allows  four  of  the  five 
electrons to bond with its neighbouring silicon atoms leaving one "free electron" to move about 
when  an  electrical  voltage  is  applied  (electron  flow).  As  each  impurity  atom  "donates"  one 
electron, pentavalent atoms are generally known as "donors". 
Antimony  (symbol  Sb)  is  frequently  used  as  a  pentavalent  additive  as  it  has  51  electrons 
arranged  in  5  shells  around  the  nucleus.  The  resulting  semiconductor  material  has  an  excess  of 
current-carrying electrons, each with a  negative charge, and  is therefore referred to as "N-type" 
material with the electrons called "Majority Carriers" and the resultant holes "Minority Carriers". 
Then  a  semiconductor  material  is  N-type  when  its  donor  density  is  greater  than  its  acceptor 
density. Therefore, a N-type semiconductor has more electrons than holes. 
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The diagram above shows the structure and lattice of the donor impurity atom 
Antimony. 
P-Type Semiconductor Basics 
If  we  go  the  other  way,  and  introduce  a  "Trivalent"  (3-electron)  impurity  into  the  crystal 
structure, such as Aluminium, Boron or Indium, only three valence electrons are available in the 
outermost covalent bond meaning that the fourth bond cannot be formed. Therefore, a complete 
connection is not possible, giving the semiconductor material an abundance of positively charged 
carriers  known  as  "holes"  in  the  structure  of  the  crystal.  As  there  is  a  hole  an  adjoining  free 
electron is attracted to it and will try to move into the hole to fill it. However, the electron filling 
the hole leaves another hole behind it as it moves. This in turn attracts another electron which in 
turn creates another hole behind, and so forth giving the appearance that the holes are moving as 
a  positive  charge  through  the  crystal  structure  (conventional  current  flow).  As  each  impurity 
atom  generates  a  hole,  trivalent  impurities  are  generally  known  as  "Acceptors"  as  they  are 
continually "accepting" extra electrons. 
Boron (symbol B) is frequently used as a trivalent additive as it has only 5 electrons arranged in 
3  shells  around  the  nucleus.  Addition  of  Boron  causes  conduction  to  consist  mainly  of  positive 
charge carriers results in a "P-type" material and the positive holes are called "Majority Carriers" 
while the free electrons are called "Minority Carriers". Then a semiconductors is P-type when its 
acceptor  density  is  greater  than  its  donor  density.  Therefore,  a  P-type  semiconductor  has  more 
holes than electrons. 
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The  diagram  above  shows  the  structure  and  lattice  of  the  acceptor  impurity 
atom Boron. 
Semiconductor Basics Summary 
N-type (e.g. add Antimony) 
These  are  materials  which  have  Pentavalent  impurity  atoms  (Donors)  added  and  conduct  by 
"electron" movement and are called, N-type Semiconductors. 
In these types of materials are: 
-  1. The Donors are positively charged. 
-  2. There are a large number of free electrons. 
-  3. A small number of holes in relation to the number of free electrons. 
-  4. Doping gives:  
o    positively charged donors. 
o    negatively charged free electrons. 
-  5. Supply of energy gives:  
o    negatively charged free electrons. 
o    positively charged holes. 
P-type (e.g. add Boron) 
These  are  materials  which  have  Trivalent  impurity  atoms  (Acceptors)  added  and  conduct  by 
"hole" movement and are called, P-type Semiconductors. 
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In these types of materials are: 
-  1. The Acceptors are negatively charged. 
-  2. There are a large number of holes. 
-  3. A small number of free electrons in relation to the number of holes. 
-  4. Doping gives:  
o    negatively charged acceptors. 
o    positively charged holes. 
-  5. Supply of energy gives:  
o    positively charged holes. 
o    negatively charged free electrons. 
and both P and N-types as a whole, are electrically neutral. 
In  the  next  tutorial  about  semiconductors  and  diodes,  we  will  look  at  joining  the  two 
semiconductor materials, the P-type and the N-type materials to form a PN Junction which can 
be used to produce diodes. 
Pn junction 
The PN junction 
In the previous tutorial we saw how to make an N-type semiconductor material by doping it with 
Antimony  and  also  how  to  make  a  P-type  semiconductor  material  by  doping  that  with  Boron. 
This is all well and good, but these semiconductor  N and P-type materials do very little on their 
own as they are electrically neutral, but when we join (or fuse) them together these two materials 
behave in a very different way producing what is generally known as a PN Junction. 
When  the  N  and  P-type  semiconductor  materials  are  first  joined  together  a  very  large  density 
gradient  exists  between  both  sides  of  the  junction  so  some  of  the  free  electrons  from  the  donor 
impurity atoms  begin to migrate across this newly  formed  junction to fill up the  holes  in the  P-
type  material  producing  negative  ions.  However,  because  the  electrons  have  moved  across  the 
junction from the N-type silicon to the P-type silicon, they leave behind positively charged donor 
ions (N
D
) on the negative side and  now the holes  from the acceptor impurity  migrate across the 
junction in the opposite direction into the region were there are large numbers of free electrons. 
As a result, the charge density of the P-type along the junction is filled with negatively charged 
acceptor  ions  (N
A
),  and  the  charge  density  of  the  N-type  along  the  junction  becomes  positive. 
This charge transfer of electrons and holes across the junction is known as diffusion. 
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This  process  continues  back  and  forth  until  the  number  of  electrons  which  have  crossed  the 
junction  have  a  large  enough  electrical  charge  to  repel  or  prevent  any  more  carriers  from 
crossing  the  junction.  The  regions  on  both  sides  of  the  junction  become  depleted  of  any  free 
carriers  in comparison to the N and P type  materials away  from the  junction. Eventually a state 
of  equilibrium  (electrically  neutral  situation)  will  occur  producing  a  "potential  barrier"  zone 
around the area of the  junction as the donor atoms repel the  holes and the acceptor atoms repel 
the electrons. Since no free charge carriers can rest in a position where there is a potential barrier 
the  regions  on  both  sides  of  the  junction  become  depleted  of  any  more  free  carriers  in 
comparison to the N and P type materials away from the junction. This area around the junction 
is now called the Depletion Layer. 
The PN junction 
 
 
The  total  charge  on  each  side  of  the  junction  must  be  equal  and  opposite  to  maintain  a  neutral 
charge condition around the junction. If the depletion  layer region has a distance D,  it therefore 
must therefore penetrate into the silicon by a distance of Dp for the positive side, and a distance 
of Dn for the negative side giving a relationship between the two of   Dp.N
A
 = Dn.N
D
  in order to 
maintain charge neutrality also called equilibrium. 
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PN junction Distance 
 
As the N-type  material  has  lost electrons and the  P-type  has  lost holes, the N-type  material  has 
become positive with respect to the P-type. Then the presence of impurity ions on both sides of 
the  junction  cause  an  electric  field  to  be  established  across  this  region  with  the  N-side  at  a 
positive voltage relative to the P-side. The problem now is that a free charge requires some extra 
energy  to  overcome  the  barrier  that  now  exists  for  it  to  be  able  to  cross  the  depletion  region 
junction. 
 
This  electric  field  created  by  the  diffusion  process  has  created  a  "built-in  potential  difference" 
across the junction with an open-circuit (zero bias) potential of: 
 
Where:  E
o
  is  the  zero  bias  junction  voltage,  V
T
  the  thermal  voltage  of  26mV  at  room 
temperature, N
D
 and N
A
 are the impurity concentrations and n
i
 is the intrinsic concentration. 
A  suitable positive  voltage (forward bias) applied between the two ends of the PN  junction  can 
supply  the  free  electrons  and  holes  with  the  extra  energy.  The  external  voltage  required  to 
overcome  this  potential  barrier  that  now  exists  is  very  much  dependent  upon  the  type  of 
semiconductor  material  used  and  its  actual  temperature.  Typically  at  room  temperature  the 
voltage across the depletion layer for silicon is about 0.6  - 0.7 volts and for germanium is about 
0.3 - 0.35 volts. This potential barrier will always exist even if the device is not connected to any 
external power source. 
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The significance of this  built-in potential across the  junction,  is that  it opposes both the flow of 
holes and electrons across the junction and is why it is called the potential barrier. In practice, a 
PN junction is formed within a single crystal of material rather than just simply joining or fusing 
together two separate pieces. Electrical  contacts are also  fused onto either side of the crystal to 
enable an electrical  connection to be  made to an  external circuit. Then the resulting device that 
has been made is called a PN junction Diode or Signal Diode. 
In the next tutorial about the PN junction, we will look at one of the most interesting aspects of 
the PN junction is its use in circuits as a diode. By adding connections to each end of the P-type 
and  the  N-type  materials  we  can  produce  a  two  terminal  device  called  a  PN  Junction  Diode 
which can be biased by an external voltage to either block or allow the flow of current through it. 
 
Introduction to depletion layer pn junction: 
If one side of crystal pure  semiconductor Si(silicon) or Ge(Germanium)  is doped with acceptor 
impurity atoms and the other side is doped with donor impurity atoms , a PN junction is formed 
as shown in figure.P region has high concentration of holes and N region contains large number 
of electrons. 
What is Depletion Layer of Pn Junction? 
As  soon  as  the  junction  is  formed,  free  electrons  and  holes  cross  through  the  junction  by  the 
process of diffusion.During this process , the electrons crossing the junction from N- region into 
P-region  ,  recombine  with  holes  in  the  P-region  very  close  to  the  junction.Similarly  holes 
crossing  the  junction  from  the  P-region  into  the  N-region,  recombine  with  electrons  in  the  N-
region  very  close  to  the  junction.  Thus  a  region  is  formed,  which  does  not  have  any  mobile 
charge very close to the junction. This region is called the depletion layer of pn junction. 
 
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In this region, on the  left side of the  junction, the acceptor atoms  become  negative  ions and on 
the right side of the junction, the donor atoms become positive ions as shown in figure.  
Function of Depletion Layer of Pn Junction : 
An electric  field  is set up, between the donor and acceptor ions  in the depletion  layer of the pn 
junction .The potential at the N-side  is higher than the potential at P-side.Therefore electrons  in 
the N- side are prevented to go to the lower potential of P-side. Similarly, holes in the P-side find 
themselves at a lower potential and are prevented to cross to the N-side. Thus, there is a barrier at 
the  junction  which  opposes  the  movement  of  the  majority  charge  carriers.  The  difference  of 
potential  from  one  side  of  the  barrier  to  the  other  side  of  the  barrier   is  called  potential 
barrier.The  potential  barrier  is  approximately  0.7V  for  a  silicon  PN  junction  and  0.3V  for 
germanium PN junction. The distance from one side of the barrier to the other side is called the 
width of the barrier, which depends on the nature of the material. 
Introduction to Diodes and Transistors: 
Diodes  are  known  as  p-n  junction  in  the  physics  or  in  most  of  the  basic  sciences  but  in  the 
electronics and engineering  sciences a p-n  junction  has the abbreviated  name  i.e. diode. Diodes 
are  the  electrical  component  of  any  electric  circuit  which  prevents  the  circuit  from  the  high 
electric  current  because  diodes  are  get  break  i.e.  they  get  burn  when  a  large  current  is  flowing 
through them and hence prevents the electrical circuits. 
Transistors are the electrical device which  mainly consists of two junctions thus they are called 
as the  junction transistors. The transistors have three terminals  instead of the two terminals  and 
each  terminal  has  its  specific  characteristics.  In  electronic  circuits  two transistors  namely  n-p-n 
and p-n-p are most preferably used. 
More about Diodes and Transistors: 
When a p-type semiconductor is brought into a close contact with an n-type semiconductor, then 
the resultant arrangement is called a p-n junction or a junction diode or simply a diode. 
A  junction  transistor  is  obtained  by  growing  a  thin  layer  of  one  semiconductor  in  between  two 
thick  layers  of  other  similar  type  semiconductor.  Thus  a  junction  transistor  is  a  semiconductor 
device having two junctions and three terminals. 
Example of Diodes and Transistors: 
Junction diodes are of many types. Important among them are: 
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(a)     Zener  diode:  A  zener  diode  is  specially  designed  junction  diode  which  can  operate 
continuously without being damaged in the region of reverse break down voltage shown in  Fig.1. 
(b)   Photo diode: Its working is based on the electric conduction from light shown in Fig.2. 
(c)    Light emitting diode (LED): Its working is based on the production of light from electric 
current shown in Fig.3. 
                                                             
    Fig.1 Zener Diode                             Fig.2 Photo Diode                                      Fig.3 LED 
The transistors are also of several types but most important among them are listed below: 
(a)     Junction  Transistors:  These  are  of  two  kind  p-n-p  and  n-p-n  and  they  are  basic  transistors 
which are used in the electronic circuitry and other electronic equipment very rapidly because of 
there low cost and high reliability. 
(b)    Field  effect  transistors:  In  present  days  most  of  the  electronic  integrated  circuits  are  using 
these  kinds  of  transistors  because  they  are  highly  conductive  and  easy  to  prepare  then  the 
junction transistor. 
The Junction Diode 
 
The Junction Diode 
The  effect  described  in  the  previous  tutorial  is  achieved  without  any  external  voltage  being 
applied  to  the  actual  PN  junction  resulting  in  the  junction  being  in  a  state  of  equilibrium. 
However, if we were to make electrical connections at the ends of both the N-type and the P-type 
materials  and  then  connect them  to  a  battery  source,  an  additional  energy  source  now  exists  to 
overcome the barrier resulting  in  free charges  being able to cross the depletion region  from one 
side  to  the  other.  The  behaviour  of  the  PN  junction  with  regards  to  the  potential  barrier  width 
produces an asymmetrical conducting two terminal device, better known as the Junction Diode. 
A  diode  is  one  of  the  simplest  semiconductor  devices,  which  has  the  characteristic  of  passing 
current  in one direction only. However, unlike a resistor, a diode does not behave  linearly  with 
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respect to the applied  voltage as the diode has an  exponential I-V relationship and therefore we 
can not described its operation by simply using an equation such as Ohm's law. 
If a suitable positive voltage (forward bias) is applied between the two ends of the PN junction, it 
can supply free electrons and holes with the extra energy they require to cross the junction as the 
width of the depletion layer around the PN junction is decreased. By applying a negative voltage 
(reverse  bias)  results  in  the  free  charges  being  pulled  away  from  the  junction  resulting  in  the 
depletion  layer  width  being  increased.  This  has  the  effect  of  increasing  or  decreasing  the 
effective resistance of the junction itself allowing or blocking current flow through the diode. 
Then  the  depletion  layer  widens  with  an  increase  in  the  application  of  a  reverse  voltage  and 
narrows with an increase in the application of a forward voltage. This is due to the differences in 
the electrical properties on the two sides of the PN junction resulting in physical changes taking 
place.  One  of  the  results  produces  rectification  as  seen  in  the  PN  junction  diodes  static  I-V 
(current-voltage)  characteristics.  Rectification  is  shown  by  an  asymmetrical  current  flow  when 
the polarity of bias voltage is altered as shown below. 
Junction Diode Symbol and Static I-V Characteristics. 
 
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But before we can use the PN junction as a practical device or as a rectifying device we need to 
firstly  bias  the  junction,  ie  connect  a  voltage  potential  across  it.  On  the  voltage  axis  above, 
"Reverse  Bias"  refers  to  an  external  voltage  potential  which  increases  the  potential  barrier.  An 
external  voltage  which  decreases  the  potential  barrier  is  said  to  act  in  the  "Forward  Bias" 
direction. 
There  are  two  operating  regions  and  three  possible  "biasing"  conditions  for  the  standard 
Junction Diode and these are: 
-  1. Zero Bias - No external voltage potential is applied to the PN-junction. 
-   
2.  Reverse  Bias  -  The  voltage  potential  is  connected  negative,  (-ve)  to  the  P-type  material  and  
      positive, (+ve) to the N-type material across the diode which has the effect of Increasing the  
      PN-junction width. 
-   
3.  Forward  Bias  -  The  voltage  potential  is  connected  positive,  (+ve)  to the  P-type  material  and  
      negative, (-ve) to the N-type material across the diode which has the effect of Decreasing the  
      PN-junction width. 
Zero Biased Junction Diode 
When a diode  is connected  in a  Zero Bias condition,  no external  potential energy  is applied to 
the  PN  junction.  However  if  the  diodes  terminals  are  shorted  together,  a  few  holes  (majority 
carriers)  in the P-type  material with enough energy to overcome the potential  barrier will  move 
across the junction against this barrier potential. This is known as the "Forward Current" and is 
referenced as I
F
 
Likewise,  holes  generated  in  the  N-type  material  (minority  carriers),  find  this  situation 
favourable and move across the junction in the opposite direction. This is known as the "Reverse 
Current" and  is referenced as I
R
. This transfer of electrons and  holes  back and  forth across the 
PN junction is known as diffusion, as shown below. 
 
 
 
 
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Zero Biased Junction Diode 
 
 
The  potential  barrier  that  now  exists  discourages  the  diffusion  of  any  more  majority  carriers 
across the  junction. However, the potential  barrier helps  minority  carriers (few  free electrons  in 
the P-region and few holes in the N-region) to drift across the junction. Then an "Equilibrium" or 
balance  will  be  established  when  the  majority  carriers  are  equal  and  both  moving  in  opposite 
directions,  so  that  the  net  result  is  zero  current  flowing  in  the  circuit.  When  this  occurs  the 
junction is said to be in a state of "Dynamic Equilibrium". 
The minority carriers are constantly generated due to thermal energy so this state of equilibrium 
can be broken by raising the temperature of the PN junction causing an increase in the generation 
of  minority  carriers,  thereby  resulting  in  an  increase  in  leakage  current  but  an  electric  current 
cannot flow since no circuit has been connected to the PN junction. 
Reverse Biased Junction Diode 
When a diode  is connected  in a  Reverse Bias condition, a positive  voltage  is applied to the N-
type  material  and  a  negative  voltage  is  applied  to  the  P-type  material.  The  positive  voltage 
applied to the N-type material attracts electrons towards the positive electrode and away from the 
junction, while the holes in the P-type end are also attracted away from the junction towards the 
negative  electrode.  The  net  result  is  that  the  depletion  layer  grows  wider  due  to  a  lack  of 
electrons and holes and presents a high impedance path, almost an insulator. The result is that a 
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high potential barrier is created thus preventing current from flowing through the semiconductor 
material. 
Reverse Biased Junction Diode showing an Increase in the Depletion Layer 
 
This condition represents a high resistance value to the PN junction and practically zero current 
flows through the junction diode with an increase in bias voltage. However, a very small  leakage 
current does flow through the junction which can be measured in microamperes, (A). One final 
point, if the reverse bias voltage Vr applied to the diode is increased to a sufficiently high enough 
value,  it  will  cause  the  PN  junction  to overheat  and  fail  due  to the  avalanche  effect  around  the 
junction.  This  may  cause  the  diode  to  become  shorted  and  will  result  in  the  flow  of  maximum 
circuit  current,  and  this  shown  as  a  step  downward  slope  in  the  reverse  static  characteristics 
curve below. 
Reverse Characteristics Curve for a Junction Diode 
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Sometimes this avalanche effect has practical applications in voltage stabilising circuits where a 
series  limiting resistor is used with the diode to limit this reverse breakdown current to a preset 
maximum value thereby producing a fixed voltage output across the diode. These types of diodes 
are commonly known as Zener Diodes and are discussed in a later tutorial. 
Forward Biased Junction Diode 
When a diode is connected in a Forward Bias condition, a negative voltage is applied to the N-
type  material  and  a  positive  voltage  is  applied  to  the  P-type  material.  If  this  external  voltage 
becomes greater than the value of the potential barrier, approx. 0.7 volts for silicon and 0.3 volts 
for germanium, the potential barriers opposition will be overcome and current will start to flow. 
This is because the negative voltage pushes or repels electrons towards the junction giving them 
the  energy  to  cross  over  and  combine  with  the  holes  being  pushed  in  the  opposite  direction 
towards the junction by the positive voltage. This results in a characteristics curve of zero current 
flowing  up  to  this  voltage  point,  called  the  "knee"  on  the  static  curves  and  then  a  high  current 
flow through the diode with little increase in the external voltage as shown below.  
Forward Characteristics Curve for a Junction Diode 
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The application of  a  forward biasing  voltage on the  junction diode results  in the depletion  layer 
becoming  very  thin  and  narrow  which  represents  a  low  impedance  path  through  the  junction 
thereby allowing high currents to flow. The point at which this sudden increase in current takes 
place is represented on the static I-V characteristics curve above as the "knee" point. 
Forward Biased Junction Diode showing a Reduction in the Depletion Layer 
 
This  condition  represents  the  low  resistance  path  through  the  PN  junction  allowing  very  large 
currents to flow through the diode with only a small increase in bias voltage. The actual potential 
difference  across  the  junction  or  diode  is  kept  constant  by  the  action  of  the  depletion  layer  at 
approximately 0.3v for germanium and approximately 0.7v for silicon junction diodes. Since the 
diode  can  conduct  "infinite"  current  above  this  knee  point  as  it  effectively  becomes  a  short 
circuit, therefore resistors are used in series with the diode to limit its current flow. Exceeding its 
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maximum forward current specification causes the device to dissipate more power in the form of 
heat than it was designed for resulting in a very quick failure of the device. 
Junction Diode Summary 
The PN junction region of a Junction Diode has the following important characteristics: 
-  1). Semiconductors contain two types of mobile charge carriers, Holes and Electrons. 
-    
-  2). The holes are positively charged while the electrons negatively charged. 
-    
-  3). A semiconductor may be doped with donor impurities such as Antimony (N-type doping), so 
that it contains mobile charges which are primarily electrons. 
-    
-  4). A  semiconductor may  be doped with  acceptor  impurities such as Boron (P-type doping), so 
that it contains mobile charges which are mainly holes. 
-    
-  5). The junction region itself has no charge carriers and is known as the depletion region. 
-    
-  6). The junction (depletion) region has a physical thickness that varies with the applied voltage. 
-    
-  7).When  a  diode  is  Zero  Biased  no  external  energy  source  is  applied  and  a  natural  Potential 
Barrier  is  developed  across  a  depletion  layer  which  is  approximately  0.5  to  0.7v  for  silicon 
diodes and approximately 0.3 of a volt for germanium diodes. 
-    
-  8). When a junction diode is Forward Biased the thickness of the depletion region reduces and 
the diode acts like a short circuit allowing full current to flow. 
-    
-  9). When a junction diode is Reverse Biased the thickness of the depletion region increases and 
the diode acts like an open circuit blocking any current flow, (only a very small leakage current). 
In  the  next  tutorial  about  diodes,  we  will  look  at  the  small  signal  diode  sometimes  called  a 
switching diode that are used  in  general electronic circuits.  A  signal diode  is designed  for  low-
voltage  or  high  frequency  signal  applications  such  as  in  radio  or  digital  switching  circuits  as 
opposed to the high-current  mains rectification diodes  in which  silicon diodes  are usually used, 
and examine the Signal Diode static current-voltage characteristics curve and parameters. 
 
 
 
 
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Signal Diode 
The Signal Diode 
The semiconductor Signal Diode is a small  non-linear semiconductor devices generally used  in 
electronic  circuits,  where  small  currents  or  high  frequencies  are  involved  such  as  in  radio, 
television and digital logic circuits. The signal diode which is also sometimes known by its older 
name of the  Point Contact Diode or the Glass  Passivated Diode, are physically  very  small  in 
size compared to their larger Power Diode cousins. 
Generally,  the  PN  junction  of  a  small  signal  diode  is  encapsulated  in  glass  to  protect  the  PN 
junction, and usually have a red or black band at one end of their body to help identify which end 
is the cathode terminal. The  most widely used of  all the glass  encapsulated signal  diodes  is the 
very common 1N4148 and its equivalent 1N914 signal diode. Small signal and switching diodes 
have  much  lower  power  and  current  ratings,  around  150mA,  500mW  maximum  compared  to 
rectifier  diodes,  but  they  can  function  better  in  high  frequency  applications  or  in  clipping  and 
switching applications that deal with short-duration pulse waveforms. 
The  characteristics  of  a  signal  point  contact  diode  are  different  for  both  germanium  and  silicon 
types and are given as: 
-  Germanium  Signal  Diodes  -  These  have  a  low  reverse  resistance  value  giving  a  lower  forward 
volt drop across the junction, typically only about 0.2-0.3v, but have a higher forward resistance 
value because of their small junction area. 
-    
-  Silicon  Signal  Diodes  -  These  have  a  very  high  value  of  reverse  resistance  and  give  a  forward 
volt drop of about 0.6-0.7v across the junction. They have fairly low values of forward resistance 
giving them high peak values of forward current and reverse voltage. 
The electronic symbol given for any type of diode is that of an arrow with a bar or line at its end 
and this is illustrated below along with the Steady State V-I Characteristics Curve. 
 
 
 
 
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Silicon Diode V-I Characteristic Curve 
 
  
The  arrow  points  in  the  direction  of  conventional  current  flow  through  the  diode  meaning  that 
the  diode  will  only  conduct  if  a  positive  supply  is  connected  to  the  Anode  (a)  terminal  and  a 
negative  supply  is  connected  to  the  Cathode  (k)  terminal  thus  only  allowing  current  to  flow 
through  it  in  one  direction  only,  acting  more  like  a  one  way  electrical  valve,  (Forward  Biased 
Condition). However, we know from the previous tutorial that if we connect the external energy 
source in the other direction the diode will block any current flowing through it and instead will 
act like an open switch, (Reversed Biased Condition) as shown below. 
Forward and Reversed Biased Diode 
 
Then  we  can  say  that  an  ideal  small  signal  diode  conducts  current  in  one  direction  (forward-
conducting) and blocks current in the other direction (reverse-blocking). Signal Diodes are used 
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in  a  wide  variety  of  applications  such  as  a  switch  in  rectifiers,  limiters,  snubbers  or  in  wave-
shaping circuits. 
Signal Diode Parameters 
Signal Diodes are manufactured in a range of voltage and current ratings and care must be taken 
when  choosing  a  diode  for  a  certain  application.  There  are  a  bewildering  array  of  static 
characteristics associated with the humble signal diode but the more important ones are. 
1. Maximum Forward Current 
The Maximum Forward Current (I
F(max)
) is as its name implies the  maximum forward current 
allowed to flow through the device. When the diode is conducting in the forward bias condition, 
it  has  a  very  small  "ON"  resistance  across  the  PN  junction  and  therefore,  power  is  dissipated 
across  this  junction  (Ohms  Law)  in  the  form  of  heat.  Then,  exceeding  its  (I
F(max)
)  value  will 
cause  more  heat  to  be  generated  across  the  junction  and  the  diode  will  fail  due  to  thermal 
overload, usually with destructive consequences. When operating diodes around their maximum 
current  ratings  it  is  always  best to  provide  additional  cooling  to  dissipate  the  heat  produced  by 
the diode. 
For example, our small 1N4148 signal diode has a maximum current rating of about 150mA with 
a power dissipation of 500mW at 25
o
C. Then a resistor must be used in series with the diode to 
limit the forward current, (I
F(max)
) through it to below this value. 
2. Peak Inverse Voltage 
The  Peak  Inverse  Voltage  (PIV)  or  Maximum  Reverse  Voltage  (V
R(max)
),  is  the  maximum 
allowable  Reverse  operating  voltage  that  can  be  applied  across  the  diode  without  reverse 
breakdown  and  damage  occurring  to  the  device.  This  rating  therefore,  is  usually  less  than  the 
"avalanche  breakdown"  level  on  the  reverse  bias  characteristic  curve.  Typical  values  of  V
R(max)
 
range from a few volts to thousands of volts and must be considered when replacing a diode. 
The  peak  inverse  voltage  is  an  important  parameter  and  is  mainly  used  for  rectifying  diodes  in 
AC rectifier circuits with reference to the amplitude of the voltage were the sinusoidal waveform 
changes from a positive to a negative value on each and every cycle. 
3. Forward Power Dissipation 
Signal diodes have a  Forward Power Dissipation, (P
D(max)
) rating. This rating  is the  maximum 
possible  power  dissipation  of  the  diode  when  it  is  forward  biased  (conducting).  When  current 
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flows  through  the  signal  diode  the  biasing  of  the  PN  junction  is  not  perfect  and  offers  some 
resistance to the flow of current resulting in power being dissipated (lost) in the diode in the form 
of  heat.  As  small  signal  diodes  are  nonlinear  devices  the  resistance  of  the  PN  junction  is  not 
constant, it is a dynamic property then we cannot use Ohms Law to define the power in terms of 
current  and  resistance  or  voltage  and  resistance  as  we  can  for  resistors. Then  to  find  the  power 
that will be dissipated by the diode we must multiply the voltage drop across it times the current 
flowing through it: P
D
 = VxI 
4. Maximum Operating Temperature 
The  Maximum  Operating  Temperature  actually  relates  to  the  Junction  Temperature  (T
J
)  of 
the diode and is related to maximum power dissipation. It is the maximum temperature allowable 
before the structure of the diode deteriorates and is expressed  in units of degrees centigrade per 
Watt, ( 
o
C/W ). This value is linked closely to the maximum forward current of the device so that 
at  this  value  the  temperature  of  the  junction  is  not  exceeded.  However,  the  maximum  forward 
current  will  also  depend  upon  the  ambient  temperature  in  which  the  device  is  operating  so  the 
maximum forward current is usually quoted for two or more ambient temperature values such as 
25
o
C or 70
o
C. 
Then there are three main parameters that must be considered when either selecting or replacing 
a signal diode and these are: 
-  The Reverse Voltage Rating 
-  The Forward Current Rating 
-  The Forward Power Dissipation Rating 
Signal Diode Arrays 
When  space  is  limited,  or  matching  pairs  of  switching  signal  diodes  are  required,  diode  arrays 
can  be  very useful. They generally consist of  low capacitance high speed silicon diodes such as 
the  1N4148  connected  together  in  multiple  diode  packages  called  an  array  for  use  in  switching 
and clamping in digital circuits. They are encased in single inline packages (SIP) containing 4 or 
more  diodes  connected  internally  to  give  either  an  individual  isolated  array,  common  cathode, 
(CC), or a common anode, (CA) configuration as shown. 
 
 
 
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Signal Diode Arrays 
 
Signal diode arrays can also  be used  in digital  and computer circuits to protect high speed data 
lines  or  other  input/output  parallel  ports  against  electrostatic  discharge,  (ESD)  and  voltage 
transients. By connecting two diodes in series across the supply rails with the data line connected 
to  their  junction  as  shown,  any  unwanted  transients  are  quickly  dissipated  and  as  the  signal 
diodes are available in 8-fold arrays they can protect eight data lines in a single package. 
 
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CPU Data Line Protection 
Signal  diode  arrays  can  also  be  used  to  connect  together  diodes  in  either  series  or  parallel 
combinations to form  voltage regulator or voltage reducing type circuits or to produce a known 
fixed  voltage.  We  know  that  the  forward  volt  drop  across  a  silicon  diode  is  about  0.7v  and  by 
connecting  together  a  number  of  diodes  in  series  the  total  voltage  drop  will  be  the  sum  of  the 
individual  voltage drops of each diode. However, when signal  diodes  are connected together  in 
series, the current will be the same for each diode so the maximum forward current must not be 
exceeded. 
Connecting Signal Diodes in Series 
Another application for the small signal diode is to create a regulated voltage supply. Diodes are 
connected together in series to provide a constant DC voltage across the diode combination. The 
output voltage across the diodes remains constant  in spite of changes  in the  load current drawn 
from  the  series  combination  or  changes  in  the  DC  power  supply  voltage  that  feeds  them. 
Consider the circuit below. 
Signal Diodes in Series 
 
As  the  forward  voltage  drop  across  a  silicon  diode  is  almost  constant  at  about  0.7v,  while  the 
current through  it  varies  by relatively  large amounts, a  forward-biased signal  diode can  make a 
simple  voltage regulating circuit. The  individual  voltage drops across each diode  are subtracted 
from  the  supply  voltage  to  leave  a  certain  voltage  potential  across  the  load  resistor,  and  in  our 
simple example above this is given as 10v  - (3 x 0.7v) = 7.9v. This is because each diode has a 
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junction  resistance  relating  to  the  small  signal  current  flowing  through  it  and  the  three  signal 
diodes  in series will  have three times the value of this resistance, along with the  load resistance 
R, forms a voltage divider across the supply. 
By  adding  more  diodes  in  series  a  greater  voltage  reduction  will  occur.  Also  series  connected 
diodes can be placed in parallel with the load resistor to act as a voltage regulating circuit. Here 
the  voltage  applied  to  the  load  resistor  will  be  3  x  0.7v  =  2.1v.  We  can  of  course  produce  the 
same  constant  voltage  source  using  a  single  Zener  Diode.  Resistor,  R
D
  is  used  to  prevent 
excessive current flowing through the diodes if the load is removed. 
Freewheel Diodes 
Signal  diodes  can  also  be  used  in  a  variety  of  clamping,  protection  and  wave  shaping  circuits 
with the  most common  form of clamping diode circuit being one which uses a diode connected 
in  parallel  with  a  coil  or  inductive  load  to  prevent  damage  to  the  delicate  switching  circuit  by 
suppressing  the  voltage  spikes  and/or  transients  that  are  generated  when  the  load  is  suddenly 
turned "OFF". This type of diode  is generally known as a "Free-wheeling Diode" or  Freewheel 
diode as it is more commonly called. 
The  Freewheel  diode  is  used  to  protect  solid  state  switches  such  as  power  transistors  and 
MOSFET's  from  damage  by  reverse  battery  protection  as  well  as  protection  from  highly 
inductive loads such as relay coils or motors, and an example of its connection is shown below.  
Use of the Freewheel Diode 
 
Modern  fast switching, power semiconductor devices require  fast switching diodes  such as  free 
wheeling  diodes  to  protect  them  form  inductive  loads  such  as  motor  coils  or  relay  windings. 
Every  time  the  switching  device  above  is  turned  "ON",  the  freewheel  diode  changes  from  a 
conducting  state  to  a  blocking  state  as  it  becomes  reversed  biased.  However,  when  the  device 
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rapidly turns "OFF", the diode becomes  forward biased and the collapse of the energy  stored in 
the  coil  causes  a  current  to  flow  through  the  freewheel  diode.  Without  the  protection  of  the 
freewheel diode high di/dt currents would occur causing a high voltage spike or transient to flow 
around the circuit possibly damaging the switching device. 
Previously,  the  operating  speed  of  the  semiconductor  switching  device,  either  transistor, 
MOSFET,  IGBT  or  digital  has  been  impaired  by  the  addition  of  a  freewheel  diode  across  the 
inductive  load  with  Schottky  and  Zener  diodes  being  used  instead  in  some  applications.  But 
during  the  past  few  years  however,  freewheel  diodes  had  regained  importance  due  mainly  to 
their improved reverse-recovery characteristics and the use of super fast semiconductor materials 
capable at operating at high switching frequencies. 
Other  types  of  specialized  diodes  not  included  here  are  Photo-Diodes,  PIN  Diodes,  Tunnel 
Diodes and Schottky Barrier Diodes. By adding more PN junctions to the basic two layer diode 
structure  other  types  of  semiconductor  devices  can  be  made.  For  example  a  three  layer 
semiconductor  device  becomes  a  Transistor,  a  four  layer  semiconductor  device  becomes  a 
Thyristor  or  Silicon  Controlled  Rectifier  and  five  layer  devices  known  as  Triacs  are  also 
available. 
In  the  next  tutorial  about  diodes,  we  will  look  at  the  large  signal  diode  sometimes  called  the 
Power  Diode.  Power  diodes  are  silicon  diodes  designed  for  use  in  high-voltage,  high-current 
mains rectification circuits. 
 
Power Diodes and Rectifiers 
 
The Power Diode 
In  the  previous  tutorials  we  saw  that  a  semiconductor  signal  diode  will  only  conduct  current  in 
one  direction  from  its  anode  to  its  cathode  (forward  direction),  but  not  in  the  reverse  direction 
acting  a  bit  like  an  electrical  one  way  valve.  A  widely  used  application  of  this  feature  is  in  the 
conversion  of  an  alternating  voltage  (AC)  into  a  continuous  voltage  (DC).  In  other  words, 
Rectification. Small  signal diodes can  be used as  rectifiers  in  low-power, low current (less than 
1-amp)  rectifiers  or  applications,  but  were  larger  forward  bias  currents  or  higher  reverse  bias 
blocking voltages are involved the PN junction of a small signal diode would eventually overheat 
and melt so larger more robust Power Diodes are used instead. 
The  power  semiconductor  diode,  known  simply  as  the  Power  Diode,  has  a  much  larger  PN 
junction  area  compared  to  its  smaller  signal  diode  cousin,  resulting  in  a  high  forward  current 
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capability  of  up  to  several  hundred  amps  (KA)  and  a  reverse  blocking  voltage  of  up  to  several 
thousand  volts  (KV).  Since  the  power  diode  has  a  large  PN  junction,  it  is  not  suitable  for  high 
frequency  applications  above  1MHz,  but  special  and  expensive  high  frequency,  high  current 
diodes  are  available.  For  high  frequency  rectifier  applications  Schottky  Diodes  are  generally 
used  because  of  their  short  reverse  recovery  time  and  low  voltage  drop  in  their  forward  bias 
condition. 
Power  diodes  provide  uncontrolled  rectification  of  power  and  are  used  in  applications  such  as 
battery charging and DC power supplies as well as AC rectifiers and inverters. Due to their high 
current  and  voltage  characteristics  they  can  also  be  used  as  freewheeling  diodes  and  snubber 
networks. Power diodes are designed to have  a forward "ON" resistance of fractions of an Ohm 
while  their  reverse  blocking  resistance  is  in  the  mega-Ohms  range.  Some  of  the  larger  value 
power diodes are designed to be "stud mounted" onto heatsinks reducing their thermal resistance 
to between 0.1 to 1
o
C/Watt. 
If an alternating voltage is applied across a power diode, during the positive half cycle the diode 
will  conduct  passing  current  and  during  the  negative  half  cycle  the  diode  will  not  conduct 
blocking  the  flow  of  current.  Then  conduction  through  the  power  diode  only  occurs  during  the 
positive half cycle and is therefore unidirectional i.e. DC as shown. 
Power Diode Rectifier 
 
 
Power  diodes  can  be  used  individually  as  above  or  connected  together  to  produce  a  variety  of 
rectifier  circuits  such  as  "Half-Wave",  "Full-Wave"  or  as  "Bridge  Rectifiers".  Each  type  of 
rectifier circuit can  be classed as either uncontrolled, half-controlled or fully controlled were an 
uncontrolled rectifier uses only power diodes, a  fully controlled rectifier uses thyristors (SCRs) 
and  a  half  controlled  rectifier  is  a  mixture  of  both  diodes  and  thyristors.  The  most  commonly 
used  individual  power  diode  for  basic  electronics  applications  is  the  general  purpose  1N400x 
Series  Glass  Passivated  type  rectifying  diode  with  standard  ratings  of  continuous  forward 
rectified current of 1.0 amp and reverse blocking voltage ratings from 50v for the 1N4001 up to 
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1000v  for  the  1N4007,  with  the  small  1N4007GP  being  the  most  popular  for  general  purpose 
mains voltage rectification. 
Half Wave Rectification 
A  rectifier  is  a  circuit  which  converts  the  Alternating  Current  (AC)  input  power  into  a  Direct 
Current  (DC)  output  power.  The  input  power  supply  may  be  either  a  single-phase  or  a  multi-
phase supply with the simplest of all the rectifier circuits being that of the Half Wave Rectifier. 
The power diode in a half wave rectifier circuit passes just one half of each complete sine wave 
of  the  AC  supply  in  order  to  convert  it  into  a  DC  supply.  Then  this  type  of  circuit  is  called  a 
"half-wave"  rectifier  because  it  passes  only  half  of  the  incoming  AC  power  supply  as  shown 
below. 
Half Wave Rectifier Circuit 
 
 
During each "positive" half cycle of the AC sine wave, the diode is forward biased as the anode 
is  positive  with  respect to the  cathode resulting  in  current  flowing  through  the  diode.  Since  the 
DC load is resistive (resistor, R), the current flowing in the load resistor is therefore proportional 
to the voltage (Ohms Law), and the voltage across the  load resistor will therefore be the same 
as  the  supply  voltage,  Vs  (minus  Vf),  that  is  the  "DC"  voltage  across the  load  is  sinusoidal  for 
the first half cycle only so Vout = Vs. 
During each "negative" half cycle of the AC sine wave, the diode is reverse biased as the anode 
is  negative with respect to the cathode therefore, No current flows through the diode or circuit. 
Then in the negative half cycle of the supply, no current flows in the load resistor as no voltage 
appears across it so Vout = 0. 
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The  current  on  the  DC  side  of  the  circuit  flows  in  one  direction  only  making  the  circuit 
Unidirectional  and  the  value  of  the  DC  voltage  V
DC
  across  the  load  resistor  is  calculated  as 
follows. 
 
 
Where  V
max
  is  the  maximum  voltage  value  of  the  AC  supply,  and  V
S
  is  the  r.m.s.  value  of  the 
supply. 
Example No1. 
Calculate the current, ( I
DC
 ) flowing through a 100 resistor connected to a 240v single phase 
half-wave rectifier as shown above. Also calculate the power consumed by the load. 
 
 
During  the  rectification  process  the  resultant  output  DC  voltage  and  current  are  therefore  both 
"ON"  and  "OFF"  during  every  cycle.  As  the  voltage  across  the  load  resistor  is  only  present 
during the positive  half of the cycle (50% of the  input waveform), this results  in a  low  average 
DC value being supplied to the load. The variation of the rectified output waveform between this 
ON  and  OFF  condition  produces  a  waveform  which  has  large  amounts  of  "ripple"  which  is  an 
undesirable  feature.  The  resultant  DC  ripple  has  a  frequency  that  is  equal  to  that  of  the  AC 
supply frequency. 
Very often when rectifying an alternating voltage we wish to produce a "steady" and continuous 
DC voltage free from any voltage variations or ripple. One way of doing this is to connect a large 
value  Capacitor  across  the  output  voltage  terminals  in  parallel  with  the  load  resistor  as  shown 
below. This type of capacitor is known commonly as a "Reservoir" or Smoothing Capacitor. 
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Half-wave Rectifier with Smoothing Capacitor 
 
When rectification  is used to provide a direct  voltage power supply  from  an alternating  source, 
the amount of ripple can be further reduced by using larger value capacitors but there are limits 
both on cost and size.  For a given capacitor value, a greater load current (smaller  load resistor) 
will  discharge  the  capacitor  more  quickly  (RC  Time  Constant)  and  so  increases  the  ripple 
obtained.  Then  for  single  phase,  half-wave  rectifier  circuits  it  is  not  very  practical  to  try  and 
reduce  the  ripple  voltage  by  capacitor  smoothing  alone,  it  is  more  practical  to  use  "Full-wave 
Rectification" instead. 
In practice, the half-wave rectifier is used most often in low-power applications because of their 
major  disadvantages  being.  The  output  amplitude  is  less  than  the  input  amplitude,  there  is  no 
output  during  the  negative  half  cycle  so  half  the  power  is  wasted  and  the  output  is  pulsed  DC 
resulting  in  excessive  ripple.  To overcome  these  disadvantages  a  number  of  Power  Diodes  are 
connected together to produce a Full Wave Rectifier as discussed in the next tutorial. 
 
Full Wave Rectifier 
 
In  the  previous  Power  Diodes  tutorial  we  discussed  ways  of  reducing  the  ripple  or  voltage 
variations on a direct DC voltage by connecting capacitors across the load resistance. While this 
method may be suitable for low power applications it is unsuitable to applications which need a 
"steady  and  smooth"  DC  supply  voltage.  One  method  to  improve  on  this  is  to  use  every  half-
cycle of the input voltage instead of every other half-cycle. The circuit which allows us to do this 
is called a Full Wave Rectifier. 
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Like  the  half  wave  circuit,  a  full  wave  rectifier  circuit  produces  an  output  voltage  or  current 
which  is  purely  DC  or  has  some  specified  DC  component.  Full  wave  rectifiers  have  some 
fundamental  advantages  over  their  half  wave  rectifier  counterparts.  The  average  (DC)  output 
voltage  is  higher  than  for  half  wave,  the  output  of  the  full  wave  rectifier  has  much  less  ripple 
than that of the half wave rectifier producing a smoother output waveform. 
In  a  Full  Wave  Rectifier  circuit  two  diodes  are  now  used,  one  for  each  half  of  the  cycle.  A 
transformer  is  used  whose  secondary  winding  is  split  equally  into  two  halves  with  a  common 
centre tapped connection, (C). This configuration results  in each diode conducting  in turn when 
its anode terminal is positive with respect to the transformer centre point C producing an output 
during  both  half-cycles,  twice  that  for  the  half  wave  rectifier  so  it  is  100%  efficient  as  shown 
below. 
Full Wave Rectifier Circuit 
 
 
The full wave rectifier circuit consists of two power diodes connected to a single load resistance 
(R
L
)  with  each  diode  taking  it  in  turn  to  supply  current  to  the  load.  When  point  A  of  the 
transformer  is  positive  with  respect  to  point  B,  diode  D
1
  conducts  in  the  forward  direction  as 
indicated by the arrows. When point B is positive (in the negative half of the cycle) with respect 
to point A, diode D
2
 conducts in the forward direction and the current flowing through resistor R 
is in the same direction for both circuits. As the output voltage across the resistor R is the phasor 
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sum  of  the  two  waveforms  combined,  this  type  of  full  wave  rectifier  circuit  is  also  known  as  a 
"bi-phase" circuit. 
As  the  spaces  between  each  half-wave  developed  by  each  diode  is  now  being  filled  in  by  the 
other  diode  the  average  DC  output  voltage  across  the  load  resistor  is  now  double  that  of  the 
single  half-wave  rectifier  circuit  and  is  about  0.637V
max
  of  the  peak  voltage,  assuming  no 
losses. However in reality, during each half cycle the current flows through two diodes instead of 
just one so the amplitude of the output voltage is two voltage drops ( 2 x 0.7 = 1.4V ) less than 
the input V
MAX
 amplitude. 
 
 
The  peak  voltage  of  the  output  waveform  is  the  same  as  before  for  the  half-wave  rectifier 
provided  each  half  of  the  transformer  windings  have  the  same  rms  voltage  value.  To  obtain  a 
different  DC  voltage  output  different transformer  ratios  can  be  used.  The  main  disadvantage  of 
this  type  of  full  wave  rectifier  circuit  is  that  a  larger  transformer  for  a  given  power  output  is 
required  with  two  separate  but  identical  secondary  windings  making  this  type  of  full  wave 
rectifying circuit costly compared to the "Full Wave Bridge Rectifier" circuit equivalent. 
The Full Wave Bridge Rectifier 
Another type of circuit that produces the same output waveform as the full wave rectifier circuit 
above,  is  that  of  the  Full  Wave  Bridge  Rectifier.  This  type  of  single  phase  rectifier  uses  four 
individual  rectifying  diodes  connected  in  a  closed  loop  "bridge"  configuration  to  produce  the 
desired  output.  The  main  advantage  of  this  bridge  circuit  is  that  it  does  not  require  a  special 
centre  tapped  transformer,  thereby  reducing  its  size  and  cost.  The  single  secondary  winding  is 
connected to one side of the diode bridge network and the load to the other side as shown below.  
The Diode Bridge Rectifier 
 
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The four diodes labelled D
1
 to D
4
 are arranged in "series pairs" with only two diodes conducting 
current  during  each  half  cycle.  During  the  positive  half  cycle  of  the  supply,  diodes  D1  and  D2 
conduct  in  series  while  diodes  D3  and  D4  are  reverse  biased  and  the  current  flows  through the 
load as shown below. 
The Positive Half-cycle 
 
 
During the negative half cycle of the supply, diodes D3 and D4 conduct in series, but diodes D1 
and  D2  switch  of  as  they  are  now  reverse  biased.  The  current  flowing  through  the  load  is  the 
same direction as before. 
 
 
 
 
 
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The Negative Half-cycle 
 
 
As  the  current  flowing  through  the  load  is  unidirectional,  so  the  voltage  developed  across  the 
load  is  also  unidirectional  the  same  as  for  the  previous  two  diode  full-wave  rectifier,  therefore 
the  average  DC  voltage  across the  load  is  0.637V
max
  and  the  ripple  frequency  is  now  twice  the 
supply frequency (e.g. 100Hz for a 50Hz supply). 
 
Typical Bridge Rectifier 
Although we can use four individual power diodes to make a full wave bridge rectifier, pre-made 
bridge  rectifier  components  are  available  "off-the-shelf"  in  a  range  of  different  voltage  and 
current  sizes  that  can  be  soldered  directly  into  a  PCB  circuit  board  or  be  connected  by  spade 
connectors. The  image to the right shows a typical single phase bridge rectifier with one corner 
cut off. This cut-off corner indicates that the terminal nearest to the corner is the positive or +ve 
output terminal  or  lead  with  the  opposite  (diagonal)  lead  being  the  negative  or  -ve output  lead. 
The  other  two  connecting  leads  are  for  the  input  alternating  voltage  from  a  transformer 
secondary winding. 
 
 
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The Smoothing Capacitor 
We saw in the previous section that the single phase half-wave rectifier produces an output wave 
every  half  cycle  and  that  it  was  not  practical  to  use  this  type  of  circuit  to  produce  a  steady  DC 
supply. The full-wave bridge rectifier however, gives us a greater mean DC value (0.637 Vmax) 
with  less  superimposed  ripple  while  the  output  waveform  is  twice  that  of  the  frequency  of  the 
input  supply  frequency.  We  can  therefore  increase  its  average  DC  output  level  even  higher  by 
connecting a suitable smoothing capacitor across the output of the bridge circuit as shown below.  
Full-wave Rectifier with Smoothing Capacitor 
 
 
The smoothing capacitor converts the full-wave rippled output of the rectifier into a smooth DC 
output voltage. Generally for DC power supply circuits the smoothing capacitor is an Aluminium 
Electrolytic type that has a capacitance value of 100uF or more with repeated DC voltage pulses 
from  the  rectifier  charging  up  the  capacitor  to  peak  voltage.  However,  their  are  two  important 
parameters to consider when choosing a suitable  smoothing capacitor and these are  its  Working 
Voltage, which must be higher than the no-load output value of the rectifier and its Capacitance 
Value,  which  determines  the  amount  of  ripple  that  will  appear  superimposed  on  top of  the  DC 
voltage. Too low a value and the capacitor has little effect but if the smoothing capacitor is large 
enough (parallel capacitors can be used) and the load current is not too large, the output voltage 
will be almost as smooth as pure DC. As a general rule of thumb, we are looking to have a ripple 
voltage of less than 100mV peak to peak. 
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The maximum ripple voltage present for a Full Wave Rectifier circuit is not only determined by 
the value of the smoothing capacitor but by the frequency and load current, and is calculated as: 
Bridge Rectifier Ripple Voltage 
 
Where:  I  is  the  DC  load  current  in  amps,    is  the  frequency  of  the  ripple  or  twice  the  input 
frequency in Hertz, and C is the capacitance in Farads. 
The main advantages of a full-wave bridge rectifier is that it has a smaller AC ripple value for a 
given load and a smaller reservoir or smoothing capacitor than an equivalent half-wave rectifier. 
Therefore,  the  fundamental  frequency  of  the  ripple  voltage  is  twice  that  of  the  AC  supply 
frequency  (100Hz)  where  for the  half-wave  rectifier  it  is  exactly  equal  to the  supply  frequency 
(50Hz). 
The amount of ripple voltage that is superimposed on top of the DC supply voltage by the diodes 
can be virtually eliminated by adding a much improved -filter (pi-filter) to the output terminals 
of the bridge rectifier. This type of low-pass filter consists of two smoothing capacitors, usually 
of the same value and a choke or inductance across them to introduce a high impedance path to 
the  alternating  ripple  component.  Another  more  practical  and  cheaper  alternative  is  to  use  a  3-
terminal voltage regulator IC, such as a LM78xx for a positive output voltage or the LM79xx for 
a  negative  output  voltage  which  can  reduce  the  ripple  by  more  than  70dB  (Datasheet)  while 
delivering a constant output current of over 1 amp. 
In the  next tutorial about diodes, we will  look at the  Zener Diode which takes advantage of  its 
reverse  breakdown  voltage  characteristic  to  produce  a  constant  and  fixed  output  voltage  across 
itself. 
Zener Diodes 
 
The Zener Diode 
In the previous Signal Diode tutorial, we saw that a "reverse biased" diode blocks current in the 
reverse  direction,  but  will  suffer  from  premature  breakdown  or  damage  if  the  reverse  voltage 
applied  across  it  is  too  high.  However,  the  Zener  Diode  or  "Breakdown  Diode"  as  they  are 
sometimes  called,  are  basically  the  same  as  the  standard  PN  junction  diode  but  are  specially 
designed  to  have  a  low  pre-determined  Reverse  Breakdown  Voltage  that  takes  advantage  of 
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this high reverse voltage. The point at which a zener diode breaks down or conducts is called the 
"Zener Voltage" (Vz). 
The  Zener  diode  is  like  a  general-purpose  signal  diode  consisting  of  a  silicon  PN  junction. 
When biased in the forward direction it behaves just like a normal signal diode passing the rated 
current,  but  when  a  reverse  voltage  is  applied  to it  the  reverse  saturation  current  remains  fairly 
constant over a wide range of voltages. The reverse voltage increases until the diodes breakdown 
voltage  V
B
  is  reached  at  which  point  a  process  called  Avalanche  Breakdown  occurs  in  the 
depletion  layer  and  the  current  flowing  through  the  zener  diode  increases  dramatically  to  the 
maximum  circuit  value  (which  is  usually  limited  by  a  series  resistor).  This  breakdown  voltage 
point is called the "zener voltage" for zener diodes. 
The point at which current flows can be very accurately controlled (to less than 1% tolerance) in 
the doping stage of the diodes construction giving the diode a specific zener breakdown voltage, 
(Vz) ranging from a few volts up to a few hundred volts. This zener breakdown voltage on the I-
V curve is almost a vertical straight line. 
Zener Diode I-V Characteristics 
 
 
The Zener Diode is used in its "reverse bias" or reverse breakdown mode, i.e. the diodes anode 
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connects  to  the  negative  supply.  From  the  I-V  characteristics  curve  above,  we  can  see  that  the 
zener diode has a region  in  its reverse  bias characteristics of almost a constant negative  voltage 
regardless of the value of the current flowing through the diode and remains nearly constant even 
with large changes in current as long as the zener diodes current remains between the breakdown 
current I
Z(min)
 and the maximum current rating I
Z(max)
. 
This  ability  to  control  itself  can  be  used  to  great effect  to  regulate  or  stabilise  a  voltage  source 
against  supply  or  load  variations.  The  fact  that  the  voltage  across  the  diode  in  the  breakdown 
region is almost constant turns out to be an important application of the zener diode as a voltage 
regulator. The function of a regulator is to provide a constant output voltage to a load connected 
in parallel with it in spite of the ripples in the supply voltage or the variation in the load current 
and the zener diode will continue to regulate the voltage until the diodes current falls below the 
minimum I
Z(min)
 value in the reverse breakdown region. 
The Zener Diode Regulator 
Zener Diodes can  be used to produce a stabilised voltage output with  low ripple under  varying 
load current conditions. By passing a small current through the diode from a voltage source, via a 
suitable current limiting resistor (R
S
), the zener diode will conduct sufficient current to maintain 
a  voltage  drop  of  Vout.  We  remember  from  the  previous  tutorials  that  the  DC  output  voltage 
from the  half or full-wave rectifiers contains ripple superimposed onto the DC  voltage and that 
as  the  load  value  changes  so  to  does  the  average  output  voltage.  By  connecting  a  simple  zener 
stabiliser circuit as shown  below across the output of the rectifier, a  more stable output voltage 
can be produced. 
Zener Diode Regulator 
 
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The resistor, R
S
 is connected in series with the zener diode to limit the current flow through the 
diode with the voltage source, V
S
 being connected across the combination. The stabilised output 
voltage V
out
 is taken from across the zener diode. The zener diode is connected with its cathode 
terminal  connected  to  the  positive  rail  of  the  DC  supply  so  it  is  reverse  biased  and  will  be 
operating  in  its  breakdown  condition.  Resistor  R
S
  is  selected  so  to  limit  the  maximum  current 
flowing in the circuit. 
With no load connected to the circuit, the load current will be zero, ( I
L
 = 0 ), and all the circuit 
current passes through the zener diode which inturn dissipates its maximum power. Also a small 
value of the series resistor R
S
 will result in a greater diode current when the load resistance R
L
 is 
connected and  large as this will  increase the power dissipation requirement of the diode so care 
must  be  taken  when  selecting  the  appropriate  value  of  series  resistance  so  that  the  zeners 
maximum power rating is not exceeded under this no-load or high-impedance condition. 
The  load  is  connected  in  parallel  with  the  zener  diode,  so  the  voltage  across  R
L
  is  always  the 
same  as  the  zener  voltage,  ( V
R
 = V
Z
 ).  There  is  a  minimum  zener  current  for  which  the 
stabilization of the voltage is effective and the zener current must stay above this value operating 
under  load  within  its  breakdown  region  at  all  times.  The  upper  limit  of  current  is  of  course 
dependant upon the power rating of the device. The supply voltage V
S
 must be greater than V
Z
. 
One  small problem with zener diode stabiliser circuits  is that the diode can sometimes generate 
electrical noise on top of the DC supply as it tries to stabilise the voltage. Normally this is not a 
problem  for  most  applications  but the  addition  of  a  large  value  decoupling  capacitor  across the 
zeners output may be required to give additional smoothing. 
Then  to  summarise  a  little.  A  zener  diode  is  always  operated  in  its  reverse  biased  condition.  A 
voltage  regulator  circuit  can  be  designed  using  a  zener  diode  to  maintain  a  constant  DC  output 
voltage across the  load  in spite of  variations  in the  input voltage or changes  in the  load current. 
The zener voltage regulator consists of a current limiting resistor R
S
 connected in series with the 
input  voltage  V
S
  with  the  zener  diode  connected  in  parallel  with  the  load  R
L
  in  this  reverse 
biased  condition.  The  stabilized  output  voltage  is  always  selected  to  be  the  same  as  the 
breakdown voltage V
Z
 of the diode. 
Example No1 
A 5.0V stabilised power supply is required to be produced from a 12V DC power supply 
input source. The  maximum power rating P
Z
 of the zener diode  is 2W. Using the zener 
regulator circuit above calculate: 
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a) The maximum current flowing through the zener diode. 
 
 
 
b) The value of the series resistor, R
S
 
 
 
 
c) The load current I
L
 if a load resistor of 1k is connected across the Zener diode. 
 
 
 
d) The total supply current I
S
 
 
 
Zener Diode Voltages 
As  well  as  producing  a  single  stabilised  voltage  output,  zener  diodes  can  also  be  connected 
together  in  series  along  with  normal  silicon  signal  diodes  to  produce  a  variety  of  different 
reference voltage output values as shown below. 
 
 
 
 
 
Zener Diodes Connected in Series 
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The values of the individual Zener diodes can be chosen to suit the application while the silicon 
diode will always drop about 0.6 - 0.7V in the  forward bias condition. The  supply  voltage, Vin 
must of course be higher than the largest output reference voltage and in our example above this 
is 19v. 
A  typical  zener  diode  for  general  electronic  circuits  is  the  500mW,  BZX55  series  or the  larger 
1.3W,  BZX85  series  were  the  zener  voltage  is  given  as,  for  example,  C7V5  for  a  7.5V  diode 
giving  a  diode  reference  number  of  BZX55C7V5.  The  500mW  series  of  zener  diodes  are 
available from about 2.4 up to about 100 volts and typically have the same sequence of values as 
used for the 5% (E24) resistor series with the individual voltage ratings for these small but very 
useful diodes are given in the table below. 
Zener Diode Standard Voltages 
  BZX55 Zener Diode Power Rating 500mW 
2.4V  2.7V  3.0V  3.3V  3.6V  3.9V  4.3V  4.7V 
5.1V  5.6V  6.2V  6.8V  7.5V  8.2V  9.1V  10V 
11V  12V  13V  15V  16V  18V  20V  22V 
24V  27V  30V  33V  36V  39V  43V  47V 
  BZX85 Zener Diode Power Rating 1.3W 
3.3V  3.6V  3.9V  4.3V  4.7V  5.1V  5.6  6.2V 
6.8V  7.5V  8.2V  9.1V  10V  11V  12V  13V 
15V  16V  18V  20V  22V  24V  27V  30V 
33V  36V  39V  43V  47V  51V  56V  62V 
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Zener Diode Clipping Circuits 
Thus far we have looked at how a zener diode can be used to regulate a constant DC source but 
what if the input signal was not steady state DC but an alternating AC waveform how would the 
zener diode react to a constantly changing signal. 
Diode  clipping  and  clamping  circuits  are  circuits  that  are  used to  shape  or  modify  an  input  AC 
waveform  (or  any  sinusoid)  producing  a  differently  shape  output  waveform  depending  on  the 
circuit arrangement. Diode clipper circuits are also called  limiters  because they  limit or clip-off 
the positive (or negative) part of an input AC signal. As zener clipper circuits limit or cut-off part 
of the waveform across them, they are mainly used for circuit protection or in waveform shaping 
circuits. For example,  if we wanted to clip an output waveform at +7.5V, we would use a 7.5V 
zener diode. If the output waveform tries to exceed the 7.5V limit, the zener diode will "clip-off" 
the excess  voltage  from the  input producing a waveform with a  flat top still keeping the output 
constant at +7.5V. Note that in the forward bias condition a zener diode is still a diode and when 
the AC waveform output goes negative below -0.7V, the zener diode turns "ON" like any normal 
silicon diode would and clips the output at -0.7V as shown below. 
Square Wave Signal 
 
The  back  to  back  connected  zener  diodes  can  be  used  as  an  AC  regulator  producing  what  is 
jokingly  called  a  "poor  man's  square  wave  generator".  Using  this  arrangement  we  can  clip  the 
waveform between a positive value of +7.5V and a negative value of -7.5V. If we wanted to clip 
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an  output  waveform  between  different  minimum  and  maximum  values  for  example,  +8V  and  -
6V, use would simply use two differently rated zener diodes. 
Note  that  the  output  will  actually  clip  the  AC  waveform  between  +8.7V  and  -6.7V  due  to  the 
addition of the  forward biasing diode  voltage, which adds another 0.7V voltage drop to it. This 
type  of  clipper  configuration  is  fairly  common  for  protecting  an  electronic  circuit  from  over 
voltage. The two zeners are generally placed across the power supply input terminals and during 
normal  operation,  one  of  the  zener  diodes  is  "OFF"  and  the  diodes  have  little  or  no  affect. 
However, if the input voltage waveform exceeds its limit, then the zeners turn "ON" and clip the 
input to protect the circuit. 
In the next tutorial about diodes, we will look at using the forward biased PN  junction of a diode 
to produce light. We know from the previous tutorials that when charge carriers move across the 
junction,  electrons  combine  with  holes  and  energy  is  lost  in  the  form  of  heat,  but  also  some  of 
this  energy  is  dissipated  as  photons  but  we  can  not  see  them.  If  we  place  a  translucent  lens 
around  the  junction,  visible  light  will  be  produced  and  the  diode  becomes  a  light  source.  This 
effect  produces  another  type  of  diode  known  commonly  as  the  Light  Emitting  Diode  which 
takes  advantage  of  this  light  producing  characteristic  to  emit  light  (photons)  in  a  variety  of 
colours and wavelengths. 
 
 
 
Light Emitting Diodes 
Light Emitting Diodes or LEDs, are among the  most widely used of all the different types of 
semiconductor diodes available today. They are the most visible type of diode, that emit a fairly 
narrow  bandwidth  of  either  visible  light  at  different  coloured  wavelengths,  invisible  infra-red 
light  for  remote  controls  or  laser  type  light  when  a  forward  current  is  passed  through  them.  A 
"Light  Emitting  Diode"  or  LED  as  it  is  more  commonly  called,  is  basically  just  a  specialised 
type  of  PN  junction  diode,  made  from  a  very  thin  layer  of  fairly  heavily  doped  semiconductor 
material. When the diode is forward biased, electrons from the semiconductors conduction band 
recombine  with  holes  from  the  valence  band  releasing  sufficient  energy  to  produce  photons 
which  emit  a  monochromatic  (single  colour)  of  light.  Because  of  this  thin  layer  a  reasonable 
number  of  these  photons  can  leave  the  junction  and  radiate  away  producing  a  coloured  light 
output.  Then  we  can  say  that  when  operated  in  a  forward  biased  direction  Light  Emitting 
Diodes are semiconductor devices that convert electrical energy into light energy. 
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The  construction  of  a  light  emitting  diode  is  very  different  from  that  of  a  normal  signal  diode. 
The  PN  junction  of  an  LED  is  surrounded  by  a  transparent,  hard  plastic  epoxy  resign 
hemispherical  shaped  shell  or  body  which  protects  the  LED  from  both  vibration  and  shock. 
Surprisingly, an LED junction does not actually emit that much light so the epoxy resin body is 
constructed  in  such  a  way  that  the  photons  of  light  emitted  by  the  junction  are  reflected  away 
from  the  surrounding  substrate  base  to  which  the  diode  is  attached  and  are  focused  upwards 
through the domed top of the LED, which itself acts like a lens concentrating the amount of light. 
This is why the emitted light appears to be brightest at the top of the LED. 
However, not all LEDs are made with a hemispherical shaped dome for their epoxy shell. Some 
LEDs  have a rectangular or cylindrical  shaped construction that has a  flat surface on top. Also, 
nearly all  LEDs  have their cathode, (K) terminal  identified  by either a  notch  or flat spot on the 
body, or by one of the leads being shorter than the other, (the Anode, A). 
Unlike  normal  incandescent  lamps  and  bulbs  which  generate  large  amounts  of  heat  when 
illuminated,  the  light  emitting  diode  produces  a  "cold"  generation  of  light which  leads  to  high 
efficiencies  than  the  normal  "light  bulb"  because  most  of  the  generated  energy  radiates away 
within the  visible  spectrum. Because LEDs  are solid-state devices, they can  be  extremely  small 
and durable and provide much longer lamp life than normal light sources. 
Light Emitting Diode Colours 
So how does a  light emitting diode get  its colour. Unlike  normal  signal diodes which are  made 
for  detection  or  power  rectification,  and  which  are  made  from  either  Germanium  or  Silicon 
semiconductor  materials,  Light  Emitting  Diodes  are  made  from  exotic  semiconductor 
compounds  such  as  Gallium  Arsenide  (GaAs),  Gallium  Phosphide  (GaP),  Gallium  Arsenide 
Phosphide  (GaAsP),  Silicon  Carbide  (SiC)  or  Gallium  Indium  Nitride  (GaInN)  all  mixed 
together at different ratios to produce a distinct wavelength of colour. Different LED compounds 
emit  light  in  specific  regions  of  the  visible  light  spectrum  and  therefore  produce  different 
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intensity  levels. The exact choice of the semiconductor material used will determine the overall 
wavelength of the photon light emissions and therefore the resulting colour of the light emitted. 
Thus,  the  actual  colour  of  a  light 
emitting  diode  is  determined  by  the 
wavelength  of  the  light  emitted,  which 
inturn  is  determined  by  the  actual 
semiconductor  compound  used  in 
forming  the  PN  junction  during 
manufacture  and  NOT  by  the  colouring 
of the LEDs plastic body although these 
are  slightly  coloured  to  both  enhance 
the light and indicate its colour when its 
not  be  used.  Light  emitting  diodes  are 
available  in  a  wide  range  of  colours  with  the  most  common  being  RED,  AMBER,   YELLOW  
and GREEN and are thus widely used as visual indicators and as moving light displays. 
Recently developed blue and white coloured LEDs are also available  but these tend to be much 
more expensive than the normal standard colours due to the production costs of mixing together 
two or  more  complementary  colours  at  an  exact  ratio  within  the  semiconductor  compound  and 
also by injecting nitrogen atoms into the crystal structure during the doping process. 
From the table above we can see that the  main P-type dopant used  in the  manufacture of  Light 
Emitting  Diodes  is  Gallium  (Ga,  atomic  number  31)  and  that  the  main  N-type  dopant  used  is 
Arsenic  (As,  atomic  number  31)  giving  the  resulting  compound  of  Gallium  Arsenide  (GaAs) 
crystal  structure.  The  problem  with  using  Gallium  Arsenide  on  its  own  as  the  semiconductor 
compound  is that  it radiates  large amounts of  low brightness  infra-red radiation (850nm-940nm 
approx.) from its junction when a forward current is flowing through it. This infra-red light is ok 
for  television  remote  controls  but  not  very  useful  if  we  want  to  use  the  LED  as  an  indicating 
light. But by adding Phosphorus (P, atomic number 15), as a third dopant the overall wavelength 
of  the  emitted  radiation  is  reduced  to  below  680nm  giving  visible  red  light  to  the  human  eye. 
Further refinements in the doping process of the PN junction have resulted in a range of colours 
spanning the spectrum of visible light as we have seen above as well as infra-red and ultra-violet 
wavelengths. 
By  mixing  together  a  variety  of  semiconductor, metal  and  gas  compounds  the  following  list  of 
LEDs can be produced. 
-  Gallium Arsenide (GaAs) - infra-red 
Typical LED Characteristics 
Semiconductor 
Material 
Wavelength  Colour  V
F
 @ 20mA 
GaAs  850-940nm  Infra-Red 1.2v 
GaAsP  630-660nm  Red  1.8v 
GaAsP  605-620nm  Amber  2.0v 
GaAsP:N  585-595nm  Yellow  2.2v 
AlGaP  550-570nm  Green  3.5v 
SiC  430-505nm  Blue  3.6v 
GaInN  450nm  White  4.0v 
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-  Gallium Arsenide Phosphide (GaAsP) - red to infra-red, orange 
-  Aluminium Gallium Arsenide Phosphide (AlGaAsP) - high-brightness red, orange-red, orange, 
and yellow 
-  Gallium Phosphide (GaP) - red, yellow and green 
-  Aluminium Gallium Phosphide (AlGaP) - green 
-  Gallium Nitride (GaN) - green, emerald green 
-  Gallium Indium Nitride (GaInN) - near ultraviolet, bluish-green and blue 
-  Silicon Carbide (SiC) - blue as a substrate 
-  Zinc Selenide (ZnSe) - blue 
-  Aluminium Gallium Nitride (AlGaN) - ultraviolet 
Like  conventional  PN  junction  diodes,  LEDs  are  current-dependent  devices  with  its  forward 
voltage drop V
F
, depending on the semiconductor compound (its light colour) and on the forward 
biased LED current. The point where conduction begins and light is produced is about 1.2V for a 
standard red LED to about 3.6V for a blue LED. The exact voltage drop will of course depend on 
the  manufacturer  because  of  the  different  dopant  materials  and  wavelengths  used.  The  voltage 
drop  across  the  LED  at  a  particular  current  value,  for  example  20mA,  will  also  depend  on  the 
initial  conduction  V
F
  point.  As  an  LED  is  effectively  a  diode,  its  forward  current  to  voltage 
characteristics curves can be plotted for each diode colour as shown below. 
Light Emitting Diodes I-V Characteristics. 
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Light Emitting Diode (LED) Schematic symbol and its I-V Characteristics Curves showing 
the different colours available. 
Before a light emitting diode can "emit" any form of light it needs a current to flow through it, as 
it is a current dependant device with their light output intensity being direct ly proportional to the 
forward  current  flowing  through  the  LED.  As  the  LED  is  to  be  connected  in  a  forward  bias 
condition  across  a  power  supply  it  should  be  current  limited  using  a  series  resistor to  protect  it 
from  excessive  current  flow.  Never  connect  an  LED  directly  to  a  battery  or  power  supply  as  it 
will be destroyed almost instantly because too much current will pass through and burn it out. 
From the table above we can see that each LED has its own forward voltage drop across the PN 
junction  and  this  parameter  which  is  determined  by  the  semiconductor  material  used,  is  the 
forward  voltage  drop  for  a  specified  amount  of  forward  conduction  current,  typically  for  a 
forward current of 20mA. In most cases LEDs are operated from a low voltage DC supply, with 
a series resistor, R
S
 used to limit the forward current to a safe value from say 5mA for a simple 
LED indicator to 30mA or more where a high brightness light output is needed. 
LED Series Resistance. 
The series resistor value R
S
 is calculated by simply using Ohms Law, by knowing the required 
forward  current  I
F
  of  the  LED,  the  supply  voltage  V
S
  across  the  combination  and  the  expected 
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forward voltage drop of the LED, V
F
 at the required current level, the current limiting resistor is 
calculated as: 
LED Series Resistor Circuit 
 
Example No1 
An  amber  coloured  LED  with  a  forward  volt  drop  of  2  volts  is  to  be  connected  to  a  5.0v 
stabilised  DC  power  supply.  Using  the  circuit  above  calculate  the  value  of  the  series  resistor 
required  to  limit  the  forward  current  to  less  than  10mA.  Also  calculate  the  current  flowing 
through the diode if a 100 series resistor is used instead of the calculated first. 
1). series resistor value at 10mA. 
 
2). with a 100 series resistor. 
 
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We remember from the Resistors tutorials, that resistors come in standard preferred values. Our 
first calculation above shows to limit the current flowing through the LED to 10mA exactly, we 
would  require  a  300  resistor.  In  the  E12  series  of  resistors  there  is  no  300  resistor  so  we 
would  need  to  choose the  next  highest  value,  which  is  330.  A  quick  re-calculation  shows  the 
new forward current value is now 9.1mA, and this is ok. 
LED Driver Circuits 
Now that  we  know  what  is  an  LED,  we  need  some  way  of  controlling  it  by  switching  it  "ON" 
and  "OFF".  The  output  stages  of  both  TTL  and  CMOS  logic  gates  can  both  source  and  sink 
useful  amounts  of  current  therefore  can  be  used  to  drive  an  LED.  Normal  integrated  circuits 
(ICs)  have  an  output  drive  current  of  up  to  50mA  in  the  sink  mode  configuration,  but  have  an 
internally limited output current of about 30mA in the source mode configuration. Either way the 
LED  current  must  be  limited  to  a  safe  value  using  a  series  resistor  as  we  have  already  seen. 
Below are some examples of driving light emitting diodes using inverting ICs but the idea is the 
same for any type of integrated circuit output whether combinational or sequential.  
IC Driver Circuit 
 
If more than one LED requires driving at the same time, such as in large LED arrays, or the load 
current  is  to  high  for  the  integrated  circuit  or  we  may  just  want  to  use  discrete  components 
instead  of  ICs,  then  an  alternative  way  of  driving  the  LEDs  using  either  bipolar  NPN  or  PNP 
transistors as switches is given below. Again as before, a series resistor, R
S
 is required to limit 
the LED current. 
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Transistor Driver Circuit 
 
 
The  brightness  of  a  light  emitting  diode  cannot  be  controlled  by  simply  varying  the  current 
flowing  through  it.  Allowing  more  current to  flow  through  the  LED  will  make  it  glow  brighter 
but will also cause it to dissipate more heat. LEDs are designed to produce a set amount of light 
operating at a specific forward current ranging from about 10 to 20mA. In situations were power 
savings are important, less current may be possible. However, reducing the current to below say 
5mA may dim its light output too much or even turn the LED "OFF" completely. A much better 
way  to  control  the  brightness  of  LEDs  is  to  use  a  control  process  known  as  "Pulse  Width 
Modulation"  or  PWM,  in  which  the  LED  is  repeatedly  turned  "ON"  and  "OFF"  at  varying 
frequencies depending upon the required light intensity. 
LED Light Intensity using PWM 
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When higher light outputs are required, a pulse width modulated current with a fairly short duty 
cycle  ("ON-OFF"  Ratio)  allows  the  diode  current  and  therefore  the  output  light  intensity  to  be 
increased  significantly  during  the  actual  pulses,  while  still  keeping  the  LEDs  "average  current 
level"  and  power  dissipation  within  safe  limits.  This  "ON-OFF"  flashing  condition  does  not 
affect what is seen as the human eyes fills in the gaps between the "ON" and "OFF" light pulses, 
providing the pulse frequency  is high enough, making it appear as a continuous light output. So 
pulses  at  a  frequency  of  100Hz  or  more  actually  appear  brighter  to  the  eye  than  a  continuous 
light of the same average intensity. 
Multi-coloured Light Emitting Diode 
LEDs  are  available  in  a  wide  range  of  shapes,  colours  and  various  sizes  with  different  light 
output intensities available, with the most common (and cheapest to produce) being the standard 
5mm  Red  Gallium  Arsenide  Phosphide  (GaAsP)  LED.  LED's  are  also  available  in  various 
"packages"  arranged  to  produce  both  letters  and  numbers  with  the  most  common  being  that  of 
the  "seven  segment  display"  arrangement.  Nowadays,  full  colour  flat  screen  LED  displays  are 
available with a  large  number of dedicated ICs  available  for driving the displays directly.  Most 
light  emitting  diodes  produce  just  a  single  output  of  coloured  light  however,  multi-coloured 
LEDs  are  now  available  that  can  produce  a  range  of  different  colours  from  within  a  single 
device. Most of these are actually two or three LEDs fabricated within a single package. 
Bicolour Light Emitting Diodes 
A bicolour light emitting diode has two LEDs chips connected together in "inverse parallel" (one 
forwards, one backwards) combined in one single package. Bicolour LEDs can produce any one 
of three colours  for example, a red colour is emitted when the device  is connected with  current 
flowing  in  one  direction  and  a  green  colour  is  emitted  when  it  is  biased  in  the  other  direction. 
This type of  bi-directional  arrangement  is useful  for giving polarity  indication,  for example, the 
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correct connection of batteries or power supplies etc. Also, a bi-directional current produces both 
colours  mixed  together  as  the  two  LEDs  would  take  it  in  turn  to  illuminate  if  the  device  was 
connected (via a suitable resistor) to a low voltage, low frequency AC supply. 
A Bicolour LED 
 
LED 
Selected 
Terminal A 
AC 
+  - 
LED 1  ON  OFF  ON 
LED 2  OFF  ON  ON 
Colour  Green  Red  Yellow 
 
Tricolour Light Emitting Diodes 
The most popular type of tricolour LED comprises of a single Red and a Green LED combined 
in  one  package  with  their  cathode  terminals  connected  together  producing  a  three  terminal 
device. They are called tricolour LEDs because they can give out a single red or a green colour 
by  turning  "ON"  only  one  LED  at  a  time.  They  can  also  generate  additional  shades  of  colours 
(the third colour) such as Orange or Yellow by turning "ON" the two LEDs in different ratios of 
forward current as shown in the table thereby generating 4 different colours from just two diode 
junctions. 
A Multi or Tricolour LED 
 
Output 
Colour 
Red  Orange  Yellow  Green 
LED  1 
Current 
0  5mA  9.5mA  15mA 
LED  2 
Current 
10mA  6.5mA  3.5mA  0 
 
 
LED Displays 
As  well  as  individual  colour  or  multi-colour  LEDs,  several  light  emitting  diodes  can  be 
combined together within a  single package to produce displays such as  bargraphs, strips, arrays 
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and  seven  segment  displays.  A  seven  segment  LED  display  provides  a  very  convenient  way 
when decoded properly of displaying  information or digital data  in the  form of  numbers,  letters 
or even alpha-numerical characters and  as their  name  suggests, they consist of seven  individual 
LEDs (the segments), within one single display package. 
In order to produce the required  numbers or characters  from 0 to 9 and  A to F respectively, on 
the display the correct combination of  LED segments  need to be  illuminated. A standard  seven 
segment LED display generally has eight input connections, one for each LED segment and one 
that acts as a common terminal or connection for all the internal segments. 
-  The  Common  Cathode  Display  (CCD) - In  the  common  cathode  display,  all  the  cathode 
connections  of  the  LEDs  are  joined  together  and  the  individual  segments  are  illuminated  by 
application of a HIGH, logic "1" signal. 
-    
-  The Common  Anode Display (CAD) - In the common anode display, all the anode connections 
of  the  LEDs  are  joined  together  and  the  individual  segments  are  illuminated  by  connecting  the 
terminals to a LOW, logic "0" signal. 
A Typical Seven Segment LED Display 
 
Opto-coupler 
Finally, another useful application of light emitting diodes is Opto-coupling. An opto-coupler or 
opto-isolator  as  it  is  also  called,  is  a  single  electronic  device  that  consists  of  a  light  emitting 
diode  combined  with  either  a  photo-diode,  photo-transistor  or  photo-triac  to  provide  an  optical 
signal  path  between  an  input  connection  and  an  output  connection  while  maintaining  electrical 
isolation  between two circuits. An opto-isolator consists of a  light proof plastic  body that has  a 
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typical  breakdown  voltages  between  the  input  (photo-diode)  and  the  output  (photo-transistor) 
circuit of up to 5000 volts. This electrical  isolation  is especially useful  where the  signal  from  a 
low voltage circuit such as a battery powered circuit, computer or microcontroller, is required to 
operate or control another external circuit operating at a potentially dangerous mains voltage. 
Photo-diode and Photo-transistor Opto-couplers 
 
The two components used in an opto-isolator, an optical transmitter such as an infra-red emitting 
Gallium  Arsenide  LED  and  an  optical  receiver  such  as  a  photo-transistor  are  closely  optically 
coupled  and  use  light  to  send  signals  and/or  information  between  its  input  and  output.  This 
allows  information  to  be  transferred  between  circuits  without  an  electrical  connection  or 
common ground potential. Opto-isolators are digital or switching devices, so they transfer either 
"ON-OFF"  control  signals  or  digital  data.  Analogue  signals  can  be  transferred  by  means  of 
frequency or pulse-width modulation. 
 
Diode 
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Figure 1: Closeup of a diode, showing the square shaped semiconductor crystal  (black object on 
left). 
 
 
Figure 2: Various semiconductor diodes. Bottom: A  bridge rectifier. In  most diodes, a white or 
black  painted  band  identifies  the  cathode  terminal,  that  is,  the  terminal  which  conventional 
current flows out of when the diode is conducting. 
 
 
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Figure  3:  Structure of  a  vacuum  tube  diode.  The  filament  may  be  bare,  or  more  commonly  (as 
shown here), embedded within and insulated from an enclosing cathode 
In  electronics,  a  diode  is  a  two-terminal  electronic  component  that  conducts  electric  current  in 
only  one  direction.  The  term  usually  refers  to  a  semiconductor  diode,  the  most  common  type 
today.  This  is  a  crystalline  piece  of  semiconductor  material  connected  to  two  electrical 
terminals.
[1]
 A vacuum tube diode (now little used except in some high-power technologies) is a 
vacuum tube with two electrodes; a plate and a cathode. 
The  most  common  function  of  a  diode  is  to  allow  an  electric  current  to  pass  in  one  direction 
(called  the  diode's  forward  direction)  while  blocking  current  in  the  opposite  direction  (the 
reverse  direction).  Thus,  the  diode  can  be  thought of  as  an  electronic  version  of  a  check  valve. 
This  unidirectional  behavior  is  called  rectification,  and  is  used  to  convert  alternating  current  to 
direct current, and to extract modulation from radio signals in radio receivers. 
However, diodes can have more complicated behavior than this simple on-off action, due to their 
complex  non-linear  electrical  characteristics,  which  can  be  tailored  by  varying  the  construction 
of their P-N junction. These are exploited in special purpose diodes that perform many different 
functions.  For  example,  specialized  diodes  are  used  to  regulate  voltage  (Zener  diodes),  to 
electronically  tune  radio  and  TV  receivers  (varactor  diodes),  to  generate  radio  frequency 
oscillations (tunnel diodes), and to produce light (light emitting diodes). 
Diodes  were  the  first  semiconductor  electronic  devices.  The  discovery  of  crystals'  rectifying 
abilities  was  made  by  German  physicist  Ferdinand  Braun  in  1874.  The  first  semiconductor 
diodes, called cat's whisker diodes were made of crystals of minerals such as galena. Today most 
diodes are made of silicon, but other semiconductors such as germanium are sometimes used.
[2]
 
o   
Thermionic and gaseous state diodes 
 
 
Figure  4:  The  symbol  for  an  indirect  heated  vacuum  tube  diode.  From  top  to  bottom,  the 
components are the anode, the cathode, and the heater filament. 
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Thermionic diodes are thermionic-valve devices (also known as vacuum tubes, tubes, or valves), 
which  are  arrangements  of  electrodes  surrounded  by  a  vacuum  within  a  glass  envelope.  Early 
examples were fairly similar in appearance to incandescent light bulbs. 
In  thermionic  valve  diodes,  a  current  through  the  heater  filament  indirectly  heats  the  cathode, 
another  internal  electrode  treated  with  a  mixture  of  barium  and  strontium  oxides,  which  are 
oxides  of  alkaline  earth  metals;  these  substances  are  chosen  because  they  have  a  small  work 
function.  (Some  valves  use  direct  heating,  in  which  a  tungsten  filament  acts  as  both  heater  and 
cathode.)  The  heat  causes  thermionic  emission  of  electrons  into  the  vacuum.  In  forward 
operation,  a  surrounding  metal  electrode  called  the  anode  is  positively  charged  so  that  it 
electrostatically  attracts  the  emitted  electrons.  However,  electrons  are  not  easily  released  from 
the  unheated  anode  surface  when  the  voltage  polarity  is  reversed.  Hence,  any  reverse  flow  is 
negligible. 
For much of the 20th century, thermionic  valve diodes were used  in analog signal  applications, 
and as rectifiers in many power supplies. Today, valve diodes are only used in niche applications 
such  as  rectifiers  in  electric  guitar  and  high-end  audio  amplifiers  as  well  as  specialized  high-
voltage equipment. 
Semiconductor diodes 
A  modern  semiconductor  diode  is  made  of  a  crystal  of  semiconductor  like  silicon  that  has 
impurities  added  to  it  to  create  a  region  on  one  side  that  contains  negative  charge  carriers 
(electrons),  called  n-type  semiconductor,  and  a  region  on  the  other  side  that  contains  positive 
charge  carriers  (holes),  called  p-type  semiconductor. The  diode's  terminals  are  attached  to  each 
of  these  regions.  The  boundary  within  the  crystal  between  these  two  regions,  called  a  PN 
junction, is where the action of the diode takes place. The crystal conducts  conventional current 
in a direction from the p-type side (called the anode) to the n-type side (called the cathode), but 
not in the opposite direction. 
Another type of semiconductor diode, the Schottky diode, is formed from the contact between a 
metal and a semiconductor rather than by a p-n junction. 
Currentvoltage characteristic 
A semiconductor diodes behavior in a circuit is given by its currentvoltage characteristic, or I
V  graph  (see  graph  below).  The  shape  of  the  curve  is  determined  by  the  transport  of  charge 
carriers  through  the  so-called  depletion  layer  or  depletion  region  that  exists  at  the  p-n  junction 
between  differing  semiconductors.  When  a  p-n  junction  is  first  created,  conduction  band 
(mobile)  electrons  from  the  N-doped  region  diffuse  into  the  P-doped  region  where  there  is  a 
large  population  of  holes  (vacant  places  for  electrons)  with  which  the  electrons  recombine. 
When  a  mobile  electron  recombines  with  a  hole,  both  hole  and  electron  vanish,  leaving  behind 
an  immobile  positively  charged  donor  (dopant)  on  the  N-side  and  negatively  charged  acceptor 
(dopant) on the P-side. The region around the p-n  junction  becomes depleted of  charge carriers 
and thus behaves as an insulator. 
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However,  the  width  of  the  depletion  region  (called  the  depletion  width)  cannot  grow  without 
limit. For each electron-hole pair that recombines, a positively charged dopant ion is left behind 
in the N-doped region, and a negatively charged dopant ion is left behind in the P-doped region. 
As  recombination  proceeds  more  ions  are  created,  an  increasing  electric  field  develops  through 
the depletion zone which acts to slow and then finally stop recombination. At this point, there is 
a built-in potential across the depletion zone. 
If an  external  voltage  is placed across the diode  with the same polarit y as the  built-in potential, 
the  depletion  zone  continues  to  act  as  an  insulator,  preventing  any  significant  electric  current 
flow (unless electron/hole pairs are actively  being created in the  junction by,  for instance,  light. 
see  photodiode).  This  is  the  reverse  bias  phenomenon.  However,  if  the  polarity  of  the  external 
voltage  opposes  the  built-in  potential,  recombination  can  once  again  proceed,  resulting  in 
substantial  electric  current  through  the  p-n  junction  (i.e.  substantial  numbers  of  electrons  and 
holes recombine at the junction). For silicon diodes, the built-in potential is approximately 0.7 V 
(0.3 V for Germanium and 0.2 V for Schottky). Thus, if an external current is passed through the 
diode,  about  0.7  V  will  be  developed  across  the  diode  such  that  the  P-doped  region  is  positive 
with  respect  to the  N-doped  region  and  the  diode  is  said  to  be  turned  on  as  it  has  a  forward 
bias. 
 
Figure 5: IV characteristics of a P-N junction diode (not to scale). 
A diodes  'IV characteristic' can  be approximated by  four regions of operation (see the  figure 
at right). 
At  very  large  reverse  bias,  beyond  the  peak  inverse  voltage  or  PIV,  a  process  called  reverse 
breakdown occurs which causes a large increase in current (i.e. a large number of electrons and 
holes  are  created  at,  and  move  away  from  the  pn  junction)  that  usually  damages  the  device 
permanently. The avalanche diode is deliberately designed for use in the avalanche region. In the 
zener  diode,  the  concept  of  PIV  is  not  applicable.  A  zener  diode  contains  a  heavily  doped  p-n 
junction  allowing  electrons  to  tunnel  from  the  valence  band  of  the  p-type  material  to  the 
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conduction  band  of  the  n-type  material,  such  that  the  reverse  voltage  is  clamped  to  a  known 
value (called the zener voltage), and avalanche does not occur. Both devices, however, do have a 
limit to the maximum current and power in the clamped reverse voltage region. Also, following 
the end of forward conduction in any diode, there is reverse current for a short time. The device 
does not attain its full blocking capability until the reverse current ceases. 
The  second  region,  at  reverse  biases  more  positive  than  the  PIV,  has  only  a  very  small  reverse 
saturation current. In the reverse bias region for a normal P-N rectifier diode, the current through 
the  device  is  very  low  (in  the  A  range).  However,  this  is  temperature  dependent,  and  at 
suffiently  high  temperatures,  a  substantial  amount  of  reverse  current  can  be  observed  (mA  or 
more). 
The third region is forward but small bias, where only a small forward current is conducted. 
As  the  potential  difference  is  increased  above  an  arbitrarily  defined  cut-in  voltage  or  on-
voltage or diode forward voltage drop (V
d
), the diode current becomes appreciable (the level 
of current considered  appreciable and the value of cut-in  voltage depends on the application), 
and  the  diode  presents  a  very  low  resistance.  The  currentvoltage  curve  is  exponential.  In  a 
normal silicon diode at rated currents, the arbitrary cut-in voltage is defined as 0.6 to 0.7 volts. 
The  value  is  different  for  other  diode  types    Schottky  diodes  can  be  rated  as  low  as  0.2  V, 
Germanium diodes 0.25-0.3 V, and red or blue  light-emitting diodes (LEDs) can have values of 
1.4 V and 4.0 V respectively. 
At  higher  currents  the  forward  voltage  drop  of  the  diode  increases.  A  drop  of  1  V  to  1.5  V  is 
typical at full rated current for power diodes. 
Shockley diode equation 
The Shockley ideal diode equation or the diode law (named after transistor co-inventor William 
Bradford Shockley,  not to be confused with  tetrode  inventor  Walter H. Schottky) gives the IV 
characteristic of an ideal diode in either forward or reverse bias (or no bias). The equation is: 
 
where 
I is the diode current, 
I
S
 is the reverse bias saturation current (or scale current), 
V
D
 is the voltage across the diode, 
V
T
 is the thermal voltage, and 
n  is  the  ideality  factor,  also  known  as  the  quality  factor  or  sometimes  emission 
coefficient. The  ideality  factor  n varies  from 1 to 2 depending on  the fabrication process 
and semiconductor material and in many cases is assumed to be approximately equal to 1 
(thus the notation n is omitted). 
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The  thermal  voltage  V
T
  is  approximately  25.85  mV  at  300  K,  a  temperature  close  to  room 
temperature  commonly  used  in  device  simulation  software.  At  any  temperature  it  is  a  known 
constant defined by: 
 
where k is the Boltzmann constant, T is the absolute temperature of the p-n junction, and q is the 
magnitude of charge on an electron (the elementary charge). 
The Shockley ideal diode equation or the diode law is derived with the assumption that the only 
processes giving rise to the current  in the diode are drift (due to electrical  field), diffusion, and 
thermal  recombination-generation.  It  also  assumes  that  the  recombination-generation  (R-G) 
current  in  the  depletion  region  is  insignificant.  This  means  that  the  Shockley  equation  doesnt 
account for the processes involved in reverse breakdown and photon-assisted R-G. Additionally, 
it  doesnt  describe  the  leveling  off  of  the  IV  curve  at  high  forward  bias  due  to  internal 
resistance. 
Under  reverse  bias  voltages  (see  Figure  5)  the  exponential  in  the  diode  equation  is  negligible, 
and  the  current  is  a  constant  (negative)  reverse  current  value  of  I
S
.  The  reverse  breakdown 
region is not modeled by the Shockley diode equation. 
For even rather small forward bias voltages (see Figure 5) the exponential is very large because 
the thermal voltage is very small, so the subtracted 1 in the diode equation is negligible and the 
forward diode current is often approximated as 
 
The use of the diode equation in circuit problems is illustrated in the article on diode modeling. 
Small-signal behaviour 
For  circuit  design,  a  small-signal  model  of  the  diode  behavior  often  proves  useful.  A  specific 
example of diode modeling is discussed in the article on small-signal circuits. 
Types of semiconductor diode 
       
Diode 
Zener 
diode
Schottky 
diode
Tunnel 
diode
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Light-emitting 
diode 
Photodiode  Varicap  Silicon controlled rectifier 
Figure 6: Some diode symbols. 
 
 
Figure  7:  Typical  diode  packages  in  same  alignment  as  diode  symbol.  Thin  bar  depicts  the 
cathode. 
 
 
Figure 8: Several types of diodes. The scale is centimeters. 
There are several types of junction diodes, which either emphasize a different physical aspect of 
a  diode  often  by  geometric  scaling,  doping  level,  choosing  the  right  electrodes,  are  just  an 
application of a diode in a special circuit, or are really different devices like the Gunn and laser 
diode and the MOSFET: 
Normal  (p-n)  diodes,  which  operate  as  described  above,  are  usually  made  of  doped  silicon  or, 
more  rarely,  germanium.  Before  the  development  of  modern  silicon  power  rectifier  diodes, 
cuprous  oxide  and  later  selenium  was  used;  its  low  efficiency  gave  it  a  much  higher  forward 
voltage  drop  (typically  1.41.7 V  per  cell,  with  multiple  cells  stacked  to  increase  the  peak 
inverse  voltage  rating  in  high  voltage  rectifiers),  and  required  a  large  heat  sink  (often  an 
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extension  of  the  diodes  metal  substrate),  much  larger  than  a  silicon  diode  of  the  same  current 
ratings  would  require.  The  vast  majority  of  all  diodes  are  the  p-n  diodes  found  in  CMOS 
integrated circuits, which include two diodes per pin and many other internal diodes. 
Avalanche diodes 
Diodes  that  conduct  in  the  reverse  direction  when  the  reverse  bias  voltage  exceeds  the 
breakdown  voltage.  These  are  electrically  very  similar  to  Zener  diodes,  and  are  often 
mistakenly called Zener diodes, but break down by a different mechanism, the avalanche 
effect. This occurs when the reverse electric field across the p-n junction causes a wave of 
ionization, reminiscent of an avalanche, leading to a large current. Avalanche diodes are 
designed  to  break  down  at  a  well-defined  reverse  voltage  without  being  destroyed.  The 
difference  between  the  avalanche  diode  (which  has  a  reverse  breakdown  above  about 
6.2 V)  and  the  Zener  is  that  the  channel  length  of  the  former  exceeds  the  mean  free 
path  of  the  electrons,  so  there  are  collisions  between  them  on  the  way  out.  The  only 
practical  difference  is  that  the  two  types  have  temperature  coefficients  of  opposite 
polarities. 
Cats whisker or crystal diodes 
These  are  a  type  of  point-contact  diode.  The  cats  whisker  diode  consists  of  a  thin  or 
sharpened  metal  wire  pressed  against  a  semiconducting  crystal,  typically  galena  or  a 
piece  of  coal.
[9]
  The  wire  forms  the  anode  and  the  crystal  forms  the  cathode.  Cats 
whisker  diodes  were  also  called  crystal  diodes  and  found  application  in  crystal  radio 
receivers.  Cats  whisker  diodes  are  generally  obsolete,  but  may  be  available  from  a  few 
manufacturers.
[citation needed]
 
Constant current diodes 
These are actually a JFET
[10]
 with the gate shorted to the source, and function like a two-
terminal current-limiter analog to the Zener diode, which is limiting voltage. They allow 
a  current  through  them  to  rise  to  a  certain  value,  and  then  level  off  at  a  specific  value. 
Also  called  CLDs,  constant-current  diodes,  diode-connected  transistors,  or  current-
regulating diodes. 
Esaki or tunnel diodes 
These  have  a  region  of  operation  showing  negative  resistance  caused  by  quantum 
tunneling, thus allowing amplification of signals and very simple bistable circuits. These 
diodes are also the type most resistant to nuclear radiation. 
Gunn diodes 
These are similar to tunnel diodes in that they are made of materials such as GaAs or InP 
that  exhibit  a  region  of  negative  differential  resistance.  With  appropriate  biasing,  dipole 
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domains form and travel across the diode, allowing high frequency  microwave oscillators 
to be built. 
Light-emitting diodes (LEDs) 
In  a  diode  formed  from  a  direct  band-gap  semiconductor,  such  as  gallium  arsenide, 
carriers  that  cross  the  junction  emit  photons  when  they  recombine  with  the  majority 
carrier on the other side. Depending on the material,  wavelengths (or colors)
[11]
 from the 
infrared to the near ultraviolet may be produced.
[12]
 The forward potential of these diodes 
depends  on  the  wavelength  of  the  emitted  photons:  1.2 V  corresponds  to  red,  2.4 V  to 
violet.  The  first  LEDs  were  red  and  yellow,  and  higher-frequency  diodes  have  been 
developed  over  time.  All  LEDs  produce  incoherent,  narrow-spectrum  light;  white 
LEDs are actually combinations of three LEDs of a different color, or a blue LED with a 
yellow  scintillator  coating.  LEDs  can  also  be  used  as  low-efficiency  photodiodes  in 
signal  applications.  An  LED  may  be  paired  with  a  photodiode  or  phototransistor  in  the 
same package, to form an opto-isolator. 
Laser diodes 
When  an  LED-like  structure  is  contained  in  a  resonant  cavity  formed  by  polishing  the 
parallel  end  faces,  a  laser  can  be  formed.  Laser  diodes  are  commonly  used  in  optical 
storage devices and for high speed optical communication. 
Peltier diodes 
These diodes are used as sensors, heat engines for thermoelectric cooling. Charge carriers 
absorb and emit their band gap energies as heat. 
Photodiodes 
All  semiconductors  are  subject  to  optical  charge  carrier  generation.  This  is  typically  an 
undesired  effect,  so  most  semiconductors  are  packaged  in  light  blocking  material. 
Photodiodes are intended to sense light(photodetector), so they are packaged in materials 
that allow light to pass, and are usually PIN (the kind of diode most sensitive to light).
[13]
 
A  photodiode  can  be  used  in  solar  cells,  in  photometry,  or  in  optical  communications. 
Multiple photodiodes may be packaged in a single device, either as a linear array or as a 
two-dimensional  array.  These  arrays  should  not  be  confused  with  charge-coupled 
devices. 
Point-contact diodes 
These  work  the  same  as  the  junction  semiconductor  diodes  described  above,  but  their 
construction is simpler. A block of n-type semiconductor is built, and a conducting sharp-
point contact made with some group-3 metal is placed in contact with the semiconductor. 
Some  metal  migrates  into  the  semiconductor  to  make  a  small  region  of  p-type 
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semiconductor near the  contact. The  long-popular 1N34 germanium  version  is still used 
in radio receivers as a detector and occasionally in specialized analog electronics. 
PIN diodes 
A PIN diode has a central un-doped, or intrinsic, layer, forming a p-type/intrinsic/n-type 
structure.
[14]
  They  are  used  as  radio  frequency  switches  and  attenuators.  They  are  also 
used  as  large  volume  ionizing  radiation  detectors and  as  photodetectors.  PIN  diodes  are 
also  used  in  power  electronics,  as  their  central  layer  can  withstand  high  voltages. 
Furthermore, the PIN structure can be found in many power semiconductor devices, such 
as IGBTs, power MOSFETs, and thyristors. 
Schottky diodes 
Schottky  diodes  are  constructed  from  a  metal  to  semiconductor  contact.  They  have  a 
lower  forward  voltage  drop  than  p-n  junction  diodes.  Their  forward  voltage  drop  at 
forward  currents  of  about  1 mA  is  in  the  range  0.15 V  to  0.45 V,  which  makes  them 
useful in voltage clamping applications and prevention of transistor saturation. They can 
also  be  used  as  low  loss  rectifiers  although  their  reverse  leakage  current  is  generally 
higher  than  that  of  other  diodes.  Schottky  diodes  are  majority  carrier  devices  and  so  do 
not suffer  from  minority carrier storage problems that slow down  many other diodes   
so they have a faster reverse recovery than p-n junction diodes. They also tend to have 
much  lower  junction  capacitance  than  p-n  diodes  which  provides  for  high  switching 
speeds  and  their  use  in  high-speed  circuitry  and  RF  devices  such  as  switched-mode 
power supply, mixers and detectors. 
Super barrier diodes 
Super barrier diodes are rectifier diodes that incorporate the low forward voltage drop of 
the Schottky diode with the surge-handling capability and low reverse leakage current of 
a normal p-n junction diode. 
Gold-doped diodes 
As  a  dopant,  gold  (or  platinum)  acts  as  recombination  centers,  which  help  a  fast 
recombination of minority carriers. This allows the diode to operate at signal frequencies, 
at the expense of a higher forward voltage drop. Gold doped diodes are faster than other 
p-n  diodes  (but  not  as  fast  as  Schottky  diodes).  They  also  have  less  reverse-current 
leakage  than  Schottky  diodes  (but  not  as  good  as  other  p-n  diodes).
[15][16]
  A  typical 
example is the 1N914. 
Snap-off or Step recovery diodes 
The term step recovery relates to the form of the reverse recovery characteristic of these 
devices. After a forward current has been passing in an SRD and the current is interrupted 
or  reversed,  the  reverse  conduction  will  cease  very  abruptly  (as  in  a  step  waveform). 
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SRDs  can  therefore  provide  very  fast  voltage  transitions  by  the  very  sudden 
disappearance of the charge carriers. 
Transient voltage suppression diode (TVS) 
These are avalanche diodes designed specifically  to protect other semiconductor devices 
from  high-voltage  transients.
[17]
  Their  p-n  junctions  have  a  much  larger  cross-sectional 
area  than  those  of  a  normal  diode,  allowing  them  to  conduct  large  currents  to  ground 
without sustaining damage. 
Varicap or varactor diodes 
These  are  used  as  voltage-controlled  capacitors.  These  are  important  in  PLL  (phase-
locked  loop) and FLL (frequency-locked  loop) circuits, allowing tuning circuits, such as 
those in television receivers, to lock quickly, replacing older designs that took a long time 
to warm up and lock. A PLL is faster than an FLL, but prone to integer harmonic locking 
(if  one  attempts  to  lock  to  a  broadband  signal).  They  also  enabled  tunable  oscillators  in 
early  discrete  tuning  of  radios,  where  a  cheap  and  stable,  but  fixed-frequency,  crystal 
oscillator provided the reference frequency for a voltage-controlled oscillator. 
Zener diodes 
Diodes  that  can  be  made  to  conduct  backwards.  This  effect,  called  Zener  breakdown, 
occurs at a precisely defined voltage, allowing the diode to be used as a precision voltage 
reference.  In  practical  voltage  reference  circuits  Zener  and  switching  diodes  are 
connected in series and opposite directions to balance the temperature coefficient to near 
zero.  Some  devices  labeled  as  high-voltage  Zener  diodes  are  actually  avalanche  diodes 
(see above). Two (equivalent) Zeners in series and in reverse order, in the same package, 
constitute a transient absorber (or  Transorb, a registered trademark). The  Zener diode  is 
named  for  Dr.  Clarence  Melvin  Zener  of  Southern  Illinois  University,  inventor  of  the 
device. 
Other  uses  for  semiconductor  diodes  include  sensing  temperature,  and  computing  analog 
logarithms (see Operational amplifier applications#Logarithmic). 
Numbering and coding schemes 
There  are  a  number  of  common,  standard  and  manufacturer-driven  numbering  and  coding 
schemes for diodes; the two most common being the EIA/JEDEC standard and the European Pro 
Electron standard: 
 EIA/JEDEC 
A  standardized  1N-series  numbering  system  was  introduced  in  the  US  by  EIA/JEDEC  (Joint 
Electron Device Engineering Council) about 1960. Among the most popular in this series were: 
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1N34A/1N270  (Germanium  signal),  1N914/1N4148  (Silicon  signal),  1N4001-1N4007  (Silicon 
1A power rectifier) and 1N54xx (Silicon 3A power rectifier)
[18][19][20]
 
Pro Electron 
The  European  Pro  Electron  coding  system  for  active  components  was  introduced  in  1966  and 
comprises  two  letters  followed  by  the  part  code.  The  first  letter  represents  the  semiconductor 
material  used  for  the  component  (A  =  Germanium  and  B  =  Silicon)  and  the  second  letter 
represents  the  general  function  of  the  part  (for  diodes:  A  =  low-power/signal,  B  =  Variable 
capacitance, X = Multiplier, Y = Rectifier and Z = Voltage reference), for example: 
-  AA-series germanium low-power/signal diodes (e.g.: AA119) 
-  BA-series silicon low-power/signal diodes (e.g.: BAT18 Silicon RF Switching Diode) 
-  BY-series silicon rectifier diodes (e.g.: BY127 1250V, 1A rectifier diode) 
-  BZ-series silicon zener diodes (e.g.: BZY88C4V7 4.7V zener diode) 
Other common numbering / coding systems (generally manufacturer-driven) include: 
-  GD-series germanium diodes (ed: GD9)  this is a very old coding system 
-  OA-series germanium diodes (e.g.: OA47)  a coding sequence developed by Mullard, a 
UK company 
As  well  as  these  common  codes,  many  manufacturers  or organisations  have  their  own  systems 
too  for example: 
-  HP diode 1901-0044 = JEDEC 1N4148 
-  UK military diode CV448 = Mullard type OA81 = GEC type GEX23 
Related devices 
-  Rectifier 
-  Transistor 
-  Thyristor or silicon controlled rectifier (SCR) 
-  TRIAC 
-  Diac 
-  Varistor 
In  optics,  an  equivalent  device  for  the  diode  but  with  laser  light  would  be  the  Optical  isolator, 
also known as an Optical Diode, that allows light to only pass in one direction. It uses a Faraday 
rotator as the main component. 
Applications 
Radio demodulation 
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The first use for the diode was the demodulation of amplitude modulated (AM) radio broadcasts. 
The  history of this discovery  is treated  in depth  in the  radio article. In summary, an  AM signal 
consists of alternating positive and negative peaks of voltage, whose  amplitude or envelope is 
proportional to the original audio signal. The diode (originally  a crystal diode)  rectifies the  AM 
radio  frequency  signal,  leaving  an  audio  signal  which  is  the  original  audio  signal,  minus 
atmospheric noise. The audio is extracted using a simple  filter and fed into an audio amplifier or 
transducer, which generates sound waves. 
 Power conversion 
Rectifiers are constructed from diodes, where they are used to convert  alternating current (AC) 
electricity  into  direct  current  (DC).  Automotive  alternators  are  a  common  example,  where  the 
diode,  which  rectifies  the  AC  into  DC,  provides  better  performance  than  the  commutator  of 
earlier  dynamo.  Similarly,  diodes  are  also  used  in  CockcroftWalton  voltage  multipliers  to 
convert AC into higher DC voltages. 
Over-voltage protection 
Diodes  are  frequently  used  to  conduct  damaging  high  voltages  away  from  sensitive  electronic 
devices.  They  are  usually  reverse-biased  (non-conducting)  under  normal  circumstances.  When 
the  voltage  rises  above  the  normal  range,  the  diodes  become  forward-biased  (conducting).  For 
example, diodes  are used  in (stepper  motor and H-bridge)  motor controller and relay circuits to 
de-energize coils rapidly without the damaging  voltage spikes that would otherwise occur. (Any 
diode  used  in  such  an  application  is  called  a  flyback  diode).  Many  integrated  circuits  also 
incorporate  diodes  on  the  connection  pins  to  prevent  external  voltages  from  damaging  their 
sensitive  transistors.  Specialized  diodes  are  used  to  protect  from  over-voltages  at  higher  power 
(see Diode types above). 
Logic gates 
Diodes  can  be  combined  with  other  components  to  construct  AND  and  OR  logic  gates.  This  is 
referred to as diode logic. 
 Ionizing radiation detectors 
In  addition  to  light,  mentioned  above,  semiconductor  diodes  are  sensitive  to  more  energetic 
radiation. In  electronics,  cosmic rays and other sources of  ionizing radiation cause  noise pulses 
and  single  and  multiple  bit  errors.  This  effect  is  sometimes  exploited  by  particle  detectors  to 
detect  radiation.  A  single  particle  of  radiation,  with  thousands  or  millions  of  electron  volts  of 
energy,  generates  many  charge  carrier  pairs,  as  its  energy  is  deposited  in  the  semiconductor 
material.  If  the  depletion  layer  is  large  enough  to  catch  the  whole  shower  or  to  stop  a  heavy 
particle,  a  fairly  accurate  measurement  of  the  particles  energy  can  be  made,  simply  by 
measuring the charge conducted and without the  complexity of  a  magnetic spectrometer or etc. 
These  semiconductor  radiation  detectors  need  efficient  and  uniform  charge  collection  and  low 
leakage current. They are often cooled by  liquid nitrogen. For longer range (about a centimetre) 
particles  they  need  a  very  large  depletion  depth  and  large  area.  For  short  range  particles,  they 
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need any contact or un-depleted semiconductor on at least one surface to be very thin. The back-
bias  voltages  are  near  breakdown  (around  a  thousand  volts  per  centimetre).  Germanium  and 
silicon  are  common  materials.  Some  of  these  detectors  sense  position  as  well  as  energy.  They 
have a finite life, especially when detecting heavy particles, because of radiation damage. Silicon 
and germanium are quite different in their ability to convert gamma rays to electron showers. 
Semiconductor detectors for high energy particles are used in large numbers. Because of energy 
loss fluctuations, accurate measurement of the energy deposited is of less use. 
Temperature measurements 
A  diode  can  be  used  as  a  temperature  measuring  device,  since  the  forward  voltage  drop  across 
the  diode  depends  on  temperature,  as  in  a  Silicon  bandgap  temperature  sensor.  From  the 
Shockley  ideal  diode  equation  given  above,  it  appears  the  voltage  has  a  positive  temperature 
coefficient  (at  a  constant  current)  but  depends  on  doping  concentration  and  operating 
temperature (Sze 2007). The temperature coefficient can be negative as in typical thermistors or 
positive  for  temperature  sense  diodes  down  to  about  20  kelvins.  Typically,  silicon  diodes  have 
approximately 2 mV/C temperature coefficient at room temperature. 
Current steering 
Diodes  will  prevent  currents  in  unintended  directions.  To  supply  power  to  an  electrical  circuit 
during  a  power  failure,  the  circuit  can  draw  current  from  a  battery.  An  Uninterruptible  power 
supply  may  use  diodes  in  this  way  to  ensure  that  current  is  only  drawn  from  the  battery  when 
necessary.  Similarly,  small  boats  typically  have  two  circuits  each  with  their  own 
battery/batteries:  one  used  for  engine  starting;  one  used  for  domestics.  Normally  both  are 
charged from a single alternator, and a heavy duty split charge diode is used to prevent the higher 
charge battery (typically the engine battery) from discharging through the lower charged battery 
when the alternator is not running. 
Diodes are also used in electronic musical keyboards. To reduce the amount of wiring needed in 
electronic  musical  keyboards,  these  instruments  often  use  keyboard  matrix  circuits.  The 
keyboard controller scans the rows and columns to determine which note the player has pressed. 
The problem  with  matrix circuits  is that when  several notes are pressed at once, the current can 
flow backwards through the circuit and trigger "phantom keys" that cause ghost notes to play. 
To avoid triggering unwanted notes, most keyboard matrix circuits have diodes soldered with the 
switch  under  each  key  of  the  musical  keyboard.  The  same  principle  is  also  used  for  the  switch 
matrix in solid state pinball machines. 
 
 p-n Junction Diode  
Diode:  
A  pure  silicon  crystal  or  germanium  crystal  is  known  as  an  intrinsic  semiconductor.  There  are 
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not  enough  free  electrons  and  holes  in  an  intrinsic  semi-conductor to  produce  a  usable  current. 
The  electrical  action  of  these  can  be  modified  by  doping  means  adding  impurity  atoms  to  a 
crystal to increase either the number of free holes or no of free electrons.  
When a crystal has been doped, it is called a extrinsic semi-conductor. They are of two types  
  n-type semiconductor having free electrons as majority carriers 
  p-type semiconductor having free holes as majority carriers 
By themselves, these doped materials are of little use. However, if a junction is made by joining 
p-type  semiconductor  to  n-type  semiconductor  a  useful  device  is  produced  known  as  diode.  It 
will  allow  current  to  flow  through  it  only  in  one  direction.  The  unidirectional  properties  of  a 
diode allow current flow when  forward  biased  and disallow  current  flow when reversed  biased. 
This is called rectification process and therefore it is also called rectifier.  
How  is  it  possible  that  by  properly 
joining  two  semiconductors  each  of 
which,  by  itself,  will  freely  conduct 
the  current  in  any  direct  refuses  to 
allow conduction in one direction.  
Consider  first  the  condition  of  p-
type  and  n-type  germanium  just 
prior to  joining  fig.  1.  The  majority 
and minority carriers are in constant 
motion.  
The  minority  carriers  are  thermally 
produced  and  they  exist  only  for 
short  time  after  which  they 
recombine  and  neutralize  each 
other.  In  the  mean  time,  other 
minority  carriers  have  been 
produced  and  this  process  goes  on 
and on.  
The  number  of  these  electron  hole 
pair  that  exist  at  any  one  time 
depends  upon  the  temperature.  The 
number  of  majority  carriers  is 
however,  fixed  depending  on  the 
number of impurity atoms available. 
While the electrons and holes are  in 
motion  but  the  atoms  are  fixed  in 
place and do not move.  
 
Fig.1  
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As soon as, the junction is formed, the following processes are initiated fig. 2. 
 
Fig.2  
-  Holes  from  the  p-side  diffuse  into  n-side  where 
they recombine with free electrons.  
-  Free  electrons  from  n-side  diffuse  into  p-side 
where they recombine with free holes.  
-  The  diffusion  of  electrons  and holes is  due  to the 
fact that large  no of electrons are concentrated in 
one area and large no of holes are concentrated in 
 another area.  
-  When  these  electrons  and  holes  begin  to  diffuse 
across the  junction  then  they  collide  each  other 
and  negative  charge   in the electrons  cancels  the 
positive charge of the hole and both will lose their 
charges.  
-  The diffusion of holes and electrons is an electric 
current  referred  to  as  a  recombination  current. 
The  recombination process  decay  exponentially 
with  both  time  and distance  from  the  junction. 
Thus  most  of  the  recombination  occurs  just  after 
the junction is made and very near to junction.  
-  A  measure  of  the  rate  of  recombination  is 
the lifetime defined  as  the  time  required  for  the 
density  of  carriers  to  decrease  to  37%  to  the 
original concentration 
The  impurity atoms are  fixed  in their  individual places. The atoms  itself  is a part of the crystal 
and so cannot move. When the electrons and hole meet, their individual charge is cancelled and 
this leaves the originating impurity atoms with a net charge, the atom that produced the electron 
now lack an electronic and so becomes charged positively, whereas the atoms that produced the 
hole now lacks a positive charge and becomes negative.  
The  electrically  charged  atoms  are  called  ions  since  they  are  no  longer  neutral.  These  ions 
produce  an  electric  field  as  shown  in  fig.  3.  After  several  collisions  occur,  the  electric  field  is 
great enough to repel rest of the majority carriers away of the junction. For example, an electron 
trying to diffuse from n to p side is repelled by the negative charge of the p-side. Thus diffusion 
process does not continue indefinitely but continues as long as the field is developed.  
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Fig.3  
This region is produced immediately surrounding the junction that has no majority carriers. The 
majority  carriers  have  been  repelled  away  from  the  junction  and  junction  is  depleted  from 
carriers.  The  junction  is  known  as  the  barrier  region  or  depletion  region.  The  electric  field 
represents a potential difference across the junction also called space charge potential or barrier 
potential . This potential is 0.7v for Si at 25
o
 celcious and 0.3v for Ge.  
The physical width of the depletion region depends on  the doping level. If very heavy doping is 
used, the depletion region  is physically thin  because diffusion charge  need  not travel  far across 
the junction  before recombination takes place (short life time). If doping  is  light, then depletion 
is more wide (long life time). 
 
p-n Junction Diode  
The symbol of diode is shown in fig. 4. The terminal connected to p-layer is called anode (A) and the terminal connected to 
n-layer is called cathode (K) 
 
 
 
 
Fig.4 
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Reverse Bias:  
If positive terminal of dc source is connected to cathode and negative terminal is connected to anode, the diode is called reverse 
biased as shown in fig. 5.  
 
Fig.5 
When the diode  is reverse  biased then the depletion region width  increases,  majority carriers  move away  from the  junction and 
there is no flow of current due to majority carriers but there are thermally produced electron hole pair also. If these elect rons and 
holes are generated in the vicinity of junction then there is a flow of current. The negative voltage applied to the diode will tend to 
attract the holes thus generated and repel the electrons. At the same time, the positive voltage will attract the electrons towards the 
battery and repel the holes. This will cause current to flow in the circuit. This current is usually very small (interms of micro amp 
to nano amp). Since this current is due to minority carriers and these number of minority carriers are fixed at a given temperature 
therefore, the current is almost constant known as reverse saturation current I
CO
.  
In actual diode, the current is not almost constant but increases slightly with voltage. This is due to surface leakage current. The 
surface of diode follows ohmic law (V=IR). The resistance under reverse bias condition is very high 100k to mega ohms. When 
the reverse voltage is increased, then at certain voltage, then breakdown to diode takes place and it conducts heavily. This  is due 
to avalanche or zener breakdown. The characteristic of the diode is shown in fig. 6.  
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Fig.6 
Forward bias:  
When the diode  is  forward bias, then  majority carriers are pushed towards  junction, when they collide  and recombination takes 
place.  Number  of  majority  carriers  are  fixed  in  semiconductor.  Therefore  as  each  electron  is  eliminated  at  the  junction,  a  new 
electron  must be  introduced, this comes  from  battery.  At the same time, one  hole  must be created  in p-layer. This  is  formed  by 
extracting one electron from p-layer. Therefore, there is a flow of carriers and thus flow of current.  
 
Diode 
Space charge capacitance C
T
 of diode:  
Reverse  bias  causes  majority  carriers  to  move  away  from  the  junction,  thereby  creating  more 
ions.  Hence  the  thickness  of  depletion  region  increases.  This  region  behaves  as  the  dielectric 
material used for making capacitors. The p-type and n-type conducting on each side of dielectric 
act as the plate. The incremental capacitance C
T
 is defined by  
 
Since         
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Therefore,                (E-1) 
where,  dQ  is  the  increase  in  charge  caused  by  a  change  dV  in  voltage.  C
T
  is  not  constant,  it 
depends upon applied voltage, there fore it is defined as dQ / dV.  
When  p-n  junction  is  forward  biased,  then  also  a  capacitance  is  defined  called  diffusion 
capacitance  C
D
  (rate  of  change  of  injected  charge  with  voltage)  to  take  into  account  the  time 
delay  in  moving  the  charges  across  the  junction  by  the  diffusion  process.  It  is  considered  as  a 
fictitious element that allow us to predict time delay.  
If the amount of charge to be moved across the junction is increased, the time delay is greater, it 
follows that diffusion capacitance varies directly with the magnitude of forward current.  
      (E-2) 
Relationship between Diode Current and Diode Voltage  
An  exponential  relationship  exists  between  the  carrier  density  and  applied  potential  of  diode 
junction as given in equation E-3. This exponential relationship of the current i
D
 and the voltage 
v
D
 holds over a range of at least seven orders of magnitudes of current - that is a factor of 10
7
.  
          (E-3) 
Where,  
i
D
=  Current  through  the  diode  (dependent  variable  in  this  expression) 
v
D
=  Potential  difference  across  the  diode  terminals  (independent  variable  in  this  expression) 
I
O
= Reverse saturation current (of the order of 10
-15
 A for small signal diodes, but I
O
 is a strong 
function  of  temperature) 
q  =  Electron  charge:  1.60  x  10
-19
  joules/volt 
k  =  Boltzmann's  constant:  1.38  x  l0
-23
  joules  /  K 
T  =  Absolute  temperature  in  degrees  Kelvin  (K  =  273  +  temperature  in  C) 
n  =  Empirical  scaling  constant  between  0.5  and  2,  sometimes  referred  to  as  the  Exponential 
Ideality Factor  
The empirical constant, n, is a number that can vary according to the voltage and current levels. 
It depends on electron drift, diffusion, and carrier recombination in the depletion region. Among 
the quantities affecting the  value of  n are the diode  manufacture, levels of doping and purity of 
materials. If n=1, the value of k T/ q is 26 mV at 25C. When n=2, k T/ q becomes 52 mV.  
For  germanium  diodes,  n  is  usually  considered  to  be  close  to  1.  For  silicon  diodes,  n  is  in  the 
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range of 1.3 to 1.6. n is assumed 1 for all junctions all throughout unless otherwise noted.  
Equation (E-3) can be simplified by defining V
T
 =k T/q, yielding  
              (E-4) 
At  room  temperature  (25C)  with  forward-bias  voltage  only  the  first  term  in  the  parentheses  is 
dominant and the current is approximately given by  
           (E-5) 
The  current-voltage  (l-V)  characteristic  of  the  diode,  as  defined  by  (E-3)  is  illustrated  in  fig.  1. 
The  curve  in  the  figure  consists  of  two  exponential  curves.  However,  the  exponent  values  are 
such that for voltages and currents experienced in practical circuits, the curve sections are close 
to being straight lines. For voltages less than V
ON
, the curve is approximated by a straight line of 
slope close to zero. Since the slope is the conductance (i.e., i / v), the conductance is very small 
in  this  region,  and  the  equivalent  resistance  is  very  high.  For  voltages  above  V
ON
,  the  curve  is 
approximated by a straight line with a very large slope. The conductance is therefore very large, 
and the diode has a very small equivalent resistance.  
 
Fig.1 - Diode Voltage relationship 
The  slope  of  the  curves  of  fig.1  changes  as  the  current  and  voltage  change  since  the  l-V 
characteristic follows the exponential relationship of relationship of equation (E-4). Differentiate 
the equation (E-4) to find the slope at any arbitrary value of v
D
or i
D
,  
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           (E-6) 
This slope is the equivalent conductance of the diode at the specified values of v
D
 or i
D
.  
We  can  approximate  the  slope  as  a  linear  function  of  the  diode  current.  To  eliminate  the 
exponential  function,  we  substitute  equation  (E-4)  into  the  exponential  of  equation  (E-7)  to 
obtain 
        (E-7) 
A realistic assumption is that I
O
<< i
D
 equation (E-7) then yields,  
        (E-8) 
The  approximation  applies  if  the  diode  is  forward  biased.  The  dynamic  resistance  is  the 
reciprocal of this expression.  
        (E-9) 
Although r
d
 is a function of i
d
, we can approximate it as a constant if the variation of i
D
 is small. 
This  corresponds  to  approximating  the  exponential  function  as  a  straight  line  within  a  specific 
operating range.  
Normally,  the  term  R
f
  to  denote  diode  forward  resistance.  R
f
  is  composed  of  r
d
  and  the  contact 
resistance.  The  contact  resistance  is  a  relatively  small  resistance  composed  of  the  resistance  of 
the actual connection to the diode and the resistance of the semiconductor prior to the  junction. 
The reverse-bias resistance is extremely large and is often approximated as infinity.  
 
Diode 
Temperature Effects:  
Temperature plays an important role in determining the characteristic of diodes. As temperature 
increases, the turn-on voltage, v
ON
, decreases. Alternatively, a decrease in temperature results in 
an increase in v
ON
. This is illustrated in fig. 2, where V
ON
 varies linearly with temperature which 
is evidenced by the evenly spaced curves for increasing temperature in 25 C increments.  
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The temperature relationship is described by equation  
V
ON
(T
New
 )  V
ON
(T
room
) = k
T
(T
New
  T 
room
)            (E-10)  
 
Fig. 2 - Dependence of iD on temperature versus vD for real diode (kT = -2.0 mV /C)  
where,  
           T
room
= room temperature, or 25C. 
            T
New
= new temperature of diode in C. 
V
ON
(T
room
 ) = diode voltage at room temperature. 
 V
ON
 (T
New
) = diode voltage at new temperature. 
                k
T
 = temperature coefficient in V/C.  
Although k
T
 varies with changing operating parameters, standard engineering practice permits 
approximation as a constant. Values of k
T
 for the various types of diodes at room temperature are 
given as follows:  
k
T
= -2.5 mV/C for germanium diodes  
k
T
 = -2.0 mV/C for silicon diodes  
The reverse saturation current, I
O
 also depends on temperature. At room temperature, it increases 
approximately 16% per C for silicon and 10% per C for germanium diodes. In other words, I
O
 
approximately doubles for every 5 C increase in temperature for silicon, and for every 7 C for 
germanium. The expression for the reverse saturation current as a function of temperature can be 
approximated as  
     (E-11) 
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where K
i
= 0.15/C ( for silicon) and T1 and T2 are two arbitrary temperatures.  
 
Applications of Diode 
Applications of diode:  
Half wave Rectifier: 
The single  phase half wave rectifier is shown in fig. 8. 
 
 
Fig. 8   Fig. 9  
In positive half cycle, D is forward biased and conducts. Thus the output voltage is same as the 
input voltage. In the negative half cycle, D is reverse biased, and therefore output voltage is zero. 
The output voltage waveform is shown in fig. 9. 
The average output voltage of the rectifier is given by  
 
The average output current is given by  
 
When  the  diode  is  reverse  biased,  entire  transformer  voltage  appears  across  the  diode.  The 
maximum  voltage across the diode  is V
m
. The diode must be  capable to withstand this  voltage. 
Therefore PIV half wave rating of diode should be equal to V
m
 in case of single-phase rectifiers. 
The average current rating must be greater than I
avg
  
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Full Wave Rectifier:  
 A single  phase full wave rectifier using center tap transformer is shown in  fig. 10. It supplies 
current in both half cycles of the input voltage.  
 
 
Fig. 10   Fig. 11  
In the  first half  cycle D
1
  is  forward biased and conducts. But D
2
 is reverse  biased and does not 
conduct. In the second half cycle D
2
 is forward biased, and conducts and D
1
 is reverse biased. It 
is also called 2  pulse midpoint converter because it supplies current in both the half cycles. The 
output voltage waveform is shown in fig. 11. 
The average output voltage is given by  
 
and the average load current is given by  
 
When  D
1
  conducts,  then  full  secondary  voltage  appears  across  D
2
,  therefore  PIV  rating  of  the 
diode should be 2 V
m
.  
 
Bridge Rectifier:  
The  single    phase  full  wave  bridge  rectifier  is  shown  in  fig.  1.  It  is  the  most  widely  used 
rectifier. It also provides currents in both the half cycle of input supply.  
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Fig. 1   Fig. 2  
In  the  positive  half  cycle,  D
1
  &  D
4
  are  forward  biased  and  D
2
  &  D
3
  are  reverse  biased.  In  the 
negative  half  cycle,  D
2
  &  D
3
  are  forward  biased,  and  D
1
  &  D
4
  are  reverse  biased.  The  output 
voltage waveform is shown in fig. 2 and it is same as full wave rectifier but the advantage is that 
PIV rating of diodes are V m and only single secondary transformer is required.   
The  main  disadvantage  is  that  it  requires  four  diodes.  When  low  dc  voltage  is  required  then 
secondary voltage is low and diodes drop (1.4V) becomes significant. For low dc output, 2-pulse 
center tap rectifier is used because only one diode drop is there.  
The ripple factor is the measure of the purity of dc output of a rectifier and is defined as  
 
Therefore,  
 
  
Zener Diode:  
The diodes designed to work in  breakdown region are called zener diode. If the reverse voltage 
exceeds  the  breakdown  voltage,  the  zener  diode  will  normally  not  be  destroyed  as  long  as  the 
current does not exceed maximum value and the device closes not over load.  
When  a  thermally  generated  carrier  (part  of  the  reverse  saturation  current)  falls  down  the 
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junction  and  acquires  energy  of  the  applied  potential,  the  carrier  collides  with  crystal  ions  and 
imparts  sufficient  energy  to  disrupt  a  covalent  bond.  In  addition  to  the  original  carrier,  a  new 
electron-hole pair is generated. This pair may pick up sufficient energy from the applied field to 
collide with another crystal  ion and create still  another electron-hole pair. This action continues 
and  thereby  disrupts  the  covalent  bonds.  The  process  is  referred  to  as  impact  ionization, 
avalanche multiplication or avalanche breakdown.  
There  is  a  second  mechanism  that  disrupts  the  covalent  bonds.  The  use  of  a  sufficiently  strong 
electric  field  at  the  junction  can  cause  a  direct  rupture of  the  bond.  If  the  electric  field  exerts  a 
strong  force  on  a  bound  electron, the  electron  can  be  torn  from  the  covalent  bond  thus  causing 
the number of electron-hole pair combinations to multiply. This  mechanism  is  called  high  field 
emission or Zener breakdown. The value of reverse voltage at which this occurs is controlled by 
the amount ot doping of the diode. A  heavily doped diode has a  low  Zener  breakdown  voltage, 
while a lightly doped diode has a high Zener breakdown voltage.  
At voltages above  approximately  8V, the predominant  mechanism  is the avalanche  breakdown. 
Since  the  Zener  effect  (avalanche)  occurs  at  a  predictable  point,  the  diode  can  be  used  as  a 
voltage reference. The reverse voltage at which the avalanche occurs is called the breakdown or 
Zener voltage.  
A typical Zener diode characteristic is shown in  fig. 1. The circuit symbol for the Zener diode is 
different  from  that  of  a  regular  diode,  and  is  illustrated  in  the  figure.  The  maximum  reverse 
current, I
Z(max)
, which the Zener diode can withstand is dependent on the design and construction 
of the diode. A design guideline that the minimum Zener current, where the characteristic curve 
remains at V
Z
 (near the knee of the curve), is 0.1/ I
Z(max)
.  
 
Fig. 1 - Zener diode characteristic  
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The  power  handling  capacity  of  these  diodes  is  better.  The  power  dissipation  of  a  zener  diode 
equals the product of its voltage and current.  
P
Z
= V
Z
 I
Z
 
The  amount  of  power  which  the  zener  diode  can  withstand  (  V
Z
.I
Z(max) 
)  is  a  limiting  factor  in 
power supply design.  
Zener Regulator:    
When  zener  diode  is  forward  biased  it  works  as  a  diode  and  drop  across  it  is  0.7  V.  When  it 
works in breakdown region the voltage across it is constant (V
Z
) and the current through diode is 
decided  by  the  external  resistance.  Thus,  zener  diode  can  be  used  as  a  voltage  regulator  in  the 
configuration  shown  in  fig.  2  for  regulating  the  dc  voltage.  It  maintains  the  output  voltage 
constant even through the current through it changes.  
 
 
Fig. 2   Fig. 3  
The load line of the circuit is given by V
s
= I
s
 R
s
 + V
z
. The load line is plotted along with zener 
characteristic  in  fig.  3.  The  intersection  point of  the  load  line  and  the  zener  characteristic  gives 
the output voltage and zener current.  
To operate the zener in breakdown region V
s
 should always be greater then V
z
. R
s
 is used to limit 
the  current.  If  the  V
s
  voltage  changes,  operating  point  also  changes  simultaneously  but  voltage 
across zener is almost constant. The first approximation of zener diode is a voltage source of V
z
 
magnitude  and  second  approximation  includes  the  resistance  also.  The  two  approximate 
equivalent circuits are shown in fig. 4. 
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If second approximation of zener diode is considered, the output voltage varies slightly as shown 
in fig. 5. The zener ON state resistance produces more I * R drop as the current increases. As the 
voltage varies form V
1
 to V
2
 the operating point shifts from Q
1
 to Q
2
.  
The voltage at Q
1
 is  
V
1
 = I
1
 R
Z
 +V
Z
 
and at Q
2
  
V
2
 = I
2
 R
Z
 +V
Z
  
Thus, change in voltage is  
                 V
2
  V
1
 = ( I
2
  I
1
 ) R
Z
  
    V
Z
 = I
Z
 R
Z
  
 
Zener Diode  
Design of Zener regulator circuit:  
A  zenere  regulator  circuit  is  shown  in  fig.  6.  The  varying  load  current  is  represented  by  a 
variable load resistance R
L
.  
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The  zener  will  work  in  the  breakdown 
region  only  if  the  Thevenin  voltage  across 
zener is more than V
Z
 .  
 
 If  zener  is  operating  in  breakdown  region, 
the current through R
S
 is given by  
 
 
Fig. 6  
and load current     
I
s
= I
z
 + I
L
  
The  circuit  is  designed  such  that  the  diode  always  operates  in  the  breakdown  region  and  the 
voltage  V
Z
  across  it  remains  fairly  constant  even  though  the  current  I
Z
  through  it  vary 
considerably.  
If the  load I
L
 should  increase, the current I
Z
 should decrease by the same percentage in order to 
maintain  load  current  constant  I
s
.  This  keeps  the  voltage  drop  across  R
s
  constant  and  hence  the 
output voltage.  
If the input voltage should increase, the zener diode passes a larger current, that extra voltage is 
dropped  across  the  resistance  R
s
.  If  input  voltage  falls,  the  current  I
Z
  falls  such  that  V
Z
  is 
constant.  
In  the  practical  application  the  source  voltage,  v
s
,  varies  and  the  load  current  also  varies.  The 
design  challenge  is  to  choose  a  value  of  R
s
  which  permits  the  diode  to  maintain  a  relatively 
constant  output  voltage,  even  when  the  input  source  voltage  varies  and  the  load  current  also 
varies.  
We now analyze the circuit to determine the proper choice of R
s
. For the circuit shown in figure,  
    (E-1) 
           (E-2) 
The variable quantities in Equation (E-2) are v
Z
 and i
L
. In order to assure that the diode remains 
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in  the  constant  voltage  (breakdown)  region,  we  examine  the  two  extremes  of  input/output 
conditions, as follows:  
-  The  current  through  the  diode,  i
Z
,  is  a  minimum  (I
Z  min
)  when  the  load  current,  i
L
  is 
maximum (I
L max
) and the source voltage, v
s
 is minimum (V
s min
).  
-  The  current  through  the  diode,  i
Z
,  is  a  maximum  (I
Z  max
)  when  the  load  current,  i
L
,  is 
minmum (i
L min
) and the source voltage v
s
is minimum(V
s max
).  
When these characteristics of the two extremes are inserted into Equation (E-1), 
we find                     (E-3) 
  (E-4) 
In  a  practical  problem,  we  know  the  range  of  input  voltages, the  range  of  output  load  currents, 
and the desired Zener voltage. Equation (E-4) thus represents one equation in two unknowns, the 
maximum  and  minimum  Zener  current.  A  second  equation  is  found  from  the  characteristic  of 
zener. To avoid the  non-constant portion of the characteristic curve, we use an accepted rule of 
thumb that the minimum Zener current should be 0.1 times the maximum (i.e., 10%), that is,  
   (E-5) 
Solving the equations E-4 and E-5, we get,  
      (E-6) 
Now  that  we  can  solve  for  the  maximum  Zener  current,  the  value  of  R
s
,  is  calculated  from 
Equation (E-3).  
Zener diodes are manufactured with breakdown voltages V
Z
 in the range of a few volts to a few 
hundred  volts.  The  manufacturer  specifies  the  maximum  power  the  diode  can  dissipate.  For 
example, a 1W, 10 V zener can operate safely at currents up to 100mA.  
 
 
Special Purpose Diodes  
Light Emitting Diode :     
 In  a  forward  biased  diode  free  electrons  cross  the  junction  and  enter  into  p-layer  where  they 
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recombine  with  holes.  Each  recombination  radiates  energy  as  electron  falls  from  higher  energy 
level  to  a  lower  energy  level.  I  n  ordinary  diodes  this  energy  is  in  the  form  of  heat.  In  light 
emitting diode, this energy is in the form of light.  
The  symbol  of  LED  is  shown  in  fig.  2.  Ordinary  diodes  are  made  of  Ge  or  Si.  This  material 
blocks  the  passage  of  light.  LEDs  are  made  of  different  materials  such  as  gallium,  arsenic  and 
phosphorus. LEDs can radiate red, green, yellow, blue, orange or infrared (invisible). The LED's 
forward voltage drop is more approximately 1.5V. Typical LED current is between 10 mA to 50 
mA.  
  
 
 
Fig. 2   Fig. 3  
Seven Segment Display :  
Seven  segment  displays  are  used  to  display  digits  and  few  alphabets.  It  contains  seven 
rectangular LEDs. Each LED is called a Segment. External resistors are used to limit the currents 
to safe Values. It can display any letters a, b, c, d, e, f, g.as shown in fig. 3. 
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Fig. 4  
The  LEDs of seven-segment display are connected  in  either  in common anode configuration or 
in common cathode configuration as shown in fig. 4. 
Photo diode :  
When  a  diode  is  reversed  biased  as  shown  in  fig.  5,  a  reverse  current  flows  due  to  minority 
carriers.  These  carriers  exist  because  thermal  energy  keeps  on  producing  free  electrons  and 
holes. The lifetime of the minority carriers is short, but while they exist they can contribute to the 
reverse current. When light energy bombards a p-n junction, it too can produce free electrons.  
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Fig. 5  
In  other  words,  the  amount  of  light  striking  the  junction  can  control  the  reverse  current  in  a 
diode.  A  photo  diode  is  made  on  the  same  principle.  It  is  sensitive  to  the  light.  In  this  diode, 
through  a  window  light  falls  to  the  junction.  The  stronger  the  light,  the  greater  the  minority 
carriers and larger the reverse current.  
 
 
Voltage regulator 
A  voltage  regulator  is  an  electrical  regulator  designed  to  automatically  maintain  a  constant 
voltage level. 
It  may  use  an  electromechanical  mechanism,  or  passive  or  active  electronic  components. 
Depending on the design, it may be used to regulate one or more AC or DC voltages. 
With the exception of passive shunt regulators, all  modern electronic  voltage regulators operate 
by comparing the actual output voltage to some internal fixed reference voltage. Any difference 
is  amplified  and  used  to  control  the  regulation  element  in  such  a  way  as  to  reduce  the  voltage 
error.  This  forms  a  negative  feedback  control  loop;  increasing  the  open-loop  gain  tends  to 
increase regulation accuracy but reduce stability (avoidance of oscillation, or ringing during step 
changes).  There  will  also  be  a  trade-off  between  stability  and  the  speed  of  the  response  to 
changes. If the output voltage  is too low (perhaps due to input voltage reducing or  load current 
increasing),  the  regulation  element  is  commanded,  up  to  a  point,  to  produce  a  higher  output 
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voltage  -  by  dropping  less  of  the  input  voltage  (for  linear  series  regulators  and  buck  switching 
regulators), or to  draw  input  current  for  longer  periods  (boost-type  switching  regulators);  if  the 
output  voltage  is  too  high,  the  regulation  element  will  normally  be  commanded  to  produce  a 
lower voltage. However, many regulators have over-current protection, so that they will entirely 
stop  sourcing  current  (or  limit  the  current  in  some  way)  if  the  output  current  is  too  high,  and 
some regulators may also shut down if the input voltage is outside a given range. 
 Measures of regulator quality 
The  output  voltage  can  only  be  held  roughly  constant;  the  regulation  is  specified  by  two 
measurements: 
-  load  regulation  is  the  change  in  output  voltage  for  a  given  change  in  load  current  (for 
example:  "typically 15mV,  maximum 100mV  for load currents between 5mA and 1.4A, 
at some specified temperature and input voltage"). 
-  line  regulation or input regulation  is the degree to which output voltage changes with 
input  (supply)  voltage  changes  -  as  a  ratio  of  output  to  input  change  (for  example 
"typically 13mV/V"), or the output voltage change over the entire specified input voltage 
range  (for  example  "plus  or  minus  2%  for  input  voltages  between  90V  and  260V,  50-
60Hz"). 
Other important parameters are: 
-  Temperature  coefficient  of  the  output  voltage  is  the  change  in  output  voltage  with 
temperature (perhaps averaged over a given temperature range), while... 
-  Initial  accuracy  of  a  voltage  regulator  (or  simply  "the  voltage  accuracy")  reflects  the 
error  in  output  voltage  for  a  fixed  regulator  without  taking  into  account  temperature  or 
aging effects on output accuracy. 
-  Dropout voltage - the minimum difference between input voltage and output voltage for 
which  the  regulator  can  still  supply  the  specified  current.  A  Low  Drop-Out  (LDO) 
regulator is designed to work well even with an input supply only a  Volt or so above the 
output voltage. 
-  Absolute  Maximum  Ratings  are  defined  for  regulator  components,  specifying  the 
continuous and peak output currents that may be used (sometimes internally limited), the 
maximum input voltage, maximum power dissipation at a given temperature, etc. 
-  Output noise (thermal white noise) and output dynamic impedance may be specified as 
graphs versus frequency, while output ripple noise (mains "hum" or switch-mode "hash" 
noise) may be given as peak-to-peak or RMS voltages, or in terms of their spectra. 
-  Quiescent current  in  a regulator circuit  is the current drawn  internally,  not available to 
the load, normally measured as the input current while no load is connected (and hence a 
source of inefficiency; some linear regulators are, surprisingly, more efficient at very low 
current loads than switch-mode designs because of this). 
 
 
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Electromechanical regulators 
 
 
Circuit design for a simple electromechanical voltage regulator. 
 
 
Interior of an old electromechanical voltage regulator. 
 
 
Graph of voltage output on a time scale. 
In  older  electromechanical  regulators,  voltage  regulation  is  easily  accomplished  by  coiling  the 
sensing  wire  to  make  an  electromagnet.  The  magnetic  field  produced  by  the  current  attracts  a 
moving ferrous core held back under spring tension or gravitational pull. As voltage increases, so 
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does  the  current,  strengthening  the  magnetic  field  produced  by  the  coil  and  pulling  the  core 
towards  the  field.  The  magnet  is  physically  connected  to  a  mechanical  power  switch,  which 
opens  as  the  magnet  moves  into  the  field.  As  voltage  decreases,  so  does  the  current,  releasing 
spring  tension  or  the  weight  of  the  core  and  causing  it  to  retract.  This  closes  the  switch  and 
allows the power to flow once more. 
If  the  mechanical  regulator  design  is  sensitive  to  small  voltage  fluctuations,  the  motion  of  the 
solenoid core can be used to move a selector switch across a range of resistances or transformer 
windings to gradually step the output voltage up or down, or to rotate the position of a moving-
coil AC regulator. 
Early  automobile generators and alternators had a  mechanical  voltage regulator using one, two, 
or three  relays and  various  resistors to stabilize the generator's output at slightly  more than 6 or 
12  V,  independent  of  the  engine's  rpm  or  the  varying  load  on  the  vehicle's  electrical  system. 
Essentially, the relay(s) employed pulse width modulation to regulate the output of the generator, 
controlling the field current reaching the generator (or alternator) and in this way controlling the 
output voltage produced. 
The regulators used for generators (but not alternators) also disconnect the generator when it was 
not producing electricity, thereby preventing the battery from discharging back into the generator 
and  attempting  to  run  it  as  a  motor.  The  rectifier  diodes  in  an  alternator  automatically  perform 
this  function  so  that  a  specific  relay  is  not  required;  this  appreciably  simplified  the  regulator 
design. 
More modern designs  now use  solid state technology (transistors) to perform the same  function 
that the relays perform in electromechanical regulators. 
Electromechanical  regulators  are  used  for  mains  voltage  stabilisationsee  Voltage 
regulator#AC voltage stabilizers below. 
Coil-rotation AC voltage regulator 
 
 
Basic design principle and circuit diagram for the rotating-coil AC voltage regulator. 
This  is  an  older  type  of  regulator  used  in  the  1920s  that  uses  the  principle  of  a  fixed-position 
field coil and a second field coil that can be rotated on an axis in parallel with the fixed coil. 
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When the  movable coil  is positioned perpendicular to the  fixed  coil, the  magnetic  forces acting 
on the movable coil balance each other out and voltage output is unchanged. Rotating the coil in 
one direction or the other away from the center position will increase or decrease voltage in the 
secondary movable coil. 
This type of regulator can be automated via a servo control mechanism to advance the movable 
coil position in order to provide voltage increase or decrease. A braking mechanism or high ratio 
gearing  is used to hold the rotating coil  in place against the powerful  magnetic  forces acting on 
the moving coil. 
AC voltage stabilizers 
 
 
Magnetic mains regulator 
Electromechanical 
Electromechanical regulators, usually  called  voltage stabilizers,  have  also been used to regulate 
the voltage on AC power distribution lines. These regulators operate by using a servomechanism 
to select the appropriate tap on an autotransformer with multiple taps, or by moving the wiper on 
a  continuously  variable  autotransfomer.  If  the  output  voltage  is  not  in  the  acceptable  range,  the 
servomechanism  switches  connections  or  moves  the  wiper  to  adjust  the  voltage  into  the 
acceptable  region.  The  controls  provide  a  deadband  wherein  the  controller  will  not  act, 
preventing  the  controller  from  constantly  adjusting  the  voltage  ("hunting")  as  it  varies  by  an 
acceptably small amount. 
Constant-voltage transformer 
An  alternative  method  is  the  use  of  a  type  of  saturating  transformer  called  a  ferro  resonant 
transformer or constant-voltage transformer. These transformers use a tank circuit composed 
of a  high-voltage resonant winding  and a  capacitor to produce a nearly constant average output 
with  a  varying  input.  The  ferroresonant  approach  is  attractive  due  to  its  lack  of  active 
components,  relying  on  the  square  loop  saturation  characteristics  of  the  tank  circuit  to  absorb 
variations  in  average  input  voltage.  Older  designs  of  ferroresonant  transformers  had  an  output 
with high harmonic content, leading to a distorted output waveform. Modern devices are used to 
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construct  a  perfect  sinewave.  The  ferroresonant  action  is  a  flux  limiter  rather  than  a  voltage 
regulator,  but  with  a  fixed  supply  frequency  it  can  maintain  an  almost  constant  average  output 
voltage even as the input voltage varies widely. 
The ferroresonant transformers, which are also known as Constant Voltage Transformers (CVTs) 
or  ferros,  are  also  good  surge  suppressors,  as  they  provide  high  isolation  and  inherent  short-
circuit protection. 
A  ferroresonant  transformer  can  operate  with  an  input  voltage  range  40%  or  more  of  the 
nominal voltage. 
Output power factor remains in the range of 0.96 or higher from half to full load. 
Because it regenerates an output voltage waveform, output distortion, which is typically less than 
4%, is independent of any input voltage distortion, including notching. 
Efficiency at full load is typically in the range of 89% to 93%. However, at low loads, efficiency 
can drop below 60% and  no  load  losses can  be  as  high as 20%. The current-limiting capability 
also  becomes  a  handicap  when  a  CVT  is  used  in  an  application  with  moderate  to  high  inrush 
current  like  motors,  transformers  or  magnets.  In  this  case,  the  CVT  has  to  be  sized  to 
accommodate the peak current, thus forcing it to run at low loads and poor efficiency.  
Minimum maintenance is required. Transformers and capacitors can be very reliable. Some units 
have  included  redundant  capacitors  to  allow  several  capacitors  to  fail  between  inspections 
without any noticeable effect on the device's performance. 
Output voltage varies about 1.2% for every 1% change in supply frequency. For example, a 2-Hz 
change  in  generator  frequency,  which  is  very  large,  results  in  an  output  voltage  change  of  only 
4%, which has little effect for most loads. 
It  accepts  100%  single-phase  switch-mode  power  supply  loading  without  any  requirement  for 
derating, including all neutral components. 
Input  current  distortion  remains  less  than  8%  THD  even  when  supplying  nonlinear  loads  with 
more than 100% current THD. 
Drawbacks  of  CVTs  (constant  voltage  transformers)  are  their  larger  size,  audible  humming 
sound, and high heat generation. 
 
 
 
 
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DC voltage stabilizers 
 
 
KPEH8A stabilizers 
Many  simple  DC  power  supplies  regulate  the  voltage  using  a  shunt  regulator  such  as  a  zener 
diode,  avalanche  breakdown  diode,  or  voltage  regulator  tube.  Each  of  these  devices  begins 
conducting  at  a  specified  voltage  and  will  conduct  as  much  current  as  required  to  hold  its 
terminal  voltage  to  that  specified  voltage.  The  power  supply  is  designed  to  only  supply  a 
maximum  amount of  current that  is  within  the  safe  operating  capability  of  the  shunt  regulating 
device  (commonly,  by  using  a  series  resistor). In  shunt  regulators, the  voltage  reference  is  also 
the regulating device. 
If the stabilizer must provide more power, the shunt regulator output is only used to provide the 
standard voltage reference for the electronic device, known as the voltage stabilizer. The voltage 
stabilizer is the electronic device, able to deliver much larger currents on demand. 
Active regulators 
Active  regulators  employ  at  least  one  active  (amplifying)  component  such  as  a  transistor  or 
operational amplifier. Shunt regulators are often (but not always) passive and simple, but always 
inefficient  because  they  (essentially)  dump  the  excess  current  not  needed  by  the  load.  When 
more  power  must  be  supplied,  more  sophisticated  circuits  are  used.  In  general,  these  active 
regulators can be divided into several classes: 
-  Linear series regulators 
-  Switching regulators 
-  SCR regulators 
Linear regulators 
Linear regulators are based on devices that operate in their linear region (in contrast, a switching 
regulator is based on a device forced to act as an on/off switch). In the past, one or more vacuum 
tubes  were  commonly  used  as  the  variable  resistance.  Modern  designs  use  one  or  more 
transistors  instead,  perhaps  within  an  Integrated  Circuit.  Linear  designs  have  the  advantage  of 
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very  "clean"  output  with  little  noise  introduced  into  their  DC  output,  but  are  most  often  much 
less efficient and unable to step-up or invert the  input voltage  like  switched supplies. All  linear 
regulators require a higher input than the output. All linear regulators are subject to the parameter 
of dropout voltage. 
Entire  linear  regulators  are  available  as  integrated  circuits.  These  chips  come  in  either  fixed  or 
adjustable voltage types. 
Switching regulators 
Switching regulators rapidly switch a series device on and off. The  duty cycle of the switch sets 
how much  charge is transferred to the load. This is controlled by a similar feedback mechanism 
as in a linear regulator. Because the series element is either fully conducting, or switched off, it 
dissipates  almost  no  power;  this  is  what  gives  the  switching  design  its  efficiency.  Switching 
regulators  are  also  able  to  generate  output  voltages  which  are  higher  than  the  input,  or  of 
opposite polarity  something not possible with a linear design. 
Like  linear  regulators,  nearly-complete  switching  regulators  are  also  available  as  integrated 
circuits. Unlike linear regulators, these usually require one external component: an  inductor that 
acts as the energy storage element. (Large-valued inductors tend to be physically large relative to 
almost all other kinds of componentry, so they are rarely fabricated within integrated circuits and 
IC regulators  with some exceptions.
[1]
) 
Comparing linear vs. switching regulators 
The two types of regulators have their different advantages: 
-  Linear regulators are best when low output noise (and low RFI radiated noise) is required 
-  Linear  regulators  are  best  when  a  fast  response  to  input  and  output  disturbances  is 
required. 
-  At  low  levels  of  power,  linear  regulators  are  cheaper  and  occupy  less  printed  circuit 
board space. 
-  Switching  regulators  are  best  when  power  efficiency  is  critical  (such  as  in  portable 
computers), except  linear regulators are  more efficient  in a  small  number of cases (such 
as a 5V microprocessor often in "sleep" mode fed from a 6V battery, if the complexity of 
the  switching  circuit  and  the  junction  capacitance  charging  current  means  a  high 
quiescent current in the switching regulator). 
-  Switching  regulators  are  required  when  the  only  power  supply  is  a  DC  voltage,  and  a 
higher output voltage is required. 
-  At  high  levels  of  power  (above  a  few  watts),  switching  regulators  are  cheaper  (for 
example, the cost of removing heat generated is less). 
SCR regulators 
Regulators  powered  from  AC  power  circuits  can  use  silicon  controlled  rectifiers  (SCRs)  as  the 
series  device.  Whenever  the  output  voltage  is  below  the  desired  value,  the  SCR  is  triggered, 
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allowing electricity to flow into the load until the AC mains voltage passes through zero (ending 
the half cycle). SCR regulators have the advantages of being both very efficient and very simple, 
but because they can not terminate an on-going half cycle of conduction, they are not capable of 
very accurate voltage regulation in response to rapidly-changing loads. 
Combination (hybrid) regulators 
Many  power  supplies  use  more  than  one  regulating  method  in  series.  For  example,  the  output 
from a switching regulator can be further regulated by a linear regulator. The switching regulator 
accepts  a  wide  range  of  input  voltages  and  efficiently  generates  a  (somewhat  noisy)  voltage 
slightly above the ultimately desired output. That is followed by a linear regulator that generates 
exactly  the  desired  voltage  and  eliminates  nearly  all  the  noise  generated  by  the  switching 
regulator.  Other  designs  may  use  an  SCR  regulator  as  the  "pre-regulator",  followed  by  another 
type of regulator. An efficient way of creating a variable-voltage, accurate output power supply 
is to combine a multi-tapped transformer with an adjustable linear post-regulator. 
Voltage stabilizer 
A  voltage  stabilizer  is  an  electronic  device  able  to  deliver  relatively  constant  output  voltage 
while input voltage and load current changes over time. 
The  voltage stabilizer  is the shunt  regulator such  as a  Zener diode or avalanche diode. Each of 
these  devices  begins  conducting  at  a  specified  voltage  and  will  conduct  as  much  current  as 
required to hold  its terminal  voltage to that specified voltage. Hence the  shunt regulator can  be 
viewed  as  the  limited  power  parallel  stabilizer.  The  shunt  regulator output  is  used  as  a  voltage 
reference. 
The  Zener  diode  and  avalanche  diode  have  opposite  threshold  voltage  dependence  on 
temperature.  By  connecting  these  two  devices  sequentially,  it  is  possible  to  construct  a  voltage 
reference  with  improved  thermal  stability.  Sometimes  (mostly  for  the  voltages  around  5.6  V) 
both effects are combined in the same diode. 
Simple voltage stabilizer 
In  the  simplest  case  emitter  follower  is  used,  the  base  of  the  regulating  transistor  is  directly 
connected to the voltage reference: 
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The stabilizer uses the power source, having voltage U
in
 that may vary over time. It delivers the 
relatively constant voltage U
out
. The output load R
L
 can also vary over time. For such a device to 
work  properly,  the  input  voltage  must  be  larger  than  the  output  voltage  and  Voltage  drop  must 
not exceed the limits of the transistor used. 
The output voltage of the stabilizer is equal to U
Z
 - U
BE
 where U
BE
 is about 0.7v and depends on 
the load current. If the output voltage drops below that limit, this increases the voltage difference 
between  the  base  and  emitter  (U
be
),  opening  the  transistor  and  delivering  more  current. 
Delivering more current through the same output resistor R
L
 increases the voltage again. 
Voltage stabilizer with an operational amplifier 
The  stability  of  the  output  voltage  can  be  significantly  increased  by  using  the  operational 
amplifier: 
 
In  this  case,  the  operational  amplifier  opens  the  transistor  more  if  the  voltage  at  its  inverting 
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input  drops  significantly  below  the  output  of  the  voltage  reference  at  the  non-inverting  input. 
Using the voltage divider (R1, R2 and R3) allows choice of the arbitrary output voltage between 
U
z
 and U
in
. 
Zener diode 
                                         
 
Current-voltage characteristic of a Zener diode with a breakdown voltage of 17 volt. Notice the 
change  of  voltage  scale  between  the  forward  biased  (positive)  direction  and  the  reverse  biased 
(negative) direction. 
A  Zener  diode  is  a  type  of  diode  that  permits  current  not  only  in  the  forward  direction  like  a 
normal diode, but also in the reverse direction if the voltage is larger than the  breakdown voltage 
known as "Zener knee voltage" or "Zener voltage". The device was named after Clarence Zener, 
who discovered this electrical property. 
A conventional solid-state diode will not allow significant current if it is reverse-biased below its 
reverse  breakdown  voltage.  When  the  reverse  bias  breakdown  voltage  is  exceeded,  a 
conventional diode is subject to high current due to avalanche breakdown. Unless this current is 
limited  by  circuitry,  the  diode  will  be  permanently  damaged.  In  case  of  large  forward  bias 
(current in the direction of the arrow), the diode exhibits a voltage drop due to its junction built-
in voltage and internal resistance. The amount of the voltage drop depends on the semiconductor 
material and the doping concentrations. 
A Zener diode exhibits almost the same properties, except the device is specially designed so as 
to  have  a  greatly  reduced  breakdown  voltage, the  so-called  Zener  voltage.  By  contrast  with  the 
conventional device, a reverse-biased Zener diode will exhibit a controlled breakdown and allow 
the current to keep the voltage across the Zener diode at the Zener voltage. For example, a diode 
with  a  Zener  breakdown  voltage  of  3.2  V  will  exhibit  a  voltage  drop  of  3.2  V  if  reverse  bias 
voltage  applied  across  it  is  more  than  its  Zener  voltage.  The  Zener  diode  is  therefore  ideal  for 
applications  such  as  the  generation  of  a  reference  voltage  (e.g.  for  an  amplifier  stage),  or  as  a 
voltage stabilizer for low-current applications. 
The Zener diode's operation depends on the heavy  doping of  its p-n  junction allowing electrons 
to  tunnel  from  the  valence  band  of  the  p-type  material  to  the  conduction  band  of  the  n-type 
material.  In  the  atomic  scale,  this  tunneling  corresponds  to  the  transport  of  valence  band 
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electrons into the empty conduction band states; as a result of the reduced barrier between these 
bands and high electric fields that are induced due to the relatively high levels of dopings on both 
sides.
[1]
 The breakdown  voltage can  be controlled quite accurately  in the doping process. While 
tolerances  within  0.05%  are  available,  the  most  widely  used  tolerances  are  5%  and  10%. 
Breakdown voltage for commonly available zener diodes can vary widely  from 1.2 volts to 200 
volts. 
Another  mechanism  that  produces  a  similar  effect  is  the  avalanche  effect  as  in  the  avalanche 
diode. The two types of diode are in fact constructed the same way and both effects are present 
in diodes of this type. In silicon diodes up to about 5.6 volts, the Zener effect is the predominant 
effect  and  shows  a  marked  negative  temperature  coefficient.  Above  5.6  volts,  the  avalanche 
effect becomes predominant and  exhibits a positive temperature coefficient
[1]
. In a 5.6 V diode, 
the  two  effects  occur  together  and  their  temperature  coefficients  neatly  cancel  each  other  out, 
thus  the  5.6  V  diode  is  the  component  of  choice  in  temperature-critical  applications.  Modern 
manufacturing techniques have produced devices with voltages lower than 5.6 V with negligible 
temperature  coefficients,  but  as  higher  voltage  devices  are  encountered,  the  temperature 
coefficient rises dramatically. A 75 V diode has 10 times the coefficient of a 12 V diode. 
All such diodes, regardless of breakdown voltage, are usually marketed under the umbrella term 
of "Zener diode". 
-   
Uses 
 
 
Zener diode shown with typical packages. Reverse current  i
Z
 is shown. 
Zener diodes are widely used as voltage references and as shunt regulators to regulate the voltage 
across  small  circuits.  When  connected  in  parallel  with  a  variable  voltage  source  so  that  it  is 
reverse  biased, a Zener diode conducts when the voltage reaches the diode's reverse breakdown 
voltage. From that point on, the relatively  low  impedance of the diode keeps the  voltage across 
the diode at that value. 
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In this circuit, a typical voltage reference or regulator, an input voltage, U
IN
, is regulated down to 
a stable output voltage U
OUT
. The intrinsic voltage drop of diode D is stable over a wide current 
range  and  holds  U
OUT
  relatively  constant  even  though  the  input  voltage  may  fluctuate  over  a 
fairly wide range. Because of the low impedance of the diode when operated like this, Resistor R 
is used to limit current through the circuit. 
In the case of this simple reference, the  current  flowing  in the diode  is determined using  Ohms 
law and the known voltage drop across the resistor R. I
Diode
 = (U
IN
 - U
OUT
) / R
 
The value of R must satisfy two conditions: 
1.  R  must  be  small  enough  that  the  current  through  D  keeps  D  in  reverse  breakdown.  The 
value  of  this  current  is  given  in  the  data  sheet  for  D.  For  example,  the  common 
BZX79C5V6
[2]
 device, a 5.6 V 0.5 W Zener diode, has a recommended reverse current of 
5  mA.  If  insufficient  current  exists  through  D,  then  U
OUT
  will  be  unregulated,  and  less 
than  the  nominal  breakdown  voltage  (this  differs  to  voltage  regulator  tubes  where  the 
output  voltage  will  be  higher  than  nominal  and  could  rise  as  high  as  U
IN
).  When 
calculating  R,  allowance  must  be  made  for  any  current  through  the  external  load,  not 
shown in this diagram, connected across U
OUT
. 
2.  R  must  be  large  enough  that  the  current  through  D  does  not  destroy  the  device.  If  the 
current  through  D  is  I
D
,  its  breakdown  voltage  V
B
  and  its  maximum  power  dissipation 
P
MAX
, then I
D
V
B
 < P
MAX
. 
A load may be placed across the diode in this reference circuit, and as long as the zener stays in 
reverse breakdown, the diode will provide a stable voltage source to the load. 
A  Zener  diode  used  in  this  way  is  known  as  a  shunt  voltage  regulator  (shunt,  in  this  context, 
meaning  connected  in  parallel,  and  voltage  regulator  being  a  class  of  circuit  that  produces  a 
stable voltage across any load). In a sense, a portion of the current through the resistor is shunted 
through the Zener diode, and the rest  is through the  load. Thus the  voltage that the  load sees  is 
controlled by causing some fraction of the current from the power source to bypass ithence the 
name, by analogy with locomotive switching points. 
Shunt  regulators  are  simple,  but  the  requirements  that  the  ballast  resistor  be  small  enough  to 
avoid  excessive  voltage  drop  during  worst-case  operation  (low  input  voltage  concurrent  with 
high load current) tends to leave a lot of current flowing in the diode much of the time, making 
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for  a  fairly  wasteful  regulator  with  high  quiescent  power  dissipation,  only  suitable  for  smaller 
loads. 
Zener diodes in this configuration are often used as stable references for more advanced voltage 
regulator circuits. 
These devices are also encountered, typically in series with a base-emitter junction, in transistor 
stages where selective choice of a device centered around the avalanche/Zener point can be used 
to  introduce  compensating  temperature  co-efficient  balancing  of  the  transistor  PN  junction.  An 
example  of  this  kind  of  use  would  be  a  DC  error  amplifier  used  in  a  stabilized  power  supply 
circuit feedback loop system. 
Zener diodes are also used in surge protectors to limit transient voltage spikes. 
Another  notable  application  of  the  zener  diode  is  the  use  of  noise  caused  by  its  avalanche 
breakdown in a random number generator that never repeats. 
Voltage Regulators:  
An  ideal  power  supply  maintains  a  constant  voltage  at  its  output  terminals  under  all  operating 
conditions. The output voltage of a practical power supply changes with load generally dropping 
as load current increases as shown in fig. 1.  
 
Fig. 1  
The  terminal  voltage  when  full  load  current  is  drawn  is  called  full  load  voltage  (V
FL
).  The  no 
load voltage is the terminal voltage when zero current is drawn from the supply, that is, the open 
circuit terminal voltage.  
Power supply performance is measured in terms of percent voltage regulation, which indicates its 
ability to maintain a constant voltage. It is defined as  
 
The Thevenin's equivalent of a power supply is shown in  fig. 2. The Thevenin voltage is the no-
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load voltage V
NL
 and the Thevenin resistance is called the output resistance R
o
. Let the full load 
current be I
FL
. Therefore, the full load resistance R
FL
 is given by  
 
 
Fig. 2  
From the equivalent circuit, we have  
 
and the voltage regulation is given by 
 
It is clear that the ideal power supply has zero outut resistance. 
Example-1  
A  power  supply  having  output  resistance  1.5  supplies  a  full  load  current  of  500mA  to  a  50 
load. Determine:  
1.  percent voltage regulation of the supply  
2.  no load output voltage.  
Solution:  
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(a). Full load output voltage V
FL
 = (500mA ) (50) = 25V.  
Therefore,     
(b). The no load voltage   
Voltage Regulators:  
An unregulated power supply consists of a transformer (step down), a rectifier and a filter. These 
power  supplies  are  not  good  for  some  applications  where  constant  voltage  is  required 
irrespective of external disturbances. The main disturbances are:  
1.  As the load current varies, the output voltage also varies because of its poor regulation.  
2.  The  dc  output  voltage  varies  directly  with  ac  input  supply.  The  input  voltage  may  vary 
over a wide range thus dc voltage also changes.  
3.  The dc output voltage varies with the temperature if semiconductor devices are used.  
An  electronic  voltage  regulator  is  essentially  a  controller  used  along  with  unregulated  power 
supply to stabilize the output dc voltage against three major disturbances  
a.  Load current (I
L
)  
b.  Supply voltage (V
i
)  
c.  Temperature (T) 
Fig. 3, shows the basic block diagram of voltage regulator. where 
V
i
 = unregulated dc voltage.  
V
o
 = regulated dc voltage.  
 
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Fig. 3  
Since the output dc voltage V
Lo
 depends on the  input unregulated dc voltage V
i
,  load current I
L
 
and the temperature t, then the change V
o
 in output voltage of a power supply can be expressed 
as follows  
V
O
 = V
O
(V
i
, I
L
, T) 
Take partial derivative of V
O
, we get, 
 
S
V
  gives  variation  in  output  voltage  only  due  to  unregulated  dc  voltage.  R
O
  gives  the  output 
voltage  variation  only  due  to  load  current.  S
T
  gives  the  variation  in  output  voltage  only  due  to 
temperature.  
The  smaller  the  value  of  the  three  coefficients,  the  better the  regulations  of  power  supply.  The 
input  voltage  variation  is  either  due  to  input  supply  fluctuations  or  presence  of  ripples  due  to 
inadequate filtering.  
Voltage Regulator:    
A  voltage  regulator  is  a  device  designed  to  maintain  the  output  voltage  of  power  supply  nearly 
constant.  It can be regarded as a closed  loop system  because  it  monitors the output voltage and 
generates  the  control  signal  to  increase  or  decrease  the  supply  voltage  as  necessary  to 
compensate  for  any  change  in  the  output  voltage.  Thus  the  purpose  of  voltage  regulator  is  to 
eliminate  any  output  voltage  variation  that  might occur  because  of  changes  in  load,  changes  in 
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supply voltage or changes in temperature.  
Zener Voltage Regulator:  
The regulated power supply  may  use zener diode as the  voltage controlling device  as shown  in 
fig.  4.  The  output  voltage  is  determined  by  the  reverse  breakdown  voltage  of  the  zener  diode. 
This is nearly constant for a wide range of currents. The load voltage can be maintained constant 
by controlling the current through zener. 
 
Fig. 4  
The zener diode regulator has limitations of range. The load current range for which regulation is 
maintained,  is  the  difference  between  maximum  allowable  zener  current  and  minimum  current 
required  for  the  zener  to  operate  in  breakdown  region.  For  example,  if  zener  diode  requires  a 
minimum  current  of  10  mA  and  is  limited  to  a  maximum  of  1A  (to  prevent  excessive 
dissipation), the range is 1 - 0.01 = 0.99A. If the load current variation exceeds 0.99A, regulation 
may be lost. 
Emitter Follower Regulator:  
To  obtain  better  voltage  regulation  in  shunt  regulator,  the  zener  diode  can  be  connected  to  the 
base circuit of a power transistor as shown in fig. 5. This amplifies the zener current range. It is 
also known as emitter follower regulation. 
 
Fig. 5  
This  configuration  reduces  the  current  flow  in  the  diode.  The  power  transistor  used  in  this 
configuration  is  known  as  pass  transistor.  The  purpose  of  C
L
  is  to  ensure  that  the  variations  in 
one  of  the  regulated  power  supply  loads  will  not  be  fed  to  other  loads.  That  is,  the  capacitor 
effectively shorts out high-frequency variations.  
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Because  of  the  current  amplifying  property  of  the  transistor,  the  current  in  the  zenor  dioide  is 
small. Hence there  is  little  voltage drop across the diode resistance, and the zener approximates 
an ideal constant voltage source. 
Operation of the circuit:  
The current through resistor R is the sum of zener current I
Z
 and the transistor base current I
B
 ( = 
I
L
 /  ).  
I
L
 = I
Z
 + I
B
  
The output voltage across R
L
 resistance is given by  
V
O
 = V
Z
  V
BE
  
Where V
BE
  0.7 V 
Therefore, V
O
= constant.  
The emitter current is same as load current. The current I
R
 is assumed to be constant for a given 
supply voltage. Therefore, if I
L
 increases, it needs more base currents, to increase base current I
z
 
decreases.  The  difference  in  this  regulator  with  zener  regulator  is  that  in  later  case  the  zener 
current  decreases  (increase)  by  same  amount  by  which  the  load  current  increases  (decreases). 
Thus the current range is less, while in the shunt regulators, if I
L
 increases by I
L
 then I
B
 should 
increase by I
L
 /  or I
Z
 should decrease by I
L
 / . Therefore the current range control is more 
for the same rating zener.  
The simplified circuit of the shunt regulator is shown in fig. 6. 
 
Fig. 6  
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In  a  power  supply  the  power  regulation  is  basically,  because  of  its  high  internal  impedance.  In 
the circuit discussed, the unregulated supply has resistance R
S
 of the order of 100 ohm. The use 
of emitter follower is to reduce the output resistance and it becomes approximately.   
R
O
 = ( R
z
 + h
ie
 ) / (1 + h
fe
)  
Where  R
Z
  represents  the  dynamic  zener  resistance.  The  voltage  stabilization  ratio  S
V
  is 
approximately  
S
V
 =  V
o
 /  V
I
 = R
z
 / (R
z
 + R)  
S
V
 can  be  improved  by  increasing  R. This  increases V
CE
 and power dissipated  in the transistor. 
Other disadvantages of the circuit are.  
1.  No provision for varying the output voltage since it is almost equal to the zener voltage.  
2.  Change  in  V
BE
and  V
z
  due  to  temperature  variations  appear  at  the  output  since  the 
transistor  is  connected  in  series  with  load,  it  is  called  series  regulator  and  transistor  is 
allow series pass transistor.  
Design of Series Voltage Regulator:  
Fig.  1  shows  the  basic  circuit  of  a  series  voltage  regulator.  The  operation  of  this  regulator  has 
been  discussed  in  previous  lecture.  It  consists  of  series  (pass)  transistor  to  control  the  output 
voltage.  
 
Fig. 1  
The circuit can be designed taking two extreme operating conditions, 
1.  V
S max
, I
Z max
, I
 load min
 /   
2.  V
S min
, I
Z min
, I
 load max
 /   
We calculate R 
s
 for both conditions and since R 
si
 is constant, we equate these two expressions 
as in Equation E-1. 
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        (E-1) 
A design guideline that set I
Z min
 = 0.1 I 
Z max
. Then we equate the expressions for Equation (E-1) 
to obtain, 
      (E-2) 
Solving for I
Z max
, we obtain, 
     (E-3) 
We  estimate  the  load  resistance  by  taking  the  ratio  of  the  minimum  source  voltage  to  the 
maximum  load current. Since  R 
load
  is  large and  in parallel,  it can  be  ignored. This  is the  worst 
case since it represents the smallest load and therefore the maximum load current. 
     (E-4) 
The  output  filter  capacitor  size  can  be  estimated  according  to  the  permissible  output  voltage 
variation and ripple voltage frequency and is given by  
      (E-5)  
Since  the  voltage  gain  of  an  EF  amplifier  is  unity,  the  output  voltage  of  teh  regulated  power 
supply is, 
V
load
=V
Z
 - V
BE
   (E-6) 
The percent regulation of the power supply is given by 
      (E-7) 
Voltage Regulator 
The  maximum  power  dissipated  in  this  type  of  series  regulator  is  the  power  dissipated  in  the 
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internal pass transistor, which  is approximately (V
S  max
 - V
out
) I
L  max
. Hence, as the  load current 
increases,  the  power  dissipated  in  the  internal  pass  transistor  increases.  If  I
Load
  exceeds  0.75  A, 
the  IC  package  should  be  secured  to  a  heat  sink.  When  this  is  done,  I
Load
  can  increase  to  about 
1.5 A.  
We  now focus our attention on the 78XX series of regulators. The last two digits of the IC part 
number denote the output voltage of the device. Thus, for example, a 7808 IC package produces 
an 8V regulated output. These packages, although  internally complex, are  inexpensive and easy 
to use.  
There are a number of different voltages that can be obtained from the 78XX series 1C; they are 
5, 6, 8, 8.5, 10, 12, 15, 18, and 24 V. In order to design a regulator around one of these ICs, we 
need  only  select  a  transformer,  diodes,  and  filter.  The  physical  configuration  is  shown  in  fig. 
3(a). The ground lead and the metal tab are connected together. This permits direct attachment to 
a heat sink for cooling purposes. A typical circuit application is shown in fig. 3(c).  
 
(a) 
 
(b) 
 
(c) 
Fig. 3  
The  specification  sheet  for  this  IC  indicates  that  there  must  be  a  common  ground  between  the 
input and output, and the minimum voltage at the IC input must be above the regulated output. In 
order to assure this last condition, it is necessary to filter the output from the rectifier. The C
F
 in 
fig. 3(b) performs this filtering when combined with the input resistance to the IC. We use an n:1 
step down transformer, with the secondary winding center-tapped, to drive a full-wave rectifier.  
 
 
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The  minimum  and  maximum  input  voltages  for  the  78XX  family  of  regulators  are  shown  in 
Table-1.  
Type  Min  Max 
7805  7  25 
7806  8  25 
7808  10.5  25 
7885  10.5  25 
7810  12.5  28 
7812  14.5  30 
7815  17.5  30 
7818  21  33 
7824  27  38 
Table - 1  
We  use  Table  -1  to  select  the  turns  ratio,  n,  for  a  78XX  regulator.  As  a  design  guide,  we  will 
take the average of V
max
 and V
min
 of the particular IC regulator to calculate n. For example, using 
a 7805 regulator, we obtain  
 
The center tap provides division by 2 so the peak voltage out of the rectifier is 115 2 / 2n = 16. 
Therefore, n = 5. This is a conservative method of selecting the transformer ratio.  
The filter capacitor, C
F
, is chosen to maintain the voltage input range to the regulator as specified 
in Table 8.1.  
The  output  capacitor,  C
Load
,  aids  in  isolating  the  effect  of  the  transients  that  may  appear  on  the 
regulated supply line. C
Load
 should be a high quality tantalum capacitor with a capacitance of 1.0 
F. It should be connected close to the 78XX regulator using short leads in order to improve  the 
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stability performance.  
This family of regulators can also be used for battery powered systems. Fig. 3(c) shows a battery 
powered application. The value of C
F
 is chosen in the same manner as for the standard filter.  
The  79XX  series  regulator  is  identical  to  the  78XX  series  except  that  it  provides  negative 
regulated voltages instead of positive.  
 
UNIVERSITY QUESTIONS  
1. What is  mean by depletion region? 
2. Define the transition capacitance  of a diode. 
3. Differentiate a PN junction diode and zener diode. 
4. Give the diode current equation. 
5. Define cutin voltage. 
6. What  assumptions are made while analyzing the motion of an electron in an electric field? 
7. How do you increase the conductivity of intrinsic semiconductor? 
8. What is Hall effect? 
9.  How  do  the  transition  region  width  and  contact  potential  across  a  pn  junction  vary  with  the 
applied bias voltage? 
10. Mention the two mechanisms of breakdown in a pn junction. 
11. State law of mass action. 
12. Why is the mobility of electrons greater than the holes? 
13.  The  reverse  saturation  current  of  a  silicon  PN  junction  diode  is  10  A.Calculate  the  diode 
current for the forward bias voltage of 0.6 V at 25 C. 
14. Give the equation for diode current under reverse bias. 
15. Compare LED and LCD. 
16. Define the potential-energy barrier. 
17. What is  mean by  Diffusion capacitance? 
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18. Name any two material used to manufacture LEDs. 
19. What is precision rectifier? 
20. Find the ripple factor for a FWR with capacitor filter with the output waveform as shown in 
the figure.Assume RL=100  with capacitor C=1000F. 
21. Derive  the ripple factor for a HWR and FWR . 
22. Why a series resistor is necessary when a diode is forward biased? 
23. List any four applications of light emitting diode. 
 
BIG QUESTIONS 
1. With the volt-ampere characteristics,explain the working principle of the diode and also 
explain the static ,dynamic resistance of the diodes?                                          (16) 
2. Write a detailed note on: 
i) diode switching times  (6) 
ii)applications of diodes. (4) 
iii)capacitance of diodes.(6) 
3. Zener diode can be used as a voltage regulator-Justify it.(8) 
4.  Explain  the  working  of  a  PN  junction  diode  under  various  biasing  conditions  using  the 
relevant circuit sketch.    (16) 
5. Explain how a PN junction is formed? (8). 
6. Write a note on diode capacitance.(8) 
7. Write a detailed note on: LED (8) 
8. Describe the conduction of current in an intrinsic semiconductor.(8) 
9. Find the conductivity and resistivity of an intrinsic semiconductor at temperature of 300k.It is 
given that 
Ni=2.5*1013/cm3,n=3800cm2/Sv; 
p=1800 cm2/Sv,q=1.6*10-19 C                           (8) 
10. Derive the continuity equation for a semiconductor.          (10) 
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11.In an N-type semiconductor ,the Fermi-level lies 0.3 Ev below the conduction band at 27 C .If 
the temperature is increased to 55 C ,find the new position of the Fermi level.(6) 
12. Give the theory of current components of pn junction diode.(10) 
13. Determine the ac resistance for a semiconductor diode having a forward bias of 200 mV and 
reverse saturation current of 1A at room temperature.(6) 
14. Derive an expression for the diffusion capacitance of a pn junction diode.      (8) 
15. What is zener effect ?Explain the function of a zener diode and draw its characteristics. (10) 
16. Write a note on temperature dependence of breakdown voltages. (6) 
17.  Derive  an  expression  for  total  current  in  a  semiconductor  due  to  drift  and  diffusion 
phenomena. 
18. What is meant by carrier life time? Discuss. (6) 
19. Describe the action of the PN junction diode under forward and reverse biased conditions and 
hence draw  the volt amp characteristics of the diode .  (10) 
20. Distinguish between avalanche breakdown and zener breakdown.  (8) 
21.Explain the switching characteristics of PN junction diode.  (8) 
22. Derive an expression for the current   under  forward  bias  and reverse bias.    (10) 
23.  The  diode  current  is  0.6  Ma,when  the  applied  voltage  is  400  Mv  20Ma    when  the  applied 
voltage is 500Mv.Determine  .Assume kt/q=25Mv. 
24. Explain the effect of temperature on PN junction diodes.   (5) 
25. Explain the use of zener diode as voltage regulator .   (6) 
26.With neat diagram explain the operation of LCD. 
27. Discuss the V-I characteristics of P-N junction diode and zener diode. 
28. Explain the operation of full wave rectifier. Also derive the expression  for its average output 
voltage. 
29. Derive  the ripple factor for FWR with capacitor filter.        (10) 
30.Explain  in  detailabout  the  operation    of  the  following    type    of  filters  and  derive  the  ripple 
factor for all i)C-filter  ii) L-filter  iii)LC-filter  iv)CLC-filter                  (16) 
31. Explain in detail the operation of the electronic voltage regulators. 
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                                 UNIT 2 
  Bipolar Junction Transistor And Its Applications 
 
Introduction 
A bipolar (junction) transistor (BJT) is a three-terminal electronic device constructed of doped 
semiconductor  material  and  may  be  used  in  amplifying  or  switching  applications.  Bipolar 
transistors are so named because their operation  involves both  electrons and holes. Charge  flow 
in a BJT is due to bidirectional diffusion of charge carriers across a junction between two regions 
of  different  charge  concentrations.  This  mode  of  operation  is  contrasted  with  unipolar 
transistors,  such  as  field-effect  transistors, in which only one carrier type  is  involved  in charge 
flow  due  to  drift.  By  design,  most  of  the  BJT  collector  current  is  due  to  the  flow  of  charges 
injected  from  a  high-concentration  emitter  into  the  base  where  they  are  minority  carriers  that 
diffuse toward the collector, and so BJTs are classified as minority-carrier devices. 
 
PNP 
 
NPN 
Schematic symbols for 
PNP- and NPN-type 
BJTs. 
-   
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NPN BJT with forward-biased EB junction and reverse-biased BC junction 
An NPN transistor can be considered as two diodes with a shared anode. In typical operation, the 
base-emitter  junction  is  forward  biased  and  the  basecollector  junction  is  reverse  biased.  In  an 
NPN transistor, for example, when a positive voltage is applied to the baseemitter junction, the 
equilibrium between thermally generated carriers and the repelling electric field of the depletion 
region  becomes unbalanced, allowing thermally  excited electrons to  inject  into the base region. 
These  electrons  wander  (or  "diffuse")  through  the  base  from  the  region  of  high  concentration 
near the emitter towards the region of  low concentration near the collector. The electrons  in the 
base are called  minority carriers  because the base  is  doped p-type which would  make  holes the 
majority carrier in the base. 
To  minimize  the  percentage  of  carriers  that  recombine  before  reaching  the  collectorbase 
junction,  the  transistor's  base  region  must  be  thin  enough  that  carriers  can  diffuse  across  it  in 
much less time than the semiconductor's minority carrier lifetime. In particular, the thickness of 
the base must be much less than the diffusion length of the electrons. The collectorbase junction 
is  reverse-biased,  and  so  little  electron  injection  occurs  from  the  collector  to  the  base,  but 
electrons  that  diffuse  through  the  base  towards the  collector  are  swept  into the  collector  by  the 
electric  field  in  the  depletion  region  of  the  collectorbase  junction.  The  thin  shared  base  and 
asymmetric collectoremitter doping is what differentiates a bipolar transistor from two separate 
and oppositely biased diodes connected in series. 
Voltage, current, and charge control 
The  collectoremitter  current  can  be  viewed  as  being  controlled  by  the  baseemitter  current 
(current control), or by the baseemitter voltage (voltage control). These views are related by the 
currentvoltage relation of the baseemitter junction, which is just the usual exponential current
voltage curve of a p-n junction (diode).
[1]
 
The  physical  explanation  for  collector  current  is  the  amount  of  minority-carrier  charge  in  the 
base  region.
[1][2][3]
  Detailed  models  of  transistor  action,  such  as  the  GummelPoon  model, 
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account for the distribution of this charge explicitly to explain transistor behavior more exactly.
[4]
 
The  charge-control  view  easily  handles  phototransistors,  where  minority  carriers  in  the  base 
region  are  created  by  the  absorption  of  photons,  and  handles  the  dynamics  of  turn-off,  or 
recovery time, which depends on charge in the base region recombining. However, because base 
charge  is  not  a  signal  that  is  visible  at the  terminals,  the  current-  and  voltage-control  views  are 
generally used in circuit design and analysis. 
In analog circuit design, the current-control view is sometimes used because it is approximately 
linear.  That  is,  the  collector  current  is  approximately  
F
  times  the  base  current.  Some  basic 
circuits  can  be  designed  by  assuming  that  the  emitterbase  voltage  is  approximately  constant, 
and  that  collector  current  is  beta  times  the  base  current.  However,  to  accurately  and  reliably 
design  production  BJT  circuits,  the  voltage-control  (for  example,  EbersMoll)  model  is 
required
[1]
. The voltage-control model requires an exponential function to be taken into account, 
but when it is linearized such that the transistor can be modelled as a transconductance, as in the 
EbersMoll  model,  design  for  circuits  such  as  differential  amplifiers  again  becomes  a  mostly 
linear  problem,  so the  voltage-control  view  is  often  preferred.  For  translinear  circuits,  in  which 
the exponential IV curve is key to the operation, the transistors are usually modelled as voltage 
controlled  with  transconductance  proportional  to  collector  current.  In  general,  transistor  level 
circuit  design  is  performed  using  SPICE  or  a  comparable  analogue  circuit  simulator,  so  model 
complexity is usually not of much concern to the designer. 
Turn-on, turn-off, and storage delay 
The  Bipolar  transistor  exhibits  a  few  delay  characteristics  when  turning  on  and  off.  Most 
transistors, and especially power transistors, exhibit long base storage time that limits maximum 
frequency of operation in switching applications. One method for reducing this storage time is by 
using a Baker clamp. 
Transistor 'alpha' and 'beta'  
The proportion of electrons able to cross the base and reach the collector is a measure of the BJT 
efficiency.  The  heavy  doping  of  the  emitter  region  and  light  doping  of  the  base  region  cause 
many more electrons to be injected from the emitter into the base than holes to be injected from 
the  base  into  the  emitter.  The  common-emitter  current  gain  is  represented  by  
F
  or  h
fe
;  it  is 
approximately  the  ratio  of  the  DC  collector  current  to  the  DC  base  current  in  forward-active 
region. It is typically greater than 100 for small-signal transistors but can be smaller in transistors 
designed for high-power applications. Another important parameter is the  common-base current 
gain,  
F
.  The  common-base  current  gain  is  approximately  the  gain  of  current  from  emitter  to 
collector in the forward-active region. This ratio usually has a value close to unity; between 0.98 
and  0.998.  Alpha  and  beta  are  more  precisely  related  by  the  following  identities  (NPN 
transistor): 
 
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 Structure 
 
Simplified cross section of a planar NPN bipolar junction transistor 
 
 
Die of a KSY34 high-frequency NPN transistor, base and emitter connected via bonded wires 
A  BJT  consists  of  three  differently  doped  semiconductor  regions,  the  emitter  region,  the  base 
region  and  the  collector  region.  These  regions  are,  respectively,  p  type,  n  type  and  p  type  in  a 
PNP, and n type, p type and n type in a NPN transistor. Each semiconductor region is connected 
to a terminal, appropriately labeled: emitter (E), base (B) and collector (C). 
The  base  is  physically  located  between  the  emitter  and  the  collector  and  is  made  from  lightly 
doped,  high  resistivity  material.  The  collector  surrounds  the  emitter  region,  making  it  almost 
impossible for the electrons injected into the base region to escape being collected, thus making 
the resulting value of  very close to unity, and so, giving the transistor a large . A cross section 
view of a BJT indicates that the collectorbase junction has a much larger area than the emitter
base junction. 
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The bipolar junction transistor, unlike other transistors, is usually not a symmetrical device. This 
means  that  interchanging  the  collector  and  the  emitter  makes  the  transistor  leave  the  forward 
active  mode  and  start  to  operate  in  reverse  mode.  Because  the  transistor's  internal  structure  is 
usually optimized for forward-mode operation, interchanging the collector and the emitter makes 
the  values  of    and    in  reverse  operation  much  smaller  than  those  in  forward  operation;  often 
the  of the reverse mode is lower than 0.5. The lack of symmetry is primarily due to the doping 
ratios of the emitter and the collector. The emitter is heavily doped, while the collector is lightly 
doped,  allowing  a  large  reverse  bias  voltage  to  be  applied  before  the  collectorbase  junction 
breaks down. The collectorbase  junction  is reverse  biased  in  normal operation. The reason the 
emitter  is  heavily  doped  is  to  increase  the  emitter  injection  efficiency:  the  ratio  of  carriers 
injected by the emitter to those injected by the  base. For high current gain,  most of the carriers 
injected into the emitterbase junction must come from the emitter. 
The  low-performance  "lateral"  bipolar  transistors  sometimes  used  in  CMOS  processes  are 
sometimes  designed  symmetrically,  that  is,  with  no  difference  between  forward  and  backward 
operation. 
Small  changes  in  the  voltage  applied  across  the  baseemitter  terminals  causes  the  current  that 
flows  between  the  emitter  and  the  collector  to  change  significantly.  This  effect  can  be  used  to 
amplify  the  input  voltage  or  current.  BJTs  can  be  thought  of  as  voltage-controlled  current 
sources,  but  are  more  simply  characterized  as  current-controlled  current  sources,  or  current 
amplifiers, due to the low impedance at the base. 
Early  transistors  were  made  from  germanium  but  most  modern  BJTs  are  made  from  silicon.  A 
significant  minority  are  also  now  made  from  gallium  arsenide,  especially  for  very  high  speed 
applications (see HBT, below). 
NPN 
 
The symbol of an NPN bipolar junction transistor 
NPN  is  one  of  the  two  types  of  bipolar  transistors,  consisting  of  a  layer  of  P-doped 
semiconductor  (the  "base")  between  two  N-doped  layers.  A  small  current  entering  the  base  is 
amplified in the collector output. That is, an NPN transistor is "on" when its base is pulled  high 
relative to the emitter. 
Most  of  the  NPN  current  is  carried  by  electrons,  moving  from  emitter  to  collector  as  minority 
carriers in the P-type base region. Most bipolar transistors used today are NPN, because electron 
mobility  is  higher  than  hole  mobility  in  semiconductors,  allowing  greater  currents  and  faster 
operation. 
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PNP 
 
 
The symbol of a PNP Bipolar Junction Transistor. 
The other type of BJT is the PNP, consisting of a layer of N-doped semiconductor between two 
layers of P-doped material. A small current leaving the base is amplified in the collector output. 
That is, a PNP transistor is "on" when its base is pulled low relative to the emitter. 
The  arrows  in  the  NPN  and  PNP  transistor  symbols  are  on  the  emitter  legs  and  point  in  the 
direction of the conventional current flow when the device is in forward active mode. 
A mnemonic device for the NPN / PNP distinction, based on the arrows in their symbols and the 
letters in their names, is not pointing in for NPN and pointing in for PNP.
[5]
 
Heterojunction bipolar transistor 
 
 
Bands  in graded  heterojunction NPN bipolar transistor. Barriers  indicated for electrons to move 
from emitter to base, and for holes to be injected backward from base to emitter; Also, grading of 
bandgap in base assists electron transport in base region; Light colors indicate depleted regions 
The  heterojunction  bipolar  transistor  (HBT)  is  an  improvement  of  the  BJT  that  can  handle 
signals  of  very  high  frequencies  up  to  several  hundred  GHz.  It  is  common  in  modern  ultrafast 
circuits, mostly RF systems.
[6][7]
 Heterojunction transistors have different semiconductors for the 
elements of the transistor. Usually the emitter is composed of a larger bandgap material than the 
base.  The  figure  shows  that  this  difference  in  bandgap  allows  the  barrier  for  holes  to  inject 
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backward into the base, denoted in figure as 
p
, to be made large, while the barrier for electrons 
to  inject  into the  base  
n
  is  made  low.  This  barrier  arrangement  helps  reduce  minority  carrier 
injection  from  the  base  when  the  emitter-base  junction  is  under  forward  bias,  and  thus  reduces 
base current and increases emitter injection efficiency. 
The  improved  injection  of  carriers  into  the  base  allows  the  base  to  have  a  higher  doping  level, 
resulting  in  lower  resistance  to  access  the  base  electrode.  In  the  more  traditional  BJT,  also 
referred to as homojunction BJT, the efficiency of carrier injection from the emitter to the base is 
primarily  determined  by  the  doping  ratio  between  the  emitter  and  base,  which  means  the  base 
must be lightly doped to obtain high injection efficiency, making its resistance relatively high. In 
addition,  higher  doping  in  the  base  can  improve  figures  of  merit  like  the  Early  voltage  by 
lessening base narrowing. 
The grading of composition in the base, for example, by progressively increasing the amount of 
germanium in a SiGe transistor, causes a gradient in bandgap in the neutral base, denoted in the 
figure  by  
G
,  providing  a  "built-in"  field  that  assists  electron  transport  across  the  base.  That 
drift  component  of  transport  aids  the  normal  diffusive  transport,  increasing  the  frequency 
response of the transistor by shortening the transit time across the base. 
Two  commonly  used  HBTs  are  silicongermanium  and  aluminum  gallium  arsenide,  though  a 
wide  variety of  semiconductors may  be used  for the HBT structure. HBT structures are usually 
grown by epitaxy techniques like MOCVD and MBE. 
 Regions of operation 
Applied voltages 
B-E Junction 
Bias (NPN) 
B-C Junction 
Bias (NPN) 
Mode (NPN) 
E < B < C  Forward  Reverse  Forward active 
E < B > C  Forward  Forward  Saturation 
E > B < C  Reverse  Reverse  Cut-off 
E > B > C  Reverse  Forward  Reverse-active 
Bipolar transistors have five distinct regions of operation, defined by BJT junction biases. 
The  modes  of  operation  can  be  described  in  terms  of  the  applied  voltages  (this  description 
applies to NPN transistors; polarities are reversed for PNP transistors): 
Forward  active:  base  higher  than  emitter,  collector  higher  than  base  (in  this  mode  the  collector 
current is proportional to base current by 
F
). 
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-  Saturation: base higher than emitter, but collector is not higher than base. 
-  Cut-Off: base lower than emitter, but collector is higher than base. It means the transistor 
is not letting conventional current to go through collector to emitter. 
-  Reverse-action:  base  lower than emitter, collector  lower than  base: reverse conventional 
current goes through transistor. 
Applied voltages 
B-E Junction 
Bias (PNP) 
B-C Junction 
Bias (PNP) 
Mode (PNP) 
E < B < C  Reverse  Forward  Reverse-active 
E < B > C  Reverse  Reverse  Cut-off 
E > B < C  Forward  Forward  Saturation 
E > B > C  Forward  Reverse  Forward active 
In terms of junction biasing: ('reverse biased basecollector junction' means Vbc < 0 for NPN, 
opposite for PNP) 
-  Forward-active  (or  simply,  active):  The  baseemitter  junction  is  forward  biased  and  the  base
collector junction is reverse biased. Most bipolar transistors are designed to afford the greatest 
common-emitter  current  gain,  
F
,  in  forward-active  mode.  If  this  is  the  case,  the  collector
emitter  current  is  approximately  proportional  to  the  base  current,  but  many  times  larger,  for 
small base current variations. 
-  Reverse-active  (or  inverse-active  or  inverted):  By  reversing  the  biasing  conditions  of  the 
forward-active  region,  a  bipolar  transistor  goes  into  reverse-active  mode.  In  this  mode,  the 
emitter and collector regions switch roles. Because most BJTs are designed to maximize current 
gain  in  forward-active  mode,  the  
F
  in  inverted  mode  is  several  (23  for  the  ordinary 
germanium  transistor)  times  smaller.  This  transistor  mode  is  seldom  used,  usually  being 
considered  only  for  failsafe  conditions  and  some  types  of  bipolar  logic.  The  reverse  bias 
breakdown voltage to the base may be an order of magnitude lower in this region. 
-  Saturation: With both junctions forward-biased, a BJT is in saturation mode and facilitates high 
current  conduction  from  the  emitter  to  the  collector.  This  mode  corresponds  to  a  logical  "on", 
or a closed switch. 
-  Cut-off: In cut-off, biasing conditions opposite of saturation (both junctions reverse biased) are 
present. There is very little current, which corresponds to a logical "off", or an open switch. 
-  Avalanche breakdown region 
Although  these  regions  are  well  defined  for  sufficiently  large  applied  voltage,  they  overlap 
somewhat  for  small  (less  than  a  few  hundred  millivolts)  biases.  For  example,  in  the  typical 
grounded-emitter  configuration  of  an  NPN  BJT  used  as  a  pulldown  switch  in  digital  logic,  the 
"off"  state  never  involves  a  reverse-biased  junction  because  the  base  voltage  never  goes  below 
ground; nevertheless the forward bias is close enough to zero that essentially no current flows, so 
this end of the forward active region can be regarded as the cutoff region. 
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 Active-mode NPN transistors in circuits 
 
Structure and use of NPN transistor. Arrow according to schematic. 
The  diagram  opposite  is  a  schematic  representation  of  an  NPN  transistor  connected  to  two 
voltage sources. To make the transistor conduct appreciable current (on the order of 1 mA) from 
C to E,  V
BE
  must be above a  minimum  value sometimes referred to as the  cut-in voltage. The 
cut-in voltage is usually about 600 mV for silicon BJTs at room temperature but can be different 
depending  on  the  type  of  transistor  and  its  biasing.  This  applied  voltage  causes  the  lower  P-N 
junction to 'turn-on' allowing a flow of electrons from the emitter into the base. In active mode, 
the electric field existing between base and collector (caused by  V
CE
) will cause the majority of 
these electrons to cross the upper P-N junction into the collector to form the collector current I
C
. 
The remainder of the electrons recombine with holes, the majority carriers in the base, making a 
current through the  base connection to form the  base current,  I
B
. As  shown  in the diagram, the 
emitter current, I
E
, is the total transistor current, which is the sum of the other terminal currents 
(i.e.,  ). 
In  the  diagram,  the  arrows  representing  current  point  in  the  direction  of  conventional  current  
the  flow of  electrons  is  in the opposite direction  of the  arrows because  electrons carry  negative 
electric charge. In active mode, the ratio of the collector current to the base current is called the 
DC current gain. This gain  is usually 100 or more, but robust circuit designs do not depend on 
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the exact value (for example see op-amp). The value of this gain for DC signals is referred to as 
h
FE
,  and the  value  of  this  gain  for  AC  signals  is  referred  to  as  h
fe
.  However,  when  there  is  no 
particular frequency range of interest, the symbol  is used
[citation needed]
. 
It  should  also  be  noted  that  the  emitter  current  is  related  to  V
BE
  exponentially.  At  room 
temperature,  an  increase  in  V
BE
  by  approximately  60  mV  increases  the  emitter  current  by  a 
factor of 10. Because the base current is approximately proportional to the collector and emitter 
currents, they vary in the same way. 
Active-mode PNP transistors in circuits 
 
Structure and use of PNP transistor. 
The diagram opposite is a schematic representation of a PNP transistor connected to two voltage 
sources. To make the transistor conduct appreciable current (on the order of 1 mA) from E to C, 
V
EB
  must  be  above  a  minimum  value  sometimes  referred  to  as  the  cut-in  voltage.  The  cut-in 
voltage  is  usually  about  600  mV  for  silicon  BJTs  at  room  temperature  but  can  be  different 
depending  on  the  type  of  transistor  and  its  biasing.  This  applied  voltage  causes  the  upper  P-N 
junction to 'turn-on' allowing a flow of holes from the emitter into the base. In active mode, the 
electric field existing between the emitter and the collector (caused by  V
CE
) causes the majority 
of these holes to cross the lower P-N junction into the collector to form the collector current  I
C
. 
The remainder of the holes recombine with electrons, the majority carriers in the base, making a 
current through the  base connection to form the  base current,  I
B
. As  shown  in the diagram, the 
emitter current, I
E
, is the total transistor current, which is the sum of the other terminal currents 
(i.e.,  ). 
In  the  diagram,  the  arrows  representing  current  point  in  the  direction  of  conventional  current  
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the  flow  of  holes  is  in  the  same  direction  of  the  arrows  because  holes  carry  positive  electric 
charge.  In  active  mode,  the  ratio  of  the  collector  current  to  the  base  current  is  called  the  DC 
current  gain.  This  gain  is  usually  100  or  more,  but  robust  circuit  designs  do  not  depend  on  the 
exact value. The value of this gain for DC signals is referred to as h
FE
, and the value of this gain 
for  AC  signals  is  referred  to  as  h
fe
.  However,  when  there  is  no  particular  frequency  range  of 
interest, the symbol  is used
[citation needed]
. 
It  should  also  be  noted  that  the  emitter  current  is  related  to  V
EB
  exponentially.  At  room 
temperature,  an  increase  in  V
EB
  by  approximately  60  mV  increases  the  emitter  current  by  a 
factor of 10. Because the base current is approximately proportional to the collector and emitter 
currents, they vary in the same way. 
History 
The  bipolar  point-contact  transistor  was  invented  in  December  1947  at  the  Bell  Telephone 
Laboratories by John Bardeen and Walter Brattain under the direction of William Shockley. The 
junction version known as the bipolar junction transistor, invented by Shockley in 1948, enjoyed 
three decades as the device of choice in the design of discrete and  integrated circuits. Nowadays, 
the use of the BJT has declined in favor of CMOS technology in the design of digital integrated 
circuits. 
Germanium transistors 
The  germanium  transistor  was  more  common  in  the  1950s  and  1960s,  and  while  it  exhibits  a 
lower "cut off" voltage, typically around 0.2 V, making it more suitable for some applications, it 
also has a greater tendency to exhibit thermal runaway. 
Early manufacturing techniques 
Various methods of manufacturing bipolar junction transistors were developed
[8]
. 
-  Point-contact  transistor   first  type  to  demonstrate  transistor  action,  limited  commercial 
use due to high cost and noise. 
-  Grown  junction  transistor   first  type  of  bipolar  junction  transistor  made
[9]
.  Invented  by 
William  Shockley  at  Bell  Labs.  Invented  on  June  23,  1948
[10]
.  Patent  filed  on  June  26, 
1948. 
-  Alloy  junction transistor  emitter and collector alloy  beads  fused to base. Developed at 
General Electric and RCA
[11]
 in 1951.  
o  Micro alloy transistor  high speed type of alloy junction transistor. Developed at 
Philco
[12]
. 
o  Micro  alloy  diffused  transistor   high  speed  type  of  alloy  junction  transistor. 
Developed at Philco. 
o  Post  alloy  diffused  transistor   high  speed  type  of  alloy  junction  transistor. 
Developed at Philips. 
-  Tetrode  transistor   high  speed  variant  of  grown  junction  transistor
[13]
  or  alloy  junction 
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transistor
[14]
 with two connections to base. 
-  Surface  barrier  transistor   high  speed  metal  barrier  junction  transistor.  Developed  at 
Philco
[15]
 in 1953
[16]
. 
-  Drift-field  transistor   high  speed  bipolar  junction  transistor.  Invented  by  Herbert 
Kroemer
[17][18]
 at the Central Bureau of Telecommunications Technology of the German 
Postal Service, in 1953. 
-  Diffusion transistor  modern type bipolar junction transistor. Prototypes
[19]
 developed at 
Bell Labs in 1954.  
o  Diffused base transistor  first implementation of diffusion transistor. 
o  Mesa transistor  Developed at Texas Instruments in 1957. 
o  Planar  transistor   the  bipolar  junction  transistor  that  made  mass  produced 
monolithic  integrated  circuits  possible.  Developed  by  Dr.  Jean  Hoerni
[20]
  at 
Fairchild in 1959. 
-  Epitaxial transistor  a bipolar junction transistor made using vapor phase deposition. See 
epitaxy. Allows very precise control of doping levels and gradients. 
Theory and modeling 
In the discussion below, focus is on the NPN bipolar transistor. In the NPN transistor in what is 
called  active  mode  the  base-emitter  voltage  V
BE
  and  collector-base  voltage  V
CB
  are  positive, 
forward  biasing  the  emitter-base  junction  and  reverse-biasing  the  collector-base  junction.  In 
active  mode  of  operation,  electrons  are  injected  from  the  forward  biased  n-type  emitter  region 
into the p-type base where they diffuse to the reverse biased n-type collector and are swept away 
by the electric field in the reverse biased collector-base junction. For a figure describing forward 
and reverse bias, see the end of the article semiconductor diodes. 
Large-signal models 
EbersMoll model 
 
EbersMoll Model for an NPN transistor.
[21]
  
-  I
B
, I
C
, I
E
: base, collector and emitter currents 
-  I
CD
, I
ED
: collector and emitter diode currents 
-  
F
, 
R
: forward and reverse common-base current gains 
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EbersMoll Model for a PNP transistor. 
 
The DC emitter and collector currents in active mode are well modeled by an approximation to the 
EbersMoll model: 
 
 
The base internal current is mainly by diffusion (see Fick's law) and 
 
where 
-  V
T
 is the thermal voltage kT / q (approximately 26 mV at 300 K  room temperature). 
-  I
E
 is the emitter current 
-  I
C
 is the collector current 
-  
T
 is the common base forward short circuit current gain (0.98 to 0.998) 
-  I
ES
 is the reverse saturation current of the baseemitter diode (on the order of 10
15
 to 10
12
 
amperes) 
-  V
BE
 is the baseemitter voltage 
-  D
n
 is the diffusion constant for electrons in the p-type base 
-  W is the base width 
The  and forward  parameters are as described previously. A reverse  is sometimes included 
in the model. 
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The  unapproximated  EbersMoll  equations  used  to  describe  the  three  currents  in  any  operating 
region are given below. These equations are based on the transport model for a bipolar junction 
transistor.
[22]
 
 
 
 
where 
-  i
C
 is the collector current 
-  i
B
 is the base current 
-  i
E
 is the emitter current 
-  
F
 is the forward common emitter current gain (20 to 500) 
-  
R
 is the reverse common emitter current gain (0 to 20) 
-  I
S
 is the reverse saturation current (on the order of 10
15
 to 10
12
 amperes) 
-  V
T
 is the thermal voltage (approximately 26 mV at 300 K  room temperature). 
-  V
BE
 is the baseemitter voltage 
-  V
BC
 is the basecollector voltage 
Base-width modulation 
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Top: NPN base width for low collector-base reverse bias; Bottom: narrower NPN base width for large 
collector-base reverse bias. Hashed regions are depleted regions. 
Main article: Early Effect 
As the applied collectorbase voltage (V
CB
 = V
CE
  V
BE
) varies, the collectorbase depletion 
region  varies  in  size.  An  increase  in  the  collectorbase  voltage,  for  example,  causes  a  greater 
reverse  bias  across  the  collectorbase  junction,  increasing  the  collectorbase  depletion  region 
width,  and  decreasing  the  width  of  the  base.  This  variation  in  base  width  often  is  called  the 
"Early effect" after its discoverer James M. Early. 
Narrowing of the base width has two consequences: 
-  There is a lesser chance for recombination within the "smaller" base region. 
-  The charge gradient is increased across the base, and consequently, the current of minority 
carriers injected across the emitter junction increases. 
Both factors increase the collector or "output" current of the transistor in response to an increase 
in the collectorbase voltage. 
In the forward-active region, the Early effect modifies the collector current (i
C
) and the forward 
common emitter current gain (
F
) as given by:
[citation needed]
 
 
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where: 
-  V
CB
 is the collectorbase voltage 
-  V
A
 is the Early voltage (15 V to 150 V) 
-  
F0
 is forward common-emitter current gain when V
CB
 = 0 V 
-  r
o
 is the output impedance 
-  I
C
 is the collector current 
 Currentvoltage characteristics 
The following assumptions are involved when deriving ideal current-voltage characteristics of 
the BJT 
-  Low level injection 
-  Uniform doping in each region with abrupt junctions 
-  One-dimensional current 
-  Negligible recombination-generation in space charge regions 
-  Negligible electric fields outside of space charge regions. 
It is important to characterize the minority diffusion currents induced by injection of carriers. 
With regard to pn-junction diode, a key relation is the diffusion equation. 
 
A solution of this equation is below, and two boundary conditions are used to solve and find C
1
 
and C
2
. 
 
The following equations apply to the emitter and collector region, respectively, and the origins 0, 
0', and 0'' apply to the base, collector, and emitter. 
 
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A boundary condition of the emitter is below: 
 
The values of the constants A
1
 and B
1
 are zero due to the following conditions of the emitter and 
collector regions as  and  . 
 
 
Because A
1
 = B
1
 = 0, the values of n
E
(0'') and n
c
(0') are A
2
 and B
2
, respectively. 
 
 
Expressions of I
En
 and I
Cn
 can be evaluated. 
 
 
Because insignificant recombination occurs, the second derivative of p
B
(x) is zero. There is 
therefore a linear relationship between excess hole density and x. 
 
The following are boundary conditions of p
B
. 
 
 
Substitute into the above linear relation. 
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. 
With this result, derive value of I
Ep
. 
 
 
Use the expressions of I
Ep
, I
En
, p
B
(0), and p
B
(W) to develop an expression of the emitter 
current. 
 
 
 
Similarly, an expression of the collector current is derived. 
 
 
 
An expression of the base current is found with the previous results. 
 
 
Punchthrough 
When the basecollector voltage reaches a certain (device specific) value, the basecollector 
depletion region boundary meets the baseemitter depletion region boundary. When in this state 
the transistor effectively has no base.The device thus loses all gain when in this state. 
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GummelPoon charge-control model 
The GummelPoon model is a detailed charge-controlled model of BJT dynamics, which has 
been adopted and elaborated by others to explain transistor dynamics in greater detail than the 
terminal-based models typically do. This model also includes the dependence of transistor -
values upon the direct current levels in the transistor, which are assumed current-independent in 
the EbersMoll model.  
Small-signal models 
hybrid-pi model 
h- parameter model 
 
Generalized h-parameter model of an NPN BJT. 
Replace x with e, b or c for CE, CB and CC topologies respectively. 
Another  model  commonly  used  to  analyze  BJT  circuits  is  the  "h-parameter"  model,  closely 
related to the  hybrid-pi  model and the  y-parameter two-port, but using  input current and output 
voltage as independent variables, rather than input and output voltages. This two-port network is 
particularly suited to BJTs as it lends itself easily to the analysis of circuit behaviour, and may be 
used  to  develop  further  accurate  models.  As  shown,  the  term  "x"  in  the  model  represents  a 
different  BJT  lead  depending  on  the  topology  used.  For  common-emitter  mode  the  various 
symbols take on the specific values as: 
-  x = 'e' because it is a common-emitter topology 
-  Terminal 1 = Base 
-  Terminal 2 = Collector 
-  Terminal 3 = Emitter 
-  i
i
 = Base current (i
b
) 
-  i
o
 = Collector current (i
c
) 
-  V
in
 = Base-to-emitter voltage (V
BE
) 
-  V
o
 = Collector-to-emitter voltage (V
CE
) 
and the h-parameters are given by: 
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-  h
ix
 = h
ie
  The  input  impedance of the transistor (corresponding to the emitter resistance 
r
e
). 
-  h
rx
 = h
re
  Represents the dependence of the transistor's I
B
V
BE
 curve on the value of V
CE
. 
It is usually very small and is often neglected (assumed to be zero). 
-  h
fx
  =  h
fe
   The  current-gain  of  the  transistor.  This  parameter  is  often  specified  as  h
FE
  or 
the DC current-gain (
DC
) in datasheets. 
-  h
ox
  =  h
oe
   The  output  impedance  of  transistor.  This  term  is  usually  specified  as  an 
admittance and has to be inverted to convert it to an impedance. 
As  shown,  the  h-parameters  have  lower-case  subscripts  and  hence  signify  AC  conditions  or 
analyses.  For  DC  conditions  they  are  specified  in  upper-case.  For  the  CE  topology,  an 
approximate h-parameter model  is commonly used which  further simplifies the circuit analysis. 
For  this  the  h
oe
  and  h
re
  parameters  are  neglected  (that  is,  they  are  set  to  infinity  and  zero, 
respectively).  It  should  also  be  noted  that  the  h-parameter  model  as  shown  is  suited  to  low-
frequency,  small-signal  analysis.  For  high-frequency  analyses  the  inter-electrode  capacitances 
that are important at high frequencies must be added. 
Applications 
The BJT remains a device that excels in some applications, such as discrete circuit design, due to 
the  very  wide  selection  of  BJT  types  available,  and  because  of  its  high  transconductance  and 
output  resistance  compared  to  MOSFETs.  The  BJT  is  also  the  choice  for  demanding  analog 
circuits,  especially  for  very-high-frequency  applications,  such  as  radio-frequency  circuits  for 
wireless systems. Bipolar transistors can be combined with MOSFETs in an integrated circuit by 
using  a  BiCMOS  process  of  wafer  fabrication  to  create  circuits  that  take  advantage  of  the 
application strengths of both types of transistor. 
Temperature sensors 
Main article: Silicon bandgap temperature sensor 
Because  of  the  known  temperature  and  current  dependence  of  the  forward-biased  baseemitter 
junction voltage, the BJT can be used to measure temperature by subtracting two voltages at two 
different bias currents in a known ratio. 
Logarithmic converters 
Because  baseemitter  voltage  varies  as  the  log  of  the  baseemitter  and  collectoremitter 
currents,  a  BJT  can  also  be  used  to  compute  logarithms  and  anti-logarithms.  A  diode  can  also 
perform these nonlinear functions, but the transistor provides more circuit flexibility.  
Vulnerabilities 
Exposure  of  the  transistor  to  ionizing  radiation  causes  radiation  damage.  Radiation  causes  a 
buildup of  'defects'  in the  base region that act as  recombination centers. The resulting reduction 
in minority carrier lifetime causes gradual loss of gain of the transistor. 
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Power  BJTs  are  subject  to  a  failure  mode  called  secondary  breakdown,  in  which  excessive 
current and normal imperfections in the silicon die cause portions of the silicon inside the device 
to  become  disproportionately  hotter  than  the  others.  The  doped  silicon  has  a  negative 
temperature coefficient, meaning that it conducts more current at higher temperatures. Thus, the 
hottest part of the die conducts the most current, causing its conductivity to increase, which then 
causes  it  to  become  progressively  hotter  again,  until  the  device  fails  internally.  The  thermal 
runaway  process  associated  with  secondary  breakdown,  once  triggered,  occurs  almost  instantly 
and may catastrophically damage the transistor package. 
If the emitter-base junction is reverse biased into avalanche (zener) mode and current flows for a 
short period of time, the current gain of the BJT will be permanently degraded. 
Why transistor(BJT) is called a current controlled device and why it is called a nonlinear 
device? 
A bipolar junction transistor (BJT) is a type of transistor. It is a three-terminal device constructed 
of doped semiconductor material and may be used in amplifying or switching applications. 
Bipolar transistors are so named because their operation involves both electrons and holes. 
 
Although a small part of the transistor current is due to the flow of majority carriers, most of the 
transistor current is due to the flow of minority carriers and so BJTs are classified as 'minority-
carrier' devices. 
 
An NPN transistor can be considered as two diodes with a shared anode region. In typical 
operation, the emitterbase junction is forward biased and the basecollector junction is reverse 
biased. In an NPN transistor, for example, when a positive voltage is applied to the baseemitter 
junction, the equilibrium between thermally generated carriers and the repelling electric field of 
the depletion region becomes unbalanced, allowing thermally excited electrons to inject into the 
base region. These electrons wander (or "diffuse") through the base from the region of high 
concentration near the emitter towards the region of low concentration near the collector. The 
electrons in the base are called minority carriers because the base is doped p-type which would 
make holes the majority carrier in the base. 
 
The base region of the transistor must be made thin, so that carriers can diffuse across it in much 
less time than the semiconductor's minority carrier lifetime, to minimize the percentage of 
carriers that recombine before reaching the collectorbase junction. The thickness of the base 
should be less than the diffusion length of the electrons. The collectorbase junction is reverse-
biased, so little electron injection occurs from the collector to the base, but electrons that diffuse 
through the base towards the collector are swept into the collector by the electric field in the 
depletion region of the collectorbase junction. 
 
Voltage, current, and charge control 
The collectoremitter current can be viewed as being controlled by the baseemitter current 
(current control), or by the baseemitter voltage (voltage control). These views are related by the 
currentvoltage relation of the baseemitter junction, which is just the usual exponential current
voltage curve of a p-n junction (diode). 
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The physical explanation for collector current is the amount of minority-carrier charge in the 
base region. Detailed models of transistor action, such as the GummelPoon model, account for 
the distribution of this charge explicitly to explain transistor behavior more exactly. The charge-
control view easily handles photo-transistors, where minority carriers in the base region are 
created by the absorption of photons, and handles the dynamics of turn-off, or recovery time, 
which depends on charge in the base region recombining. However, since base charge is not a 
signal that is visible at the terminals, the current- and voltage-control views are usually used in 
circuit design and analysis. 
 
In analog circuit design, the current-control view is sometimes used since it is approximately 
linear. That is, the collector current is approximately F times the base current. Some basic 
circuits can be designed by assuming that the emitterbase voltage is approximately constant, 
and that collector current is beta times the base current. However, to accurately and reliably 
design production bjt circuits, the voltage-control (for example, EbersMoll) model is required 
The voltage-control model requires an exponential function to be taken into account, but when it 
is linearized such that the transistor can be modelled as a transconductance, as in the EbersMoll 
model, design for circuits such as differential amplifiers again becomes a mostly linear problem, 
so the voltage-control view is often preferred. For translinear circuits, in which the exponential 
IV curve is key to the operation, the transistors are usually modelled as voltage controlled with 
transconductance proportional to collector current. In general, transistor level circuit design is 
performed using SPICE or a comparable analogue circuit simulator, so model complexity is 
usually not of much concern to the designer. 
 
Biploar transistor: 
A transistor  is basically  a Si on Ge 
crystal  containing  three  separate 
regions.  It  can  be  either  NPN  or 
PNP type  fig. 1. The middle region 
is called the base and the outer two 
regions  are  called  emitter  and  the 
collector. The outer layers although 
they  are  of  same  type  but  their 
functions  cannot  be  changed.  They 
have  different  physical  and 
electrical properties.  
In  most  transistors,  emitter  is 
heavily  doped.  Its  job  is  to  emit  or 
inject electrons into the base. These 
bases  are  lightly  doped  and  very 
thin,  it  passes  most  of  the  emitter-
injected  electrons  on  to  the 
collector.  The  doping  level  of 
                                 
   
 
                                fig. 1 
 
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collector  is  intermediate  between 
the heavy doping of emitter and the 
light doping of the base.  
The  collector  is  so  named  because 
it  collects  electrons  from  base.  The 
collector  is  the  largest  of  the  three 
regions; it must dissipate more heat 
than  the  emitter  or  base.  The 
transistor  has  two  junctions.  One 
between  emitter  and  the  base  and 
other  between  the  base  and  the 
collector.  Because  of  this  the 
transistor  is  similar  to  two  diodes, 
one  emitter  diode  and  other 
collector base diode. 
 
The depletion layers do not have the same width, because different regions have different doping 
levels.  The  more  heavily  doped  a  region  is,  the  greater  the  concentration  of  ions  near  the 
junction.  This  means  the  depletion  layer  penetrates  more  deeply  into  the  base  and  slightly  into 
emitter. Similarly, it penetration more into collector. The thickness of collector depletion layer is 
large while the base depletion layer is small as shown in fig. 2. 
When  transistor  is  made,  the  diffusion  of  free  electrons  across  the  junction  produces  two 
depletion layers. For each of these depletion layers, the barrier potential is 0.7 V for Si transistor 
and 0.3 V for Ge transistor.  
 
  
fig. 2 
If both the junctions are forward biased using two d.c sources, as shown in  fig. 3a. free electrons 
(majority carriers) enter the emitter and collector of the transistor, joins at the base and come out 
of  the  base.  Because  both  the  diodes  are  forward  biased,  the  emitter  and  collector  currents  are 
large.  
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Fig. 3a  
 
                                     Fig. 3b 
If both the junction are reverse biased as shown in fig. 3b, then small currents flows through both 
junctions  only  due  to  thermally  produced  minority  carriers  and  surface  leakage.  Thermally 
produced  carriers  are  temperature  dependent  it  approximately  doubles  for  every  10  degree 
celsius rise in ambient temperature. The surface leakage current increases with voltage.  
When the emitter diode is forward biased and collector diode is reverse biased as shown in  fig. 4 
then one expect large emitter current and small collector current but collector current is almost as 
large as emitter current.  
 
Fig. 4  
When  emitter  diodes  forward  biased  and  the  applied  voltage  is  more  than  0.7  V  (barrier 
potential)  then  larger  number  of  majority  carriers  (electrons  in  n-type)  diffuse  across  the 
junction.  
Once the electrons are injected by the emitter enter into the base, they become minority carriers. 
These electrons do not have separate identities from those, which are thermally generated, in the 
base region itself. The base is made very thin and is very lightly doped. Because of this only few 
electrons  traveling  from  the  emitter  to  base  region  recombine  with  holes.  This  gives  rise  to 
recombination current. The rest of the electrons exist for more time. Since the collector diode is 
reverse biased, (n is connected to positive supply) therefore most of the electrons are pushed into 
collector layer. These collector elections can then flow into the external collector lead.  
Thus, there is a steady stream of electrons leaving the negative source terminal and entering the 
emitter region. The V
EB
 forward bias forces these emitter electrons to enter the base region. The 
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thin  and  lightly  doped  base  gives  almost  all  those  electrons  enough  lifetime  to  diffuse  into  the 
depletion  layer.  The  depletion  layer  field  pushes  a  steady  stream  of  electron  into  the  collector 
region.  These  electrons  leave  the  collector  and  flow  into  the  positive  terminal  of  the  voltage 
source. In most transistor, more than 95% of the emitter injected electrons flow to the collector, 
less than 5% fall into base holes and flow out the external base lead. But the collector current is 
less than emitter current. 
Relation between different currents in a transistor:  
The total current  flowing  into the transistor must be  equal to the total current  flowing out of  it. 
Hence, the emitter current I
E
 is equal to the sum of the collector (I
C
 ) and base current (I
B
). That 
is,  
I
E
 = I
C
 + I
B
  
The  currents  directions  are  positive  directions.  The  total  collector  current  I
C
  is  made  up  of  two 
components.  
1. The fraction of emitter (electron) current which reaches the collector ( a
dc
 I
E
 )  
2. The normal reverse leakage current I
CO
  
 
o
dc
 is known as large signal current gain or dc alpha. It is always positive. Since collector current 
is  almost  equal  to  the  I
E
  therefore  dc  I
E
  varies  from  0.9  to  0.98.  Usually,  the  reverse  leakage 
current is very small compared to the total collector current.  
 
NOTE: The forward bias on the emitter diode controls the number of free electrons infected into 
the  base.  The  larger  (V
BE
)  forward  voltage,  the  greater  the  number  of  injected  electrons.  The 
reverse  bias on the  collector diode  has  little  influence  on the  number of electrons that enter the 
collector.  Increasing  V
CB
  does  not  change  the  number  of  free  electrons  arriving  at the  collector 
junction layer.  
The symbol of npn and pnp transistors are shown in fig. 5. 
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Fig. 5  
Breakdown Voltages:  
Since  the  two  halves  of  a  transistor  are  diodes,  two  much  reverse  voltage  on  either  diode  can 
cause  breakdown.  The  breakdown  voltage  depends  on  the  width  of  the  depletion  layer  and  the 
doping levels. Because of the heavy doping level, the emitter diode has a low breakdown voltage 
approximately 5 to 30 V. The collector diode  is  less  heavily doped so  its  breakdown  voltage  is 
higher around 20 to 300 V.  
Common Base Configuration 
 
If the base is common to the input and output circuits, it is know as common base configuration 
as shown in fig. 1. 
 
Fig. 1  
For a pnp transistor the largest current components are due to holes. Holes flow from emitter to 
collector  and  few  holes  flow  down  towards  ground  out  of  the  base  terminal.  The  current 
directions are shown in fig. 1.  
(I
E
 = I
C
 + I
B
 ).  
For a forward biased junction, V
EB
 is positive and for a reverse biased junction V
CB
 is negative. 
The  complete  transistor  can  be  described  by  the  following  two  relations,  which  give  the  input 
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voltage V
EB
 and output current I
C
 in terms of the output voltage (V
CB
) and input current I
E
.  
V
EB
 = f
1
(V
CB
, I
E
)  
I
C
= f
2
(V
CB
, I
E
)   
The output characteristic:  
The  collector  current  I
C 
is  completely  determined  by  the  input  current  I
E
  and  the  V
CB
  voltage. 
The  relationship  is  given  in  fig.  2.  It  is  a  plot  of  I
C
  versus  V
CB
,  with  emitter  current  I
E
  as 
parameter. The curves are known as the output or collector or static characteristics. The transistor 
consists of two diodes placed in series back to back (with two cathodes connected together). The 
complete characteristic can be divided in three regions.  
 
Figure 7.2  
(1). Active region:  
In  this  region  the  collector  diode  is  reverse  biased  and  the  emitter  diode  is  forward  biased. 
Consider  first that the emitter current is zero. Then the collector current is small and equals the 
reverse saturation current I
CO
 of the collector junction considered as a diode.  
If the forward current I
B
 is increased, then a fraction of I
E
 ie. o
dc
I
E
 will reach the collector. In the 
active  region,  the  collector  current  is  essentially  independent  of  collector  voltage  and  depends 
only  upon  the  emitter  current.  Because  o
dc
  is,  less  than  one  but  almost  equal  to  unity,  the 
magnitude of the collector current is slightly less that of emitter current. The collector current is 
almost constant and work as a current source.  
The collector current slightly increases with voltage. This is due to early effect. At higher voltage 
collector  gathers  in  a  few  more  electrons.  This  reduces  the  base  current.  The  difference  is  so 
small,  that  it  is  usually  neglected.  If  the  collector  voltage  is  increased,  then  space  charge  width 
increases;  this  decreased  the  effective  base  width.  Then  there  is  less  chance  for  recombination 
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within the base region.  
(2). Saturation region:  
The region to the left of the ordinate V
CB
 = 0, and above the I
E
 = 0, characteristic in which both 
emitter and collector junction are forward biased, is called saturation region.  
When  collector  diode  is  forward  biased,  there  is  large  change  in  collector  current  with  small 
changes  in  collector  voltage.  A  forward  bias  means,  that  p  is  made  positive  with  respect  to  n, 
there  is  a  flow  of  holes  from  p  to  n.  This  changes  the  collector  current  direction.  If  diode  is 
sufficiently forward biased the current changes rapidly. It does not depend upon emitter current.  
(3). Cut off region:  
The region below I
E
 = 0 and to the right of V
CB
 for which emitter and collector junctions are both 
reversed  biased  is  referred  to  cutoff  region.  The  characteristics  I
E
  =  0,  is  similar  to  other 
characteristics but not coincident with horizontal axis. The collector current is same as I
CO
. I
CBO
 
is  frequently  used  for  I
CO
.  It  means  collector  to  base  current  with  emitter  open.  This  is  also 
temperature dependent.  
 
 
Common Base Amplifier 
The common base amplifier circuit is 
shown  in  Fig.  1.  The  V
EE
  source 
forward  biases  the  emitter  diode  and 
V
CC
  source  reverse  biased  collector 
diode. The ac source v
in
 is connected 
to  emitter  through  a  coupling 
capacitor so that it blocks dc. This ac 
voltage produces small fluctuation in 
currents  and  voltages.  The  load 
resistance  R
L
  is  also  connected  to 
collector  through  coupling  capacitor 
so  the  fluctuation  in  collector  base 
voltage will be observed across R
L
. 
The  dc  equivalent  circuit  is  obtained 
by  reducing  all  ac  sources  to  zero 
and  opening  all  capacitors.  The  dc 
collector  current  is  same  as  I
E
  and 
 
Fig. 1  
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V
CB
 is given by  
V
CB
 = V
CC
 - I
C
 R
C
.  
These current and voltage fix the Q point. The ac equivalent circuit is obtained by reducing all dc 
sources to zero and shorting all coupling capacitors. r'
e
 represents the ac resistance of the diode 
as shown in Fig. 2. 
 
Fig. 2  
Fig.  3,  shows  the  diode  curve  relating  I
E
  and  V
BE
.  In  the  absence  of  ac  signal,  the  transistor 
operates  at  Q  point  (point  of  intersection  of  load  line  and  input  characteristic).  When  the  ac 
signal is applied, the emitter current and voltage also change. If the signal is small, the operating 
point swings sinusoidally about Q point (A to B).  
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Fig .3  
If the ac signal is small, the points A and B are close to Q, and arc A B can be approximated by a 
straight line and diode appears to be a resistance given by  
 
If the input signal is small, input voltage and current will be sinusoidal but if the input voltage is 
large then current will  no  longer  be  sinusoidal  because of the  non  linearity of diode curve. The 
emitter  current  is  elongated  on  the  positive  half  cycle  and  compressed  on  negative  half  cycle. 
Therefore the output will also be distorted.  
r'
e
  is the ratio of V
BE
 and  I
E
 and  its  value depends upon the  location of Q. Higher up the  Q 
point small will be the value of r' e because the same change  in V
BE
 produces large change in I
E
. 
The slope of the curve at Q determines the value of r'
e
. From calculation it can be proved that.  
r'e = 25mV / IE  
 
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Common Base Amplifier 
Proof: 
In general, the current through a diode is given by  
 
Where  q  is  he  charge  on  electron,  V  is  the  drop  across  diode,  T  is  the  temperature  and  K  is  a 
constant.  
On differentiating w.r.t V, we get,  
 
The value of (q / KT) at 25C is approximately 40.  
Therefore,   
or,        
 
To  a  close  approximation  the  small  changes  in  collector  current  equal  the  small  changes  in 
emitter  current.  In  the  ac  equivalent  circuit,  the  current  i
C
'  is  shown  upward  because  if  i
e
' 
increases, then i
C
' also increases in the same direction.  
Voltage gain:  
Since  the  ac  input  voltage  source  is  connected  across  r'
e
.  Therefore,  the  ac  emitter  current  is 
given by  
i
e
 = V
in
 / r'
e
 
or,        V
in
 = ie r'
e
  
The output voltage is given by V
out
 = i
c
 (R
C
 || R
L
)  
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Under open circuit condition v
out
 = i
c
 R
c
 
 
 
Common Base Amplifier 
Example-1  
Find the voltage gain and output of the amplifier shown in fig. 4, if input voltage is 1.5mV.  
 
Fig. 4  
Solution:  
The emitter dc current I E is given by   
Therefore, emitter ac resistance =   
or,           A
V
= 56.6  
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and, V
out
 = 1.5 x 56.6 = 84.9 mV  
Example-2  
Repeat example-1 if ac source has resistance R s = 100 W .  
Solution:  
The ac equivalent circuit with ac source resistance is shown in fig. 5. 
 
Fig. 5  
The emitter ac current is given by   
or,                
Therefore, voltage gain of the amplifier =   
      
and,                       V
out
 = 1.5 x 8.71 =13.1 mV  
 
 
Common Emitter Configuration 
Common Emitter Curves:  
The common emitter configuration of BJT is shown in fig. 1. 
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Fig. 1 
In C.E. configuration the emitter is made common to the input and output. It is also referred to as 
grounded  emitter  configuration.  It  is  most  commonly  used  configuration.  In  this,  base  current 
and  output  voltages  are  taken  as  impendent  parameters  and  input  voltage  and  output  current  as 
dependent parameters  
V
BE
 = f
1
 ( I
B
, V
CE
 )  
I
C
 = f
2
( I
B
, V
CE 
)  
Input Characteristic:  
The  curve  between  I
B
  and  V
BE
  for  different  values  of  V
CE
  are  shown  in  fig.  2.  Since  the  base 
emitter junction of a transistor is a diode, therefore the characteristic is similar to diode one. With 
higher values of V
CE
 collector gathers slightly more electrons and therefore base current reduces. 
Normally this  effect is neglected. (Early effect). When collector is shorted with emitter then the 
input characteristic is the characteristic of a forward biased diode when V
BE
 is zero and I
B
 is also 
zero. 
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Fig. 2 
 
 
Common Emitter Configuration 
Output Characteristic:  
The  output  characteristic  is  the  curve  between  V
CE
  and  I
C
  for  various  values  of  I
B
.  For  fixed 
value of I
B 
and is shown in fig. 3. For fixed value of I
B
, I
C
 is not varying much dependent on V
CE
 
but slopes are greater than CE characteristic. The output characteristics can again be divided into 
three parts.  
 
Fig. 3  
(1) Active Region:  
In this region collector junction is reverse biased and emitter junction is forward biased. It is the 
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area to the right of V
CE
 = 0.5 V and above I
B
= 0. In this region transistor current responds most 
sensitively to I
B
. If transistor is to be used as an amplifier, it must operate in this region.  
 
If  o
dc
  is  truly  constant  then  I
C
  would  be  independent  of  V
CE
.  But  because  of  early  effect,  o
dc
 
increases  by  0.1%  (0.001)  e.g.  from  0.995  to  0.996  as  V
CE
  increases  from  a  few  volts  to  10V. 
Then |
dc
  increases  from 0.995 / (1-0.995) = 200 to 0.996 / (1-0.996) = 250 or about 25%. This 
shows  that  small  change  in  o  reflects  large  change  in  |.  Therefore  the  curves  are  subjected  to 
large variations for the same type of transistors.  
(2) Cut Off:  
Cut off in a transistor is given by I
B
 = 0, I
C
= I
CO
. A transistor is not at cut off if the base current is 
simply reduced to zero (open circuited) under this condition,  
I
C
 = I
E
= I
CO
 / ( 1-
dc
) = I
CEO
  
The actual collector current with base open is designated as I
CEO
. Since even in the neighborhood 
of cut off, o 
dc
 may be as large as 0.9 for Ge, then I
C
=10 I
CO
(approximately), at zero base current. 
Accordingly in order to cut off transistor it is not enough to reduce I
B
 to zero, but it is necessary 
to reverse bias the emitter junction slightly. It is found that reverse  voltage of 0.1 V is sufficient 
for cut off a transistor. In Si, the o 
dc
 is very nearly equal to zero, therefore, I
C
 = I
CO
. Hence even 
with I
B
= 0, I
C
= I
E
= I
CO
 so that transistor is very close to cut off.  
In summary, cut off means I
E
 = 0, I
C
 = I
CO
, I
B
 = -I
C
 = -I
CO
 , and V
BE
 is a reverse voltage whose 
magnitude is of the order of 0.1 V for Ge and 0 V for Si.  
Reverse Collector Saturation Current I
CBO
:  
When  in  a  physical  transistor  emitter  current  is  reduced  to  zero,  then  the  collector  current  is 
known as I
CBO
 (approximately equal to I
CO
). Reverse collector saturation current I
CBO
 also varies 
with temperature, avalanche  multiplication and  variability  from sample to sample. Consider the 
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circuit shown in fig. 4. V
BB
 is the reverse voltage applied to reduce the emitter current to zero.  
I
E
 = 0,          I
B
 = -I
CBO
  
If we require, V
BE
 = - 0.1 V  
Then  - V
BB
 + I
CBO
 R
B
 < - 0.1 V  
 
Fig. 4  
If R
B
 = 100 K, I
CBO
 = 100 m A, Then V
BB
 must be 10.1 Volts. Hence transistor must be capable 
to withstand this reverse voltage before breakdown voltage exceeds. 
(3).Saturation Region:  
In this region both the diodes are forward biased by at least cut in voltage. Since the voltage V
BE
 
and V
BC
 across a  forward is approximately 0.7 V therefore, V
CE
 = V
CB
 + V
BE
 = - V
BC
 + V
BE
  is 
also few tenths of volts. Hence saturation region is very close to zero voltage axis, where all the 
current  rapidly  reduces  to  zero.  In  this  region  the  transistor  collector  current  is  approximately 
given  by  V
CC
  /  R
  C
  and  independent  of  base  current.  Normal  transistor  action  is  last  and  it  acts 
like a small ohmic resistance.  
  
 
Common Emitter Configuration 
Large Signal Current Gain 
dc
 :-  
The ratio I
c
 / I
B
 is defined as transfer ratio or large signal current gain b
dc
  
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Where I
C
 is the collector current and I
B
 is the base current. The b
dc
 is an indication if how well 
the transistor works. The typical value of b
dc
 varies from 50 to 300.  
In  terms  of  h  parameters,  b 
dc
  is  known  as  dc  current  gain  and  in  designated  h
fE
  (  b 
dc
  =  h
fE
). 
Knowing the maximum collector current and b
dc
 the minimum base current can be found which 
will be needed to saturate the transistor. 
 
This expression of b
dc
 is defined neglecting reverse leakage current (I
CO
).  
Taking reverse leakage current (I
CO
) into account, the expression for the b
dc
 can be obtained as 
follows:  
b
dc
 in terms of a
dc
 is given by  
 
Since, I
CO 
= I
CBO
 
 
Cut  off  of  a  transistor  means  I
E
  =  0,  then  I
C
=  I
CBO
  and  I
B
  =  -  I
CBO
.  Therefore,  the  above 
expression b
dc
 gives the collector current increment to the base current change form cut off to I
B
 
and hence it represents the large signal current gain of all common emitter transistor.  
 
 
 
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Biasing Techniques for CE Amplifiers  
Biasing Circuit Techniques or Locating the Q - Point:  
Fixed Bias or Base Bias:  
In order for a transistor to amplify, it has to be properly biased. This means forward biasing the 
base  emitter  junction  and  reverse  biasing  collector  base  junction.  For  linear  amplification,  the 
transistor  should  operate  in  active  region  (  If  I
E
  increases,  I
C
  increases,  V
CE
  decreases 
proportionally).  
The  source  V
BB
,  through  a  current  limit  resistor  R
B
  forward  biases  the  emitter  diode  and  V
CC
 
through resistor R
C
 (load resistance) reverse biases the collector junction as shown in fig. 1. 
 
Fig. 1  
The dc base current through R
B
 is given by  
I
B
 = (V
BB
 - V
BE
) / R
B
       
or          V
BE
 = V
BB
 - I
B
 R
B
 
Normally V
BE
 is taken 0.7V or 0.3V. If exact voltage is required, then the input characteristic ( I
B
 
vs V
BE
) of the transistor should be used to solve the above equation. The load line for the input 
circuit is drawn on input characteristic. The two points of the load line can be obtained as given 
below  
For   I
B
 = 0,          V
BE 
= V
BB
.  
and      For    V
BE
 = 0,         I
B
 = V
BB
/ R
B
.  
The intersection of this line with input characteristic gives the operating point Q as shown in  
fig. 2. If an ac signal is connected to the base of the transistor, then variation in V
BE
 is about  
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Q - point. This gives variation in I
B
 and hence I
C
.  
 
Fig. 2  
 
 
Biasing Techniques for CE Amplifiers  
In the output circuit, the load equation can be written as  
V
CE
 = V
CC
- I
C
 R
C
  
This equation  involves two unknown  V
CE
  and I
C
  and therefore can  not be solved. To solve this 
equation output characteristic ( I
C
vs V
CE
) is used. 
The load equation is the equation of a straight line and given by two points:  
I
C
= 0,         V
CE 
= V
CC
  
&            V
CE
 = 0,        I
C
= V
CC 
/ R
C
 
The  intersection  of  this  line  which  is  also  called  dc  load  line  and  the  characteristic  gives  the 
operating point Q as shown in fig. 3. 
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Fig. 3  
The point at which the load line intersects with I
B
 = 0 characteristic is known as cut off point. At 
this  point  base  current  is  zero  and  collector  current  is  almost  negligibly  small.  At  cut  off  the 
emitter  diode  comes  out  of  forward  bias  and  normal  transistor  action  is  lost.  To  a  close 
approximation.  
V
CE
 ( cut off) ~ V
CC
 (approximately).  
The  intersection of the  load  line and I
B
 = I
B(max)
 characteristic  is known as saturation point . At 
this point I
B
= I
B(max)
, I
C
= I
C(sat)
. At this point collector diodes comes out of reverse bias and again 
transistor action is lost. To a close approximation, 
I
C(sat)
 ~ V
CC
 / R
C
(approximately ).  
The I
B(sat)
 is the minimum current required to operate the transistor in saturation region. If the I
B
 
is  less than I
B  (sat)
, the transistor will operate in active region. If I
B
 > I
B  (sat)
  it always operates  in 
saturation region.  
If the transistor operates at saturation or cut off points and no where else then it is operating as a 
switch is shown in fig. 4.  
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Fig. 4 
V
BB
 = I
B
 R
B
+ V
BE
 
I
B
 = (V
BB
  V
BE
 ) / R
B
  
If I
B
> I
B(sat)
, then it operates at saturation, If I
B
 = 0, then it operates at cut off.  
If a transistor is operating as an amplifier then Q point must be selected carefully. Although we 
can select the operating point any where in the active region by choosing different values of R
B
 
& R
C
 but the various transistor ratings such as maximum collector dissipation P
C(max)
 maximum 
collector voltage V
C(max)
 and I
C(max)
 & V
BE(max)
 limit the operating range. 
Once  the  Q  point  is  established  an  ac  input  is  connected.  Due  to  this  the  ac  source  the  base 
current  varies.  As  a  result  of  this  collector  current  and  collector  voltage  also  varies  and  the 
amplified output is obtained. 
If  the  Q-point  is  not  selected  properly  then  the  output  waveform  will  not  be  exactly  the  input 
waveform. i.e. It may be clipped from one side or both sides or it may be distorted one.  
 
 
Biasing Techniques for CE Amplifiers  
Example-1  
Find the transistor current in the circuit shown in fig. 5, if I
CO
= 20nA,  =100. 
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Solution:  
For the base circuit, 5 = 200 x IB + 0.7 
Therefore,    
Since I
CO
 << I
B
, therefore, I
C
 =  I
B
 = 2.15 mA 
From the collector circuit, V
CE
 = 10 - 3 x 2.15 = 3.55 V 
Since, V
CE
 = V
CB
 + V
BE
 
Thus, V
CB
 = 3.55 - 0.7 = 2.55 V 
Therefore,  collector  junction  is  reverse  biased  and 
transistor is operating in its active region.  
 
Fig. 5  
Example - 2 
If  a  resistor  of  2K  is  connected  in  series  with  emitter  in 
the  circuit  as  shown  in  fig.  6,  find  the  currents.  Given 
I
CO
= 20 nA,  =100.  
Solution: 
I
E
 = I
B
 + I
C
 = I
B
 + 100 I
B
 = 101 I
B
 
For the base circuit, 5 = 200 x I
B
 + 0.7 + 2k x 101 I
B
 
Therefore,     
Since I
CO
 << I
B
, therefore, I
C
 = I
B
 = 1.07 mA 
From the collector circuit, V
CB
 = 10 - 3 x 1.07 - 0.7 - 2 x 
101 x 0.0107 = 3.93 V 
Therefore  collector  junction  is  reverse  biased  and 
transistor is operating in its active region.  
 
Fig. 6  
 
 
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Example - 3 
Repeat the example-1 if R
B
 is replaced by 50k.  
Solution:  
The circuit is shown in fig. 7. 
Since the base resistance is reduced, the base current must 
have increased and there is a possibility that the transistor 
has entered into saturation region.  
Assuming transistor is operating in its saturation region,  
V
BE (sat)
= 0.8 V and V
CE (sat)
 = 0.2V  
Therefore,   
and             
The  minimum  base  current  required  for  operating  the 
transistor in saturation region is  
 
Since  I
B
  >  I
B(min)
,  therefore,  transistor  is  operating  in  its 
saturation region. 
 
Fig. 7  
Example - 4 
Repeat the example-2 if R
B
 is replaced by 50k.  
Solution:  
The circuit is shown in fig. 8. 
Since the base resistance is reduced, the base current must 
have increased and there is a possibility that the transistor 
has entered into saturation region.  
Assuming transistor is operating in its saturation region,  
 
Fig. 8  
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Solving these equations, we get,  
I
C
 = 1.96mA and I
B
 = 0.0035mA  
The  minimum  base  current  required  for  operating  the 
transistor in saturation region is  
 
Since I B < I B(min) , therefore, transistor is operating in 
its  active  region  and  not  in  saturation.  The  base  and  the 
collector  currents  can  be  recalculated  assuming  the 
transistor to be in active region.  
For the base circuit, 5 = 50 x I
B
 + 0.7 + 2k x 101 I
B
 
Therefore,   
    I
C
 = 1.71mA  
From the collector circuit, V
CB
 = 10 - 3 x 1.71 - 0.7 - 2 x 
101 x 0.0171 = 0.716 V 
 
 
Stability of Operating Point 
Let us consider three operating points of transistor operating in common emitter amplifier.  
1.  Near cut off  
2.  Near saturation  
3.  In the middle of active region  
If the operating point is selected near the cutoff region, the output is clipped in negative half cycle as shown in fig. 1.  
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Fig. 1  
If  the  operating  point  is  selected  near  saturation  region,  then  the  output  is  clipped  in  positive 
cycle as shown in fig. 2. 
 
 
Fig. 2  Fig. 3 
If the operating point is selected in the middle of active region, then there is no clipping and the 
output follows input faithfully as shown in fig. 3. If input is large then clipping at both sides will 
take place. The first circuit for biasing the transistor is CE configuration is fixed bias.  
In biasing circuit shown in fig. 4(a), two different power supplies are required. To avoid the use 
of two supplies the base resistance R
B
 is connected to V
CC
 as shown in fig. 4(b).  
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Fig. 4(a)   Fig. 4(b) 
Now V
CC
 is still forward biasing emitter diode. In this circuit Q point is very unstable. The base 
resistance R
B
 is selected by noting the required base current I
B
 for operating point Q.  
I
B
 = (V
CC
  V
BE
 ) / R
B
  
Voltage across base emitter junction is approximately 0.7 V. Since V
CC
 is usually very high  
i.e. I
B
 = V
CC
/ R
B
 
Since I
B
 is constant therefore it is called fixed bias circuit.  
 
 
Biasing 
Stability of quiescent operating point:  
Let  us  assume  that the  transistor  is  replaced  by  an  other  transistor of  same  type.  The  |
dc
  of  the 
two transistors of same type may not be same. Therefore, if |
dc
 increases then for same I
B
, output 
characteristic shifts upward. If |
dc
 decreases, the output characteristic shifts downward. Since I
B
 
is maintained constant, therefore the operating point shifts from Q to Q
1
 as shown in fig. 5. The 
new operating point may be completely unsatisfactory.  
Therefore, to  maintain  operating  point  stable,  I
B
  should  be  allowed  to  change  so  as to  maintain 
V
CE
 & I
C
 constant as |
dc
 changes.  
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Fig. 5  
A  second  cause  for  bias  instability  is  a  variation  in  temperature.  The  reverse  saturation  current 
changes  with  temperature.  Specifically,  I
CO
  doubles  for  every  10
o
C  rise  in  temperature.  The 
collector current I
C
 causes the collector junction temperature to rise, which in turn increases I
CO
. 
As  a  result  of  this  growth  I
CO
,  I
C
  will  increase  (  |
dc
  I
B
  +  (1+  | 
dc
  )  I
CO
  )  and  so  on.  It  may  be 
possible that this process goes on and the ratings of the transistors are exceeded. This increase in 
I
C
 changes the characteristic and hence the operating point. 
Stability Factor:  
The  operating  point  can  be  made  stable  by  keeping  I
C
  and  V
CE
  constant.  There  are  two 
techniques to make Q point stable. 
1.  stabilization techniques 
2.  compensation techniques  
In  first,  resistor  biasing  circuits  are  used  which  allow  I
B
  to  vary  so  as  to  keep  I
C
  relatively 
constant with variations in |
dc
 , I
CO
 and V
BE
.  
In  second,  temperature  sensitive  devices  such  as  diodes,  transistors  are  used  which  provide 
compensating voltages and currents to maintain the operating point constant.  
To  compare  different  biasing  circuits,  stability  factor  S  is  defined  as  the  rate  of  change  of 
collector current with respect to the I
CO
, keeping |
dc
 and V
CE
 constant  
S = c I
C
 / c I
CO
  
If  S  is  large,  then  circuit  is  thermally  instable.  S  cannot  be  less  than  unity.  The  other  stability 
factors are, c I
C
 / c |
dc
 and c I
C
 / c V
BE
. The  bias circuit, which provide  stability  with I
CO
, also 
show stability even if | and V
BE
changes.  
I
C
 = | 
dc
I
B
 + (I + | 
dc
 ) I
CO
  
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Differentiating with respect to I
C
,  
 
In fixed bias circuit, I
B
 & I
C
 are independent. Therefore  and S = 1 + |
dc
. If | 
dc
=100, S = 
101, which means I
C
increases 101 times as fast as I
CO
. Such a large change definitely operate the 
transistor in saturation.  
 
 
Biasing Techniques  
Emitter Feedback Bias:  
Fig.  1,  shows  the  emitter  feedback  bias  circuit.  In  this  circuit,  the  voltage  across  resistor  R
E
  is 
used to offset the changes  in  b
dc
. If  b
dc
  increases,  the collector current increases. This  increases 
the emitter voltage which decrease the voltage across base resistor and reduces base current. The 
reduced base current result  in  less collector current, which partially offsets the original  increase 
in b
dc
. The feedback term is used because output current ( I
C
) produces a change in input current 
( I
B
 ). R
E
 is common in input and output circuits.  
 
Fig. 1  
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In this case  
   
Since I
E
 = I
C
 + I
B
 
 
Therefore, 
 
In this case, S is less compared to fixed bias circuit. Thus the stability of the Q point is better. 
Further, 
 
If I
C
 is to be made insensitive to 
dc
 than 
 
R
E
 cannot be made large enough to swamp out the effects of 
dc
 without saturating the transistor.  
Collector Feedback Bias:  
In  this  case,  the  base  resistor  is  returned  back  to  collector  as  shown  in  fig.  2.  If  temperature 
increases. 
dc
 increases. This produces more collectors current. As I
C
 increases, collector emitter 
voltage  decreases.  It  means  less  voltage  across  R
B
  and  causes  a  decrease  in  base  current  this 
decreasing I
C
, and compensating the effect of |
dc
.  
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Fig. 2 
In this circuit, the voltage equation is given by  
 
Circuit is stiff sensitive to changes in 
dc
. The advantage is only two resistors are used. 
Then, 
 
Therefore, 
 
It is better as compared to fixed bias circuit. 
Further, 
 
Circuit is still sensitive to changes in 
dc
. The advantage is only two resistors are used. 
 
 
 
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Biasing Techniques 
Voltage Divider Bias:  
If  the  load  resistance  R
C
  is  very  small,  e.g.  in  a  transformer  coupled  circuit,  then  there  is  no 
improvement in stabilization in the collector to base bias circuit over fixed bias circuit. A circuit 
which  can  be  used  even  if  there  is  no  dc  resistance  in  series  with  the  collector,  is  the  voltage 
divider bias or self bias. fig. 3.  
The current in the resistance R
E
 in the emitter lead causes a voltage drop which is in the direction 
to reverse bias the emitter junction. Since this junction must be forward biased, the base voltage 
is obtained from the supply through R
1
, R
2
 network. If R
b
 = R
1
 || R
2
 equivalent resistance is very 
 very small, then V
BE
 voltage is independent of I
CO
 and  I
C
 /  I
CO
  0. For best stability R
1
 & 
R
2
 must be kept small.  
 
Fig. 3  
If  I
C
  tends  to  increase,  because  of  I
CO
,  then  the  current  in  R
C
  increases,  hence  base  current  is 
decreased because of more reverse biasing and it reduces I
C
 .  
To analysis this circuit, the base circuit is replaced by its thevenin's equivalent as shown in fig. 4. 
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Fig. 4  
Thevenin's voltage is 
 
R
b
 is the effective resistance seen back from the base terminal. 
 
If V
BE
 is considered to be independent of I
C
, then 
 
 
The smaller the value of R
b
, the better is the stabilization but S cannot be reduced be unity. 
Hence  I
C
  always  increases  more  than  I
CO
.  If  R
b
  is  reduced, then  current  drawn  from  the  supply 
increases. Also if R
E
 is increased then to operate at same Q-point, the magnitude of V
CC
 must be 
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increased. In both the cases the power loss increased and reduced h.  
In  order  to  avoid  the  loss  of  ac  signal  because  of  the  feedback  caused  by  R
E
,  this  resistance  is 
often  by  passed  by  a  large  capacitance  (>  10  m  F)  so  that  its  reactance  at  the  frequency  under 
consideration is very small.  
 
 
Biasing Techniques 
Emitter Bias:  
Fig. 5, shown the emitter bias circuit. The circuit gets this name because the negative supply V
EE
 
is used to forward bias the emitter junction through resistor R
E
. V
CC
 still reverse biases collector 
junction.  This  also  gives  the  same  stability  as  voltage  divider  circuit  but  it  is  used  only  if  split 
supply is available.  
 
Fig. 5  
In this circuit, the voltage equation is given by  
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Biasing Techniques  
Example-1  
Determine the Q-point  for the CE amplifier given  in  fig. 1,  if  R
1
 = 1.5K O and R
s
  = 7K O . A 
2N3904 transistor is used with  = 180, R
E
 = 100O and R
C
 = R
load
 = 1K O . Also determine the 
P
out
(ac) and the dc power delivered to the circuit by the source.  
 
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Fig. 1  
Solution: 
We first obtain the Thevenin equivalent. 
 
and   
 
Note that this is not a desirable Q-point location since V
BB
 is very close to V
BE
. Variation in V
BE
 
therefore significantly  change I
C
.We  find  R
ac
 =  R
C
 || R
load
= 500  W  and R
dc
  = R
C
 + R
E
 =1.1KO. 
The value of V
CE
 representing the quiescent value associated with I
CQ
 is found as follows, 
 
Then 
 
Since  the  Q-point  is  on  the  lower  half  of  the  ac  load  line,  the  maximum  possible  symmetrical 
output voltage swing is  
 
The ac power output can be calculated as 
 
The power drawn from the dc source is given by 
 
The power loss in the transistor is given by 
 
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The  Q-point  in  this  example  is  not  in  the  middle  of  the  load  line  so  that output  swing  is  not  as 
great  as  possible.  However,  if  the  input  signal  is  small  and  maximum  output  is  not  required,  a 
small I
C
 can be used to reduce the power dissipated in the circuit. 
 
 Biasing Techniques  
Moving Ground Around:  
Ground  is  a  reference  point  that  can  be  moved  around.  e.g.  consider  a  collector  feedback  bias 
circuit. The various stages of moving ground are shown in fig. 2. 
 
Fig. 2  
Biasing a pnp Transistor:  
The  biasing  of  pnp  transistor  is  done  similar  to  npn  transistor  except that  supply  is  of  opposite 
polarity The various biasing circuits of pnp transistor are shown in fig. 3. 
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Fig. 3  
Example 2: 
For the circuit shown in fig. 4, calculate I
C
 and V
CE
  
Solution: 
 
 
Fig. 4  
 
 
 
 
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Small Signal CE Amplifiers 
Small Signal CE Amplifiers:  
CE amplifiers are very popular to amplify the small signal ac. After a transistor has been biased 
with  a  Q  point  near  the  middle  of  a  dc  load  line,  ac  source  can  be  coupled  to  the  base.  This 
produces fluctuations in the base current and hence in the collector current of the same shape and 
frequency. The output will be enlarged sine wave of same frequency.  
The amplifier  is  called  linear  if  it does  not change the wave shape of the signal.  As  long as the 
input  signal  is  small,  the  transistor  will  use  only  a  small  part of  the  load  line  and  the  operation 
will be linear.  
On the other hand, if the input signal is too large. The fluctuations along the load line will drive 
the transistor into either saturation or cut off. This clips the peaks of the input and the amplifier is 
no longer linear.  
The CE amplifier configuration is shown in fig. 1. 
 
Fig. 1 
The coupling capacitor (C
C
 ) passes an ac signal  from one point to another. At the same time  it 
does not allow the dc to pass through it. Hence it is also called blocking capacitor.  
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Fig. 2 
For example in fig. 2, the ac voltage at point A is transmitted to point B. For this series reactance 
X
C
 should  be  very  small compared to  series resistance R
S
. The circuit to the  left of  A  may  be  a 
source and a series resistor or may be the Thevenin equivalent of a complex circuit. Similarly R
L
 
may be the load resistance or equivalent resistance of a complex network. The current in the loop 
is given by  
 
As  frequency  increases, decreases,  and  current  increases  until  it  reaches  to  its 
maximum  value  v
in
 / R. Therefore the capacitor couples the signal properly  from  A to B when 
X
C
<<  R.  The  size  of  the  coupling  capacitor  depends  upon  the  lowest  frequency  to  be  coupled. 
Normally, for lowest frequency X
C
 s 0.1R is taken as design rule.  
The coupling capacitor acts like a switch, which is open to dc and shorted for ac.  
The bypass capacitor C
b
 is similar to a coupling capacitor, except that it couples an ungrounded 
point  to  a  grounded  point.  The  C
b
  capacitor  looks  like  a  short  to  an  ac  signal  and  therefore 
emitter is said ac grounded. A bypass capacitor does not disturb the dc voltage at emitter because 
it looks open to dc current. As a design rule X
Cb
 s 0.1R
E
 at lowest frequency.  
 
 
Small Signal CE Amplifiers 
Analysis of CE amplifier:  
In a transistor amplifier, the dc source sets up quiescent current and voltages. The ac source then 
produces fluctuations in these current and voltages. The simplest way to analyze this circuit is to 
split the analysis in two parts: dc analysis and ac analysis. One can use superposition theorem for 
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analysis .  
AC & DC Equivalent Circuits:  
For  dc  equivalent  circuit,  reduce  all  ac  voltage  sources  to  zero  and  open  all  ac  current  sources 
and open all capacitors. With this reduced circuit shown in  fig. 3 dc current and voltages can be 
calculated.  
 
Fig. 3  
For ac equivalent circuits reduce dc  voltage sources to zero and open current sources and  short 
all capacitors. This circuit is used to calculate ac currents and voltage as shown in  fig. 4.  
 
Fig. 4  
The  total  current  in  any  branch  is  the  sum  of  dc  and  ac  currents  through  that  branch.  The  total 
voltage across any branch is the sum of the dc voltage and ac voltage across that branch.  
Phase Inversion:  
Because  of  the  fluctuation  is  base  current;  collector  current  and  collector  voltage  also  swings 
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above  and  below the quiescent voltage. The ac output voltage  is  inverted with respect to the ac 
input voltage, meaning it is 180
o
 out of phase with input.  
During  the  positive  half  cycle  base  current  increase,  causing  the  collector  current  to  increase. 
This  produces  a  large  voltage  drop  across  the  collector  resistor;  therefore,  the  voltage  output 
decreases and negative half cycle of output voltage is obtained. Conversely, on the negative half 
cycle  of  input  voltage  less  collector  current  flows  and  the  voltage  drop  across  the  collector 
resistor decreases, and hence collector voltage increases we get the positive half cycle of output 
voltage as shown in fig. 5. 
 
Fig. 5  
 
Analysis of CE amplifier  
AC Load line:  
Consider the dc equivalent circuit fig. 1.  
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Fig. 1  
Assuming I
C
 = I
C
(approx), the output circuit voltage equation can be written as  
 
The slop of the d.c load line is  .  
When considering the ac equivalent circuit, the output impedance becomes R
C
 || R
L
 which is less 
than (R
C
 +R
E
).  
In the absence of ac signal, this load line passes through Q point. Therefore ac load line is a line 
of slope (-1 / ( R
C
 || R
L
) ) passing through Q point. Therefore, the output voltage fluctuations will 
now be corresponding to ac load  line as shown  in  fig. 2. Under this condition, Q-point is not in 
the  middle  of  load  line,  therefore  Q-point  is  selected  slightly  upward,  means  slightly  shifted  to 
saturation side.  
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Fig. 2  
 
 
Analysis of CE amplifier  
Voltage gain:  
To find the voltage gain, consider an unloaded CE amplifier. The ac equival ent circuit is 
shown  in  fig.  3.  The  transistor  can  be  replaced  by  its  collector  equivalent  model  i.e.  a 
current source and emitter diode which offers ac resistance r'
e
.  
 
Fig. 3 
The input voltage appears directly across the emitter diode.  
Therefore emitter current i
e
 = V
in
 / r'
e
.  
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Since,  collector  current  approximately  equals  emitter  current  and  i
C
  =  i
e
  and  v
out
  =  -  i
e
  R
C
  (The 
minus sign is used here to indicate phase inversion)  
Further v
out
 = - (V
in
 R
C
) / r'
e
 
Therefore voltage gain A = v
out
 / v
in
 = -R
C
 / r'
e
  
The ac source driving an amplifier has to supply alternating current to the amplifier. The 
input impedance of an  amplifier determines how  much current the amplifier takes from 
the ac source.  
In a normal frequency range of an amplifier, where all capacitors look like ac shorts and 
other reactance are negligible, the ac input impedance is defined as  
z
in
= v
in
/ i
in
  
Where v
in
, i
in
 are peak to peak values or rms values  
The impedance looking directly into the base is symbolized z
in (base)
 and is given by  
  Z 
in(base)
 = v
in
 / i
b
 ,  
Since,v 
in
 = i
e
 r'
e
   
                   b
i
 b r'
e
  
  z
in (base)
 = b r'
e
.  
From the ac equivalent circuit, the input impedance z
in
 is the parallel combination of R
1
 , 
R
2
 and b r'
e
.  
Z
in
 = R
1
 || R
2
 || b r'
e
  
The Thevenin voltage appearing at the output is  
v
out
 = A v
in
  
The Thevenin impedance is the parallel combination of R
C
 and the internal impedance 
of the current source. The collector current source is an ideal source, therefore it has an 
infinite internal impedance.  
z
out
 = R
C
.  
The simplified ac equivalent circuit is shown in fig. 4.  
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Fig. 4  
 
h-Parameters 
Small signal low frequency transistor Models:  
All  the  transistor  amplifiers  are  two  port  networks  having  two  voltages  and  two  currents.  The 
positive directions of voltages and currents are shown in fig. 1. 
 
Fig. 1  
Out  of  four  quantities  two  are  independent  and  two  are  dependent.  If  the  input  current  i
1
  and 
output  voltage  v
2
  are  taken  independent then  other two  quantities  i
2
  and  v
1
  can  be  expressed  in 
terms of i
1
 and V
2
.  
 
The equations can be written as 
 
where h
11
, h
12
, h
21
 and h
22
 are called h-parameters. 
 
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        = h
i
 = input impedance with output short circuit to ac. 
 
=h
r
  =  fraction  of  output  voltage  at  input  with  input open  circuited  or  reverse  voltage  gain  with 
input open circuited to ac (dimensions). 
 
= h
f
 = negative of current gain with output short circuited to ac. 
The current entering the load is negative of I
2
. This is also known as forward short circuit current 
gain. 
 
= h
o
 = output admittance with input open circuited to ac. 
If  these  parameters  are  specified  for  a  particular  configuration,  then  suffixes  e,b  or  c  are  also 
included, e.g. h
fe
 ,h 
ib
 are h parameters of common emitter and common collector amplifiers  
Using two equations the generalized model of the amplifier can be drawn as shown in  fig. 2. 
 
Fig. 2 
 
 
  
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h-Parameters 
The hybrid model for a transistor amplifier can be derived as follow: 
Let us consider CE configuration as show in fig. 3. The variables, i
B
, i
C
 ,v
C
, and v
B
 represent total 
instantaneous currents and voltages i
B
 and v
C
 can be taken as independent variables and v
B
, I
C
 as 
dependent variables.  
 
Fig. 3 
v
B
 = f
1
 (i
B
 ,v
C
 )  
I
C
 = f
2
 ( i
B
 , v
C
 ).  
Using Taylor 's series expression, and neglecting higher order terms we obtain.  
 
The partial derivatives are taken keeping the collector voltage or base current constant. The  v
B
, 
  v
C
,    i
B
,    i
C
  represent the  small  signal  (incremental)  base  and  collector  current  and  voltage 
and can be represented as v
b
 ,i
b
 ,v
C
 ,i
C
.  
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The model for CE configuration is shown in fig. 4. 
 
Fig. 4 
 
h-Parameters 
Actcivotiov o| q  tooctco:  
To determine the four h-parameters of transister amplifier, input and output characteristic are 
used. Input characteristic depicts the relationship between input voltage and input current with 
output voltage as parameter. The output characteristic depicts the relationship between output 
voltage and output current with input current as parameter. Fig. 5, shows the output 
characterisitcs of CE amplifier.  
 
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Fig. 5  
The current increments are taken around the quiescent point Q which corresponds to i
B
 = I
B
 and 
to the collector voltage V
CE
 = V
C
  
 
The value of h
oe
 at the quiescent operating point is given by the slope of the output characteristic 
at the operating point (i.e. slope of tangent AB). 
 
h
ie
 is the slope of the appropriate input on fig. 6, at the operating point (slope of tangent EF at Q).  
 
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Fig. 6  
A vertical line on the input characteristic represents constant base current. The parameter hre can 
be obtained from the ratio (V
B2
 V 
B1
 ) and (V
C2
 V 
C1
 ) for at Q.  
Typical CE h-parametersof transistor 2N1573 are given below:  
h
ie
 = 1000 ohm. 
h
re
 = 2.5 * 10 4 
h
fe
 = 50 
h
oe
 = 25 m A / V  
 
h-parameters 
Analysis of a transistor amplifier using h-parameters:  
To form a transistor amplifier  it  is only  necessary to connect an external  load and signal  source 
as indicated in fig. 1 and to bias the transistor properly. 
 
Fig. 1 
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Consider  the  two-port  network  of  CE  amplifier.  R
S
  is  the  source  resistance  and  Z
L
  is  the  load 
impedence h-parameters are assumed to be constant over the operating range. The ac equivalent 
circuit  is  shown  in  fig.  2.  (Phasor  notations  are  used  assuming  sinusoidal  voltage  input).  The 
quantities of interest are the current gain, input impedence, voltage gain, and output impedence.  
 
Fig. 2  
Current gain:  
For the transistor amplifier stage, A
i
 is defined as the ratio of output to input currents.  
 
Input Impedence: 
The impedence looking into the amplifier input terminals ( 1,1' ) is the input impedence Z
i
  
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h-parameters 
Voltage gain:  
The ratio of output voltage to input voltage gives the gain of the transistors.  
 
Output Admittance:  
It is defined as  
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A
v
 is the voltage gain for an ideal voltage source (R
v
 = 0).  
Consider input source to be a current source I
S
 in parallel with a resistance R
S
 as shown in fig. 3. 
 
Fig. 3 
In this case, overall current gain A
IS
 is defined as  
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h-parameters 
To  analyze  multistage  amplifier  the  h-parameters  of  the  transistor  used  are  obtained  from 
manufacture  data  sheet.  The  manufacture  data  sheet  usually  provides  h-parameter  in  CE 
configuration. These parameters may be converted into CC and CB values. For example  fig. 4 h
rc
 
in terms of CE parameter can be obtained as follows.  
 
Fig. 4  
For CE transistor configuaration  
V
be
 = h
ie
 I
b
 + h
re
 V
ce
  
I
c
 = h 
fe
 I
b
 + h
oe
 V
ce
  
The circuit can be redrawn like CC transistor configuration as shown in fig. 5.  
V
bc
 = h
ie
 I
b
 + h
rc
 V
ec
  
I
c
 = h
fe
 I
b
 + h
oe
 V
ec
  
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Fig. 5  
 
 
h-parameters 
Example - 1  
For the circuits shown in fig. 1. (CECC configuration) various h-parameters are given  
h 
ie
 = 2K, h
fe
 = 50, h
re
 = 6 * 10 
-4
, h 
oc
= 25 m A / V.  
h
ic
 = 2K, h
fe
 = -51, h
re
 = 1, h
oc
 = 25 m A / V.  
 
Fig. 1  
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The small signal model of the transistor amplifier is shown in fig. 2.  
 
Fig. 2  
In  the  circuit,  the  collector  resistance  of  first  stage  is  shunted  by  the  input  impedence  of  last 
stage. Therefore the analysis  is  started with  last stage. It is convenient; to first compute current 
gain,  input  impedence and  voltage gain. Then output impedence  is  calculated starting  from  first 
stage and moving towards end.  
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The effective source resistance R'
S2
 for the second stage is R
01
 || R
C1
 . Thus R
S2
 = R'
01
 = 4.65K  
 
 
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Frequency response  
 
Overall  current  gain  of  the  amplifier  is  A
i
  and  is 
given by  
 
The  equivalent  circuit  of  the  amplifier  is  shown  in 
fig. 3. From the circuit it is clear that the current i
c1
 is 
divided into two parts. 
Therefore, 
 
and 
 
 
Fig.3 
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Overall voltage gain of the amplifier is given by 
 
 
 
h-parameters 
Simplified common emitter hybrid model:  
In most practical cases it is appropriate to obtain approximate values of A
  V
 , A 
i
 etc rather than 
calculating exact values. How the circuit can be modified without greatly reducing the accuracy. 
Fig. 4 shows the CE amplifier equivalent circuit in terms of h-parameters Since 1 / h
oe
 in parallel 
with  R
L
  is  approximately  equal  to  R
L
  if  1  /  h
oe
  >>  R
L
  then  h
oe
  may  be  neglected.  Under  these 
conditions.  
I
c
 = h
fe
 I
B
 .  
h
re
 v
c
 = h
re
 I
c
 R
L
 = h
re
 h
fe
 I
b
 R
L
 .  
 
Fig. 4  
Since  h 
fe
.h 
re
  ~  0.01,  this  voltage  may  be  neglected  in  comparison  with  h 
ic
  I
b
  drop  across  h 
ie
 
provided R
L
 is not very large. If load resistance R
L
 is small than hoe and h
re
 can be neglected.  
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Output  impedence  seems  to  be  infinite.  When  V
s
  =  0,  and  an  external  voltage  is  applied  at  the 
output we fined I
b
 = 0, I 
C
 = 0. True value depends upon R
S
 and lies between 40 K and 80K.  
On the same lines, the calculations for CC and CB can be done.  
CE amplifier with an emitter resistor:  
The  voltage  gain  of  a  CE  stage  depends  upon  h
fe
.  This  transistor  parameter  depends  upon 
temperature,  aging  and  the  operating  point.  Moreover,  h
fe
  may  vary  widely  from  device  to 
device, even for same type of transistor. To stabilize voltage gain A 
V
 of each stage, it should be 
independent of  h
fe
. A simple  and effective way  is to connect an emitter resistor R
e
 as shown  in 
fig. 5. The resistor provides negative feedback and provide stabilization. 
 
Fig. 5  
An approximate analysis of the circuit can be made using the simplified model.  
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Subject to above approximation A 
V
 is completely stable. The output resistance is infinite for the 
approximate model.  
Opto Coupler:  
It combines a LED and a photo diode in a single package as shown in fig. 6. LED radiates the light depending on the current 
through LED. This light fails on photo diode and this sets up a reverse current. The advantage of an opto coupler is the electrical 
isolation between the input and output circuits. The only contact between the input and output is a beam of light. Because of this, 
it is possible to have an insulation resistance between the two circuits of the order of thousands of mega ohms. They can be  used 
to isolate two circuits of different voltage levels. 
 
Fig. 6  
 
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                       TRANSISTOR BIAS STABILITY 
BJT: Bipolar Junction Transistors: 
Bipolar transistor amplifiers  must be properly  biased to operate correctly. In circuits  made with 
individual  devices  (discrete  circuits),  biasing  networks  consisting  of  resistors  are  commonly 
employed.  Much  more  elaborate  biasing  arrangements  are  used  in  integrated  circuits,  for 
example, bandgap voltage references and current mirrors. 
Bias circuit requirements: 
For analog circuit operation, the Q-point is placed so the transistor stays in active mode (does not 
shift  to  operation  in  the  saturation  region  or  cut-off  region)  when  input  is  applied.  For  digital 
operation, the Q-point is placed so the transistor does the contrary  - switches from "on" to "off" 
state. Often, Q-point is established near the center of active region of transistor characteristic to 
allow  similar  signal  swings  in  positive  and  negative  directions.  Q-point  should  be  stable.  In 
particular, it should be insensitive to variations in transistor parameters (for example, should not 
shift if transistor is replaced by another of the same type), variations in temperature, variations in 
power  supply  voltage  and  so  forth.  The  circuit  must  be  practical:  easily  implemented  and  cost-
effective. 
Load line: 
 The  concept  of  load  line  is  very  important  in  understanding  the  working  of  a  transistor. It  is 
defined as the locus of operating points on the output characteristics of the transistor. It is the line 
on which the operating point moves when ac signal is applied to the transistor. 
 The  dc  load  line  gives  the  value  of  I
c
  and  V
CE
  corresponding  to  zero  signal  conditions. The  ac 
load line gives the value of I
C
 and V
CE
 when ac signal is applied. AC load line is steeper than the 
dc  load  line  but  the  two  intersect  at  the  Q-point  determined  by  biasing  dc  voltages  and 
currents. AC load line takes into account the ac load resistance while dc load line considers only 
the dc load resistance. 
Q Point: 
The  operating  point  of  a  device,  also  known  as  bias  point,  quiescent  point,  or  Q-point,  is  the 
point  on  the  output  characteristics  that  shows  the  DC  collectoremitter  voltage  (Vce)  and  the 
collector current (Ic) with no input signal applied. The term is normally used in connection with 
devices such as transistors. 
For  bipolar  junction  transistors  the  bias  point  is  chosen  to  keep  the  transistor  operating  in  the 
active  mode,  using  a  variety  of  circuit  techniques,  establishing  the  Q-point  DC  voltage  and 
current.  A  small  signal  is  then  applied  on  top  of  the  Q-point  bias  voltage,  thereby  either 
modulating or switching the current, depending on the purpose of the circuit. 
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The  quiescent  point  of  operation  is  typically  near  the  middle  of  DC  load  line.  The  process  of 
obtaining  certain  DC  collector  current  at  a  certain  DC  collector  voltage  by  setting  up  operating 
point is called biasing. 
After establishing the operating point, when input signal is applied, the output signal should not 
move  the  transistor  either  to  saturation  or  to  cut-off.  However,  this  unwanted  shift  still  might 
occur, due to the following reasons: 
1.  Parameters  of  transistors  depend  on  junction  temperature.  As  junction  temperature 
increases,  leakage  current  due  to  minority  charge  carriers  (I
CBO
)  increases.  As  I
CBO
 
increases,  I
CEO
  also  increases,  causing  an  increase  in  collector  current  I
C
.  This  produces 
heat at the collector junction. This process repeats, and, finally, Q-point may shift into the 
saturation region. Sometimes, the excess heat produced at the junction may even burn the 
transistor. This is known as thermal runaway.  
2.  When a transistor is replaced  by another of the same type, the Q-point  may shift, due to 
changes in parameters of the transistor, such as current gain () which varies slightly for 
each unique transistor.  
To avoid a shift of Q-point, bias-stabilization  is  necessary. Various  biasing circuits can  be used 
for this purpose. 
VARIOUS METHODS FOR TRANSISTOR BIASING 
1.  Fixed bias  
2.  Collector-to-base bias  
3.  Voltage divider bias  
4.  Emitter bias  
 
 
 
 
 
 
 
 
 
 
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1)Fixed bias (base bias): 
 
 
 
This form of biasing is also called base bias. In the example image on the right, the single power 
source (for example, a battery) is used for both collector and base of transistor, although separate 
batteries can also be used. 
In the given circuit, 
V
CC
 = I
B
R
B
 + V
be
  
Therefore, 
I
B
 = (V
CC
 - V
be
)/R
B
  
For  a  given  transistor,  V
be
  does  not  vary  significantly  during  use.  As  V
CC
  is  of  fixed  value,  on 
selection of R
B
, the base current I
B
 is fixed. Therefore this type is called fixed bias type of circuit. 
Also for given circuit, 
V
CC
 = I
C
R
C
 + V
ce
  
Therefore, 
V
ce
 = V
CC
 - I
C
R
C
  
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The common-emitter current gain of a transistor is an important parameter in circuit design, and 
is specified on the data sheet for a particular transistor. It is denoted as  on this page.  
Because   I
C
 = I
B
  
we can obtain I
C
 as  well. In this  manner, operating point given as (V
CE
,I
C
) can  be  set  for given 
transistor. 
Merits: 
-  It is simple to shift the operating point anywhere in the active region by merely changing 
the base resistor (R
B
).  
-  A very small number of components are required.  
Demerits: 
-  The  collector  current  does  not  remain  constant  with  variation  in  temperature  or  power 
supply voltage. Therefore the operating point is unstable.  
-  Changes in V
be
 will change I
B
 and thus cause R
E
 to change. This in turn will alter the gain 
of the stage.  
-  When  the  transistor  is  replaced  with  another  one,  considerable  change  in  the  value  of   
can be expected. Due to this change the operating point will shift.  
2)Collector-to-base bias: 
 
 
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This  configuration  employs  negative  feedback  to  prevent  thermal  runaway  and  stabilize  the 
operating point. In this form of biasing, the base resistor RB is connected to the collector instead 
of connecting it to the DC source V
CC
. So any thermal runaway will induce a voltage drop across 
the R
C
 resistor that will throttle the transistor's base current. 
If V
be
 is held constant and temperature increases, then the collector current I
c
 increases. However, 
a larger I
c
 causes the voltage drop across resistor R
c
 to increase, which in turn reduces the voltage 
across the base resistor R
b
. A lower base-resistor voltage drop reduces the base current I
b
, which 
results  in  less  collector  current  I
c
.  Because  an  increase  in  collector  current  with  temperature  is 
opposed, the operating point is kept stable. 
Merits: 
-  Circuit  stabilizes  the  operating  point  against  variations  in  temperature  and    (ie. 
replacement of transistor)  
Demerits: 
-  In this circuit, to keep I
c
 independent of , the following condition must be met:  
which is the case when 
-  As  -value  is  fixed  (and  generally  unknown)  for  a  given  transistor,  this  relation  can  be 
satisfied either by keeping R
c
 fairly large or making R
b
 very low.  
-  If R
c
 is large, a high V
cc
 is necessary, which increases cost as well as precautions 
necessary while handling.  
-  If R
b
 is low, the reverse bias of the collectorbase region is small, which limits the 
range of collector voltage swing that leaves the transistor in active mode.  
-  The  resistor  R
b
  causes  an  AC  feedback,  reducing  the  voltage  gain  of  the  amplifier.  This 
undesirable effect is a trade-off for greater Q-point stability.  
 
 
 
 
 
 
 
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3)Voltage divider bias 
 
The voltage divider is formed using external resistors R
1
 and R
2
. The voltage across R
2
 forward 
biases the emitter junction. By proper selection of resistors R
1
 and R
2
, the operating point of the 
transistor can be made independent of . In this circuit, the voltage divider holds the base voltage 
fixed  independent  of  base  current  provided  the  divider  current  is  large  compared  to  the  base 
current. However, even with a  fixed  base  voltage, collector current varies with temperature (for 
example) so an emitter resistor is added to stabilize the Q-point, similar to the above circuits with 
emitter resistor. 
Merits: 
-  Unlike above circuits, only one dc supply is necessary.  
-  Operating point is almost independent of  variation.  
-  Operating point stabilized against shift in temperature.  
Demerits: 
-  As -value  is  fixed  for a given transistor, this relation can  be satisfied either  by keeping 
R
E
 fairly large, or making R
1
||R
2
 very low.  
-  If  R
E
  is  of  large  value,  high  V
CC
  is  necessary.  This  increases  cost  as  well  as 
precautions necessary while handling.  
-  If R
1
 || R
2
 is low, either R
1
 is low, or R
2
 is low, or both are low. A low R
1
 raises 
V
B
  closer  to  V
C
,  reducing  the  available  swing  in  collector  voltage,  and  limiting 
how  large  R
C
  can  be  made  without  driving  the  transistor  out  of  active  mode.  A 
low R
2
 lowers V
be
, reducing the allowed collector current. Lowering both resistor 
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values draws more current from the power supply and lowers the input resistance 
of the amplifier as seen from the base.  
-  AC  as  well  as  DC  feedback  is  caused  by  R
E
,  which  reduces  the  AC  voltage  gain  of  the 
amplifier.  A  method  to  avoid  AC  feedback  while  retaining  DC  feedback  is  discussed 
below.  
4)Emitter bias: 
 
 
When  a  split  supply  (dual  power  supply)  is  available,  this  biasing  circuit  is  the  most  effective, 
and  provides  zero  bias  voltage  at  the  emitter  or  collector  for  load.  The  negative  supply  V
EE
  is 
used to forward-bias the emitter junction through R
E
. The positive supply V
CC
 is used to reverse-
bias the collector junction. Only two resistors are necessary for the common collector stage and 
four resistors for the common emitter or common base stage. 
We know that, 
V
B
 - V
E
 = V
be
 
If R
B
 is small enough, base voltage will be approximately zero. Therefore emitter current is, 
I
E
 = (V
EE
 - V
be
)/R
E
 
The operating point is independent of  if R
E
 >> R
B
/ 
 
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Merit: 
Good stability of operating point similar to voltage divider bias. 
Demerit: 
This type can only be used when a split (dual) power supply is available. 
Stability Factor: 
The  degree  of  success  achieved  in  stabilizing  I
C
  in  the  face  of  variations  in  I
CO
  is  expressed  in 
terms  of  stability  factor  S  and  it  is  defined  as  the  rate of  change  of  I
C
  w.r.t.  I
CO
,  keeping    and 
V
BE
 constant. 
i.e.       S = dI
c
/dI
co
  at constant  and V
BE
 (or I
B
) 
 From  above  expression  it  is  obvious  that  smaller  is  the  value  of  S,  higher  is  the  stability. It  is 
desirable to have as low stability factor as possible so as to achieve greater thermal stability. The 
ideal value of S is unity (because I
C
 includes I
CO
) but it is never possible to achieve it in practice. 
 Stability Factor in case of CB circuit, 
 S = dI
c
/dI
co
 = d(I
E
 + I
co
)/dI
co
 0+1                  or S = 1 
Stability factor in case of CE circuit 
S = dI
c
/dI
co
 = d[I
 + (1+ ) I
co
]/dI
co
  1 +   taking I
B
 constant. 
Stabilization: 
 It  is  desirable  that  once  selected,  the  operating  (or  Q)  point  should  remain  stable  i.e.  the 
operating point should not shift its position owing to change in temperature etc. Unfortunately it 
is  not  possible  in  practice  unless  special  efforts  are  made  to  achieve  it. The  maintenance  of  the 
operating point stable is called the stabilization.   
 The stabilization of operating point is essential because of  
 a) Temperature dependence of I
C
 
 (b) Individual variations and  
 (c) Thermal runaway. 
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 With  the  increase  in  temperature,  the  collector  leakage  current  I
CO
,  the  current  gain    tend  to 
increase and V
BE
 required to produce a given collector current I
C 
tends to decrease. Thus increase 
in temperature tends to cause increase in I
C
.  
The value of  and V
BE 
are not exactly the same for any two transistors even of the same type. So 
when  a  transistor  is  replaced  by  another  one  (even  of  the  same  type)  the  operating  point  (zero 
signals I
C
 and V
CE
) is shifted. 
The  collector  current  I
C
,  being  equal  to    I
B
  +  (1+    )  I
CO
,  increases  with  the  increase  in 
temperature. This  leads  to  increased  power  dissipation  with  further  increase  in  temperature. 
Being a cumulative process, it can lead to thermal runaway resulting in burn out of the transistor. 
However, if by some modification, I
C
 is made to fall with increase in temperature automatically, 
then  decrease  in  the  term     can  be  made  to  neutralize  the  increase  in  the  term  (1  +  )  I
CO
, 
thereby keeping I
C 
almost constant. This will achieve thermal stability resulting in bias stability. 
The biasing network associated with the transistor should fulfill the requirements of (i) ensuring 
proper zero signal collector current, (ii) ensuring  V
CE
 not falling  below 0.5 V  for Ge transistors 
and  1  V  for  Si  transistors  at  any  instant  and  (iii)  ensuring  stabilization  of  operating  point  (zero 
signal I
C
 and V
CE
) 
Bias Compensation techniques: 
Diode Compensation: 
In the previous section, we looked at how four 
parameters  (VCC,  VBE,  ICBO,  and  )  can 
affect  the  total  collector  current  and, 
therefore, the  Q-point  of  the  amplifier.  Diode 
compensation  is  a  technique  that  is  used  to 
reduce  the  Q-point  variations  by  selecting  a 
diode  that  has  temperature  characteristics 
similar to the transistor. To make sure that the 
diode  and  transistor  have  the  same 
temperature characteristics, we can use a BJT 
with  the  same  specifications  as  the  amplifier 
transistor that is diode-connected. This simply 
involves  shorting  the  collector  to  the  base  as 
shown  in  the  figure  to  the  right  for  an  npn 
BJT (this can also be done with pnp BJTs). As 
a  reminder,  the  diode  symbol  and  the  model 
for  the  forward  biased  silicon  diode  are  also 
shown to the right  remember that the current flows in the direction of the arrow and that, unless 
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an ideal diode is specified, the diode forward resistance and turn-on voltage must be included in 
all calculations.  
 
The  diode  is  connected  in  the  base  circuit  of 
the  amplifier  as  shown  in  Figure  7.9a, 
reproduced  to  the  right.  The  addition  of  the 
diode  in  this  manner  allows  temperature 
compensation  since  the  VON  of  the  diode 
varies  in  the  same  fashion  as  the  VBE  of  the 
transistor.  If  the  transistors  used  in  the 
amplifier  and  to  construct  the  diode  are 
matched,  the  diode  characteristics  and  base-
emitter  junction  characteristics  will  be  the 
same.  Under  these  circumstances,  variations 
in VBE due to changes in bias parameters will 
effectively  be  significantly  reduced  or 
cancelled. 
Sensistor & Thermistor Compensation: 
Sensistor is a resistor whose resistance changes with temperature. 
The resistance increases exponentially with temperature[1], that is the temperature coefficient is 
positive (eg. 0.7% per degree Celsius).[2] 
Sensistors are used in electronic circuits for compensation of temperature influence or as sensors 
of temperature for other circuits.[3] 
Sensistors are  made  by using  semiconducting silicon and  in their operation are similar to  PTC-
type thermistors. 
 
 
 
 
 
 
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  2MARKS 
1.Why do we choose q point at the center of the loadline?  
The operating point of a transistor is kept fixed usually at the center of the active region 
in order that the input signal is well amplified. If the point is fixed in the saturation region or the 
cut off region the positive and negative half cycle gets clipped off respectively.  
 
2. Name the two techniques used in the stability of the q point .explain.  
Stabilization technique: This refers to the use of resistive biasing circuit which 
allows IB to vary so as to keep IC relatively constant with variations in Ico,, and VBE. 
Compensation techniques: This refers to the use of temperature sensitive devices such as 
thermistors diodes. They provide compensating voltages ¤ts to maintain operating 
point constant. 
 
3. List out the different types of biasing.  
1 )  Voltage divider bias 
2 ) Base bias 
3 )  Emitter feed back bias 
4 )  Collector feedback bias 
 
5. What do you meant by thermal runway?  
Due to the self heating at the collector junction, the collector current rises. This 
causes damage to the device. This phenomenon is called thermal runway. 
 
6.  Why is the transistor called a current controlled device? 
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               The output characteristics of the transistor depend on the input current. So the 
transistor is called a current controlled device. 
 
7. Define current amplification factor? 
It is defined as the ratio of change in output current to the change in input current at 
constant other side voltage. 
 
8. What are the requirements for biasing circuits? 
The q point must be taken at the Centre of the active region of the output  
characteristics.  
 
9. When does a transistor act as a switch? 
The transistor acts as a switch when it is operated at either cutoff region or saturation 
region 
 
10. What is biasing? 
To use the transistor in any application it is necessary to provide sufficient voltage  
and current to operate the transistor. This is called biasing.  
 
11. What is operating point?  
For the proper operation of the transistor a fixed level of current and voltages are  
required. This values of currents and voltages defined at a point at which the transistor 
operate is called operating point. 
 
12. What is stability factor? 
Stability factor is defined as the rate of change of collector current with respect to 
the rate of change of reverse saturation current. 
 
13. What is d.c load line? 
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The d.c load line is defined as a line on the output characteristics of the transistor 
which gives the value of Ic & Vce corresponding to zero signal condition. 
 
14. What are the advantages of fixed bias circuit? 
This is simple circuit which uses a few components. The operating point can be 
fixed any where on the Centre of the active region 
 
15. Explain about the various regions in a transistor? 
The three regions are active region saturation region cutoff region.  
 
16. Explain about the characteristics of a transistor?  
Input characteristics: it is drawn between input voltage & input current while keeping  
output voltage as constant.  
Output characteristics: It is drawn between the output voltage &output current while 
keeping input current as constant. 
 
 
 
 
                                                 UNIT III 
                        Field Effect Transistor And Its Applications  
 
Field Effect Transistor:  
The  field  effect  transistor  is  a  semiconductor  device,  which  depends  for  its  operation  on  the 
control of current by an electric field. There are two of field effect transistors:  
1.  JFET (Junction Field Effect Transistor)  
2.  MOSFET (Metal Oxide Semiconductor Field Effect Transistor)  
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The FET has several advantages over conventional transistor.  
1.  In a conventional transistor, the operation depends upon the flow of majority and 
minority carriers. That is why  it  is called  bipolar transistor. In FET the operation 
depends upon the flow of majority carriers only. It is called unipolar device.  
2.  The  input  to  conventional  transistor  amplifier  involves  a  forward  biased  PN 
junction with its inherently low dynamic impedance. The input to FET involves a 
reverse  biased  PN  junction  hence  the  high  input  impedance  of  the  order  of  M-
ohm.  
3.  It is less noisy than a bipolar transistor.  
4.  It exhibits no offset voltage at zero drain current.  
5.  It has thermal stability.  
6.  It is relatively immune to radiation.  
The  main  disadvantage  is  its  relatively  small  gain  bandwidth  product  in  comparison  with 
conventional transistor.  
Operation of FET:  
Consider  a  sample  bar  of  N-type  semiconductor.  This  is  called  N-channel  and  it  is  electrically 
equivalent to a resistance as shown in fig. 1. 
 
Fig. 1  
Ohmic contacts are then added on each side of the channel to bring the external connection. Thus 
if a voltage is applied across the bar, the current flows through the channel.  
The  terminal  from  where  the  majority  carriers  (electrons)  enter  the  channel  is  called  source 
designated by S. The terminal through which majority carriers leaves the channel is called drain 
and  designated  by  D.  For  an  N-channel  device,  electrons  are  the  majority  carriers.  Hence  the 
circuit behaves like a dc voltage V
DS
 applied across a resistance R
DS
. The resulting current is the 
drain current I
D
. If V
DS
 increases, I
D
 increases proportionally. 
Now on both sides of the n-type bar heavily doped regions of p-type impurity have been formed 
by any method for creating pn junction. These impurity regions are called gates (gate1 and gate2) 
as shown in fig. 2. 
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Both the gates are internally connected and they 
are  grounded  yielding  zero  gate  source  voltage 
(V
GS
  =0).  The  word  gate  is  used  because  the 
potential  applied  between  gate  and  source 
controls  the  channel  width  and  hence  the 
current.  
As  with  all  PN  junctions,  a  depletion  region  is 
formed  on  the  two  sides  of  the  reverse  biased 
PN  junction.  The  current  carriers  have  diffused 
across  the  junction,  leaving  only  uncovered 
positive  ions on the  n side and  negative  ions on 
the p side. The depletion region width  increases 
with  the  magnitude  of  reverse  bias.  The 
conductivity  of  this  channel  is  normally  zero 
because of the unavailability of current carriers.  
The  potential  at  any  point  along  the  channel 
depends  on  the  distance  of  that  point  from  the 
drain,  points  close  to  the  drain  are  at  a  higher 
positive potential, relative to ground, then points 
close  to  the  source.  Both  depletion  regions  are 
therefore  subject  to  greater  reverse  voltage  near 
the  drain.  Therefore  the  depletion  region  width 
increases as we move towards drain. The flow of 
electrons  from  source  to  drain  is  now  restricted 
to  the  narrow  channel  between  the  no 
conducting  depletion  regions.  The  width  of  this 
channel determines the resistance  between drain 
and source.  
 
Fig. 2  
 
 
Field Effect Transistor  
Consider  now  the  behavior  of  drain  current  I
D
  vs  drain  source  voltage  V
DS
.  The  gate  source 
voltage  is zero therefore V
GS
= 0. Suppose that V
DS
  is gradually  linearly  increased  linearly  from 
0V. I
D
 also increases.  
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Since  the  channel  behaves  as  a  semiconductor 
resistance, therefore it follows ohm's law. The region 
is  called  ohmic  region,  with  increasing  current,  the 
ohmic  voltage  drop  between  the  source  and  the 
channel  region  reverse  biased  the  junction,  the 
conducting portion of the channel begins to constrict 
and  I
D
  begins  to  level  off  until  a  specific  value  of 
V
DS
 is reached, called the pinch of voltage V
P
.  
At  this  point  further  increase  in  V
DS
  do  not  produce 
corresponding  increase  in  I
D
.  Instead,  as  V
DS
 
increases,  both  depletion  regions  extend  further  into 
the channel, resulting in a no more cross section, and 
hence a higher channel resistance. Thus even though, 
there  is  more  voltage,  the  resistance  is  also  greater 
and  the  current  remains  relatively  constant.  This  is 
called  pinch  off  or  saturation  region.  The  current  in 
this  region  is  maximum  current  that  FET  can 
produce  and  designated  by  I
DSS
.  (Drain  to  source 
current with gate shorted).  
 
Fig. 3  
As with all pn junctions, when the reverse voltage exceeds a certain level, avalanche breakdown 
of pn junction occurs and I
D
 rises very rapidly as shown in fig. 3. 
Consider now an N-channel JFET with a reverse gate source voltage as shown in fig. 4. 
 
  
Fig. 4  
 
Fig. 5  
The additional reverse bias, pinch off will occur for smaller values of | V
DS 
|, and the maximum 
drain current will  be smaller. A  family of curves  for different values of V
GS
(negative)  is  shown 
in fig. 5. 
Suppose  that  V
GS
=  0  and  that  due  of  V
DS
  at  a  specific  point  along  the  channel  is  +5V  with 
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respect  to  ground.  Therefore  reverse  voltage  across  either  p-n  junction  is  now  5V.  If  V
GS
  is 
decreased from 0 to 1V the net reverse bias near the point is 5  - (-1) = 6V. Thus for any fixed 
value of V
DS
, the channel width decreases as V
GS
 is made more negative.  
Thus I
D
 value changes correspondingly. When the gate voltage is negative enough, the depletion 
layers  touch  each  other  and  the  conducting  channel  pinches  off  (disappears).  In  this  case  the 
drain current is cut off. The gate voltage that produces cut off is symbolized V
GS
(off) . It is same 
as pinch off voltage.  
Since the gate source junction is a reverse biased silicon diode, only a very small reverse current 
flows through it. Ideally gate current is zero. As a result, all the free electrons from the source go 
to  the  drain  i.e.  I
D
  =  I
S
.  Because  the  gate  draws  almost  negligible  reverse  current  the  input 
resistance  is  very  high  10's  or  100's  of  M  ohm.  Therefore  where  high  input  impedance  is 
required,  JFET  is  preferred  over  BJT.  The  disadvantage  is  less  control  over  output  current  i.e. 
FET takes larger changes in input voltage to produce changes in output current. For this reason, 
JFET has less voltage gain than a bipolar amplifier.  
 
 Biasing the Field Effect Transistor  
Transductance Curves:  
The  transductance  curve  of  a  JFET  is  a  graph  of  output  current  (I
D
)  vs  input  voltage  (V
GS
)  as 
shown in fig. 1. 
 
Fig. 1  
By reading the value of I
D
 and V
GS
 for a particular value of V
DS
, the transductance curve can be 
plotted. The transductance curve is a part of parabola. It has an equation of  
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Data sheet provides only I
DSS
 and V
GS
(off) value. Using these values the transductance curve can 
be plotted.  
Biasing the FET:  
The  FET  can  be  biased  as  an  amplifier.  Consider  the  common  source  drain  characteristic  of  a 
JFET. For linear amplification, Q point  must be selected somewhere  in the saturation region. Q 
point  is  selected  on  the  basis  of  ac  performance  i.e.  gain,  frequency  response,  noise,  power, 
current and voltage ratings.  
  Gate Bias:  
Fig. 2, shows a simple gate bias circuit.  
 
Fig. 2  
Separate V
GS
 supply is used to set up Q point. This is the worst way to select Q point. The reason 
is  that  there  is  considerable  variation  between  the  maximum  and  minimum  values  of  FET 
parameters e.g.  
   I
DSS
         V
GS
(off)  
Minimum  4mA  -2V  
Maximum  13mA  -8V  
This implies that the minimum and maximum transductance curves are displaced as shown in fig. 
3. 
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Gate  bias  applies  a  fixed  voltage  to  the  gate. 
This  fixed  voltage  results  in  a  Q  point  that  is 
highly sensitive to the particular JFET used. For 
instance,  if  V
GS
=  -1V  the  Q  point  may  very 
from  Q
1
  to  Q
2
  depending  upon  the  JFET 
parameter is use.  
At Q
1
, I
D
= 0.016 (1 - (1/8))
2
 = 12.3 mA  
At Q
2
, I
D
= 0.004 (1-(1/2))
2
 = 1 mA.  
The variation in drain current is very large.  
 
Fig. 3  
 
 
Biasing the Field Effect Transistor  
Self Bias:  
Fig. 4, shows a self bias circuit another way to bias a FET. 
Only a drain supply is used and no gate supply. The idea 
is to use the voltage across R
S
 to produce the gate source 
reverse voltage.  
This  is  a  form  of  a  local  feedback  similar  to  that  used 
with  bipolar  transistors.  If  drain  current  increases,  the 
voltage  drop  across  R
S
  increases  because  the  I
D
  R
S
 
increases.  This  increases  the  gate  source  reverse  voltage 
which  makes  the  channel  narrow  and  reduces  the  drain 
current.  The  overall  effect  is  to  partially  offset  the 
original  increase  in  drain  current.  Similarly,  if  I
D
 
decreases,  drop  across  R
S
  decreases,  hence  reverse  bias 
decreases and I
D
 increases.  
 
Fig. 4  
Since the gate source junction is reverse biased, negligible gate current flows through R
G
 and so 
the gate voltage with respect to ground is zero.    
 V
G
= 0;  
The source to ground voltage equals the product of the drain current and the source resistance.  
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\ V
S
= I
D
 R 
S
.  
The gate source voltage is the difference between the gate voltage and the source voltage.  
V
GS
 = V
G
  V
S
 = 0  I
D
R
S
  
V
GS
 = -I
D
 R
S
.  
This  means  that  the  gate  source  voltage  equals  the  negative  of  the  voltage  across  the  source 
resistor. The greater the drain current, the more negative the gate source voltage becomes.  
Rearranging the equation:      
 I
D
 = -V
GS
 / R
S
  
The graph of this equation is called self base line a shown in Fig. 5. 
 
Fig. 5  
 
 
 
 
 
 
Biasing the Field Effect Transistor  
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The  operating  point  on  transductance  curve  is  the 
intersection  of  self  bias  line  and  transductance  curve. 
The slope of the line is (-1 / R
S
). If the source resistance 
is  very  large  (-1  /  R
S
  is  small)  then  Q-point  is  far  down 
the  transductance  curve  and  the  drain  current  is  small. 
When R
S
 is small, the Q point is far up the transductance 
curve  and  the  drain  current  is  large.  In  between  there  is 
an  optimum  value  of  R
S
  that  sets  up  a  Q  point  near  the 
middle of the transductance curve.  
The transductance curve varies widely  for FET (because 
of variation in I
DSS
 and V
GS
(off)) as shown in fig. 6. The 
actual curve may be in between there extremes. A and B 
are  the  optimum  points  for  the  two  extreme  curves.  To 
find the optimum resistance R
S
, so that Q-point is correct 
for all the curves,  A and  B points are  joined  such that it 
passes through origin.  
The slope of this  line gives the resistance  value R
S
( V
GS
 
= -I
D
 R
S
). The current I
Q
 is such that I
A
 > I
Q
 > I
B
. Here A, 
Q and B all points are in straight line.  
 
                           Fig. 6  
Consider the case where a line drawn to pass between points A and B does not pass through the 
origin. The equation V
GS
 = - I
D
 R
S
 is not valid. The equation of this line is V
GS
 = V
GG
  I
D
 R
S
.  
Such  a  bias  relationship  may  be  obtained  by  adding  a  fixed  bias  to  the  gate  in  addition  to  the 
source self bias as shown in fig. 7. 
 
Fig. 7  
In this circuit.  
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V
GG
 = R
S
 I
G
 + V
GS
 + I
D
 R
S
  
Since R
S
 I
G
 = 0;  
        V
GG
 = V
GS
 + I
D
 R
S
  
or     V
GS
 = V
GG
 I
D
 R
S
  
 
 
Biasing the Field Effect Transistor  
Voltage Divider Bias :  
The biasing circuit based on single power supply is shown in fig. 1. This is similar to the voltage 
divider bias used with a bipolar transistor.  
 
Fig. 1  
The Thevenin voltage V
TH
 applied to the gate is  
 
The Thevenin resistance is given as 
 
The gate current is assumed to be negligible. V
TH
 is the dc voltage from gate to ground.  
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The drain current ID is given by 
 
and the dc voltage from the drain to ground is V
D
 = V
DD
  I
D
 R
D
.  
If  V
TH
  is  large  enough  to  swamp  out  V
GS
  the  drain  current  is  approximately  constant  for  any 
JFET as shown in fig. 2. 
 
Fig. 2  
There  is  a  problem  in  JFET.  In  a  BJT,  V
BE
  is  approximately  0.7V,  with  only  minor  variations 
from one transistor to other. In a FET, V
GS
 can vary several volts from one JFET to another. It is 
therefore, difficult to make V
TH
 large enough to swamp out V
GS
. For this reason, voltage divider 
bias is less effective with, FET than BJT. Therefore, V
GS
 is not negligible. The current increases 
slightly from Q2 to Q1. However, voltage divider bias maintains I
D
 nearly constant.  
Consider a voltage divider bias circuit shown in fig. 3. 
 
Difference in I
D (min
) and I
D (max)
 is less  
V
D (max)
 = 30  2.13 * 4.7 = 20 V  
V
D (min)
 = 30  2.67 * 4.7 = 17.5 V  
 
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Fig. 3  
 
 Biasing the Field Effect Transistor  
Current Source Bias:  
This  is  another  way  to  produce  solid  Q  point.  The  aim  is  to  produce  a  drain  current  that  is 
independent  of  V
GS
.  Voltage  divider  bias  and  self  bias  attempt  to  do  this  by  swamping  out  of 
variations in V
GS
.  
Using two power supplies:  
The current source bias can be used to make I
D
 constant fig. 4. 
 
Fig. 4  
The bipolar transistor is emitter biased; its collector current is given by  
I
C
 = (V
EE
  V
BE
 ) / R
E
.  
Because  the  bipolar  transistor  acts  like  a  current source,  it  forces  the  drain  current  to  equal  the 
bipolar collector current.  
I
D
 = I
C
  
Since  I
C
  is  constant,  both  Q  points  have  the  same  value  of  drain  current.  The  current  source 
effectively  wipes  out  the  influence  of  V
GS
.  Although  V
GS
  is  different  for  each  Q  point,  it  no 
longer influences the value of drain current.  
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Using One power supply:  
When  only  a  positive  supply  is  available,  the  circuit 
shown  in  fig.  5,  can  be  used  to  set  up  a  constant  drain 
current. 
In  this  case,  the  bipolar  transistor  is  voltage  divider 
biased. Assuming a stiff voltage divider, the emitter and 
collector currents are constant for all bipolar transistors. 
This  forces  the  FET  drain  current  equal  the  bipolar 
collector current.  
 
 
Fig. 5  
 
 
Biasing the Field Effect Transistor  
Transductance: 
The transductance of a FET is defined as  
 
Because  the  changes  in  I
D
  and  V
GS
  are  equivalent 
to  ac  current  and  voltage.  This  equation  can  be 
written as  
 
The unit of g
m
 is mho or siemems.  
Typical value of g
m
 is 2000 m A / V.  
 
Fig. 6  
The value of g
m
 can be obtained from the transductance curve as shown in fig. 6. 
If A and B points are considered, than a change in V
GS
 produces a change in I
D
. The ratio of I
D
 
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and V
GS
 is the value of g
m
 between A and B points. If C and D points are considered, then same 
change in V
GS
 produces more change in I
D
. Therefore, g
m
 value is higher. In a nutshell, g
m
 tells 
us  how  much  control  gate  voltage  has  over  drain  current.  Higher  the  value  of  g
m
,  the  more 
effective  is  gate  voltage  in  controlling  gate  current.  The  second  parameter  r
d
  is  the  drain 
resistance.  
 
 
 
FET a amplifier 
Similar to Bipolar  junction transistor. JFET can also be used as an amplifier. The ac equivalent 
circuit of a JFET is shown in fig. 1. 
 
Fig. 1  
The resistance between the gate and the source R
GS
 is very high. The drain of a JFET acts like a 
current source with a value of g
m
 V
gs
. This model is applicable at low frequencies.  
From the ac equivalent model  
 
 
The amplification factor  for FET is defined as 
 
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When V
GS
 = 0, g
m
 has its maximum value. The maximum value is designated as g
mo.
 
Again consider the equation, 
 
 
 
As V
GS
 increases, gm decreases linearly. 
 
Measuring I
DSS
 and g
m
, V
GS(off)
 can be determined  
 
 
FET as amplifier 
 
Fig. 2, shows a common source amplifier.  
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Fig. 2  
When a small ac signal is coupled into the gate it produces variations in gate source voltage. This 
produces  a  sinusoidal  drain  current.  Since  an  ac  current  flows  through  the  drain  resistor.  An 
amplified ac voltage is obtained at the output. An increase in gate source voltage produces more 
drain current, which  means that the drain  voltage  is decreasing. Since the positive  half cycle of 
input voltage produces the negative half cycle of output voltage, we get phase inversion in a CS 
amplifier. 
The ac equivalent circuit is shown in fig. 3. 
  
 
Fig. 3 
The ac output voltage is  
v
out
 = - g
m
 v 
gS
 R
D
  
Negative  sign  means  phase  inversion.  Because  the  ac  source  is  directly  connected  between  the 
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gate source terminals therefore ac input voltage equals  
V
in
 = V
gs
  
The voltage gain is given by  
 
The further simplified model of the amplifieris shown in fig. 4. 
 
Fig. 4  
Z
in
 is the input impedance. At low frequencies, this is parallel combination of R
1
|| R
2
|| R
GS
. Since 
R
GS
  is  very  large,  it  is  parallel  combination  of  R
1
  &  R
2
.  A  V
in
  is  output  voltage  and  R
D
  is  the 
output impedance.  
 
 
FET as amplifier  
Because of nonlinear transductance curve, a JFET distorts large signals, as shown in fig. 5. 
Given  a  sinusoidal  input  voltage,  we  get  a  non-sinusoidal  output  current  in  which  positive  half 
cycle is elongated and negative cycle is compressed. This type of distortion is called Square law 
distortion because the transductance curve is parabolic.  
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Fig. 5   Fig. 6  
This  distortion  is  undesirable  for  an  amplifier.  One  way  to  minimize  this  is  to  keep  the  signal 
small. In that case a part of the curve is used and operation is approximately linear. Some times 
swamping resistor is used to minimize distortion and gain constant. Now the source is no longer 
ac ground as shown in fig. 6. 
The drain current through r
S
 produces an ac voltage between the source and ground. If r
S
 is large 
enough the  local  feedback can  swamp out the non-linearity of the curve. Then the  voltage gain 
approaches an ideal value of R
D
 / r
S
.  
Since  R
GS
  approaches  infinity  therefore,  all  the  drain  current  flows  through  r
S
  producing  a 
voltage drop of g
m
 V
gS
 r
S
. The ac equivalent circuit is shown in fig. 7. 
 
Fig. 7  
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The  voltage  gain  reduces  but  voltage  gain  is  less  effective  by  change  in  g
m
.  r
S
  must  be  greater 
than 1 / g
m
 only then  
 
 
JFET Applications 
Example-1:  
Determine gm for an n-channel JFET with characteristic curve shown in fig. 1. 
 
Fig. 1 
Solution:  
We  select  an  operating  region  which  is  approximately  in  the  middle  of  the  curves;  that  is, 
between  v
GS
  =  -0.8  V  and  v
GS
  =  -1.2  V;  i
D
  =  8.5mA  and  i
D
  =  5.5  mA.  Therefore,  the 
transductance of the JFET is given by  
 
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Design of JFET amplifier:  
To  design  a  JFET  amplifier,  the  Q  point  for the  dc  bias  current  can  be  determined  graphically. 
The dc  bias current at the Q point should  lie  between 30% and 70% of I
DSS
. This  locates the Q 
point in the linear region of the characteristic curves.  
The relationship between i
D
 and v
GS
 can be plotted on a dimensionless graph (i.e., a normalized 
curve) as shown in fig. 2 . 
 
Fig. 2  
The  vertical  axis  of  this  graph  is  i
D
  /  I
DSS
  and  the  horizontal  axis  is  v
GS
  /  V
P
.  The  slope  of  the 
curve is g
m
.  
A  reasonable  procedure  for  locating  the  quiescent  point  near  the  center  of  the  linear  operating 
region  is  to  select  I
DQ
    I
DSS
  /  2  and  V
GSQ
    0.3V
P
.  Note  that  this  is  near  the  midpoint  of  the 
curve.  Next  we  select  v
DS
    V
DD
  /  2.  This  gives  a  wide  range  of  values  for  v
ds
  that  keep  the 
transistor in the pinch off mode.  
The transductance at the Q-point can  be  found  from the slope of the curve of  fig.2 and  is given 
by  
 
Example-2  
Determine g m for a JFET where I
DSS
 = 7 mA, V
P
 = -3.5 V and V
DD
 = 15V. Choose a reasonable 
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location for the Q-point.  
Solution:  
Let us select the Q-point as given below:  
 
The  transconductance,  g
m
,  is  found  from  the  slope  of  the  curve  at the  point   i
D
  /  I
DSS
  =  0.5  and 
v
GS
 / V
P
 =0.3. Hence,  
 
 
 
JFET Applications 
JEFT as Analog Switch:  
JFET can  be used  as an analog switch as shown  in  fig.  3. It is the  major application of a JFET. 
The idea is to use two points on the load line: cut off and saturation. When JFET is cut off, it is 
like an open switch. When it is saturated, it is like a closed switch.  
 
 
Fig. 3   Fig. 4  
When V
GS
 =0, the JFET is saturated and operates at the upper end of the load line. When V
GS
 is 
equal to or more negative than V
GS
(off) ,  it is cut off and operates at lower end of the  load  line 
(open and closed switch).This is shown in fig. 4.  
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Only  these  two  points  are  used  for  operation  when  used  as  a  switch.  The  JFET  is  normally 
saturated  well  below  the  knee  of  the  drain  curve.  For  this  reason  the  drain  current  is  much 
smaller than I
DSS
 .  
FET as a Shunt Switch:  
FET can be used as a shunt switch as shown in fig. 5. When V
cont
=0, the JFT is saturated and the 
switch is closed When V
cont
 is more negative FET is like an open switch. The equivalent circuit 
is also shown in fig. 5. 
 
Fig. 5  
FET as a series switch:  
JFET  can  also  be  used  as  series  switch  as  shown  in  fig.  6.  When  control  is  zero,  the  FET  is  a 
closed switch. When V
con
= negative, the FET is an open switch. It is better than shunt switch.  
 
Fig. 6 
Multiplexing:  
One of the important application of FET is in analog multiplexer. Analog multiplexer is a  circuit 
that selects one of the output lines as  shown  in  fig.  7. When control voltages are  more  negative 
all  switches  are  open  and  output  is  zero.  When  any  control  voltage  becomes  zero  the  input  is 
transmitted to the output.  
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Fig. 7  
 
Circuit symbols 
A  variety  of  symbols  are  used  for  the  MOSFET.  The  basic  design  is  generally  a  line  for  the 
channel with the source and drain leaving it at right angles and then bending back at right angles 
into the same direction as the channel. Sometimes three line segments are used for enhancement 
mode and a solid  line  for depletion  mode.  Another  line  is drawn parallel to the channel  for the 
gate. 
The  bulk  connection,  if  shown,  is  shown  connected  to  the  back  of  the  channel  with  an  arrow 
indicating  PMOS  or  NMOS.  Arrows  always  point  from  P  to  N,  so  an  NMOS  (N-channel  in  P-
well  or  P-substrate)  has  the  arrow  pointing  in  (from  the  bulk  to  the  channel).  If  the  bulk  is 
connected to the source (as is generally the case with discrete devices) it is sometimes angled to 
meet up with the source leaving the transistor. If the bulk is not shown (as is often the case in IC 
design  as  they  are  generally  common  bulk)  an  inversion  symbol  is  sometimes  used  to  indicate 
PMOS,  alternatively  an  arrow  on  the  source  may  be  used  in  the  same  way  as  for  bipolar 
transistors (out for nMOS, in for pMOS). 
Comparison  of  enhancement-mode  and  depletion-mode  MOSFET  symbols,  along  with  JFET 
symbols  (drawn  with  source  and  drain  ordered  such  that  higher  voltages  appear  higher  on  the 
page than lower voltages): 
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P-channel 
         
N-channel 
JFET  MOSFET enh  MOSFET enh (no bulk)  MOSFET dep 
 
For  the  symbols  in  which  the  bulk,  or  body,  terminal  is  shown,  it  is  here  shown  internally 
connected  to  the  source.  This  is  a  typical  configuration,  but  by  no  means  the  only  important 
configuration. In general, the MOSFET is a four-terminal device, and in integrated circuits many 
of the MOSFETs share a  body connection,  not necessarily connected to the source terminals of 
all the transistors. 
MOSFET operation 
 
 
Example application of an N-Channel MOSFET. When the switch is pushed the LED lights up.
[2]
 
 
 
Metaloxidesemiconductor structure on P-type silicon 
Metaloxidesemiconductor structure 
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A  traditional  metaloxidesemiconductor  (MOS)  structure  is  obtained  by  growing  a  layer  of 
silicon  dioxide  (SiO
2
)  on  top  of  a  silicon  substrate  and  depositing  a  layer  of  metal  or 
polycrystalline  silicon  (the  latter  is  commonly  used).  As  the  silicon  dioxide  is  a  dielectric 
material, its structure is equivalent to a planar capacitor, with one of the electrodes replaced by a 
semiconductor. 
When a  voltage is applied across a MOS structure, it modifies the distribution of charges  in the 
semiconductor.  If  we  consider  a  P-type  semiconductor  (with  N
A
  the  density  of  acceptors,  p the 
density of holes; p = N
A
 in neutral bulk), a positive voltage, V
GB
, from gate to body (see figure) 
creates  a  depletion  layer  by  forcing  the  positively  charged  holes  away  from  the  gate-
insulator/semiconductor interface,  leaving exposed a carrier-free region of  immobile, negatively 
charged acceptor ions (see doping (semiconductor)). If V
GB
 is high enough, a high concentration 
of  negative  charge  carriers  forms  in  an  inversion  layer  located  in  a  thin  layer  next  to  the 
interface between the semiconductor and the insulator. Unlike the MOSFET, where the inversion 
layer electrons are supplied rapidly from the source/drain electrodes, in the MOS capacitor they 
are  produced  much  more  slowly  by  thermal  generation  through  carrier  generation  and 
recombination  centers  in  the  depletion  region.  Conventionally,  the  gate  voltage  at  which  the 
volume density of electrons  in the  inversion  layer  is the same as the volume density of holes  in 
the body is called the threshold voltage. 
This structure with P-type body is the basis of the N-type MOSFET, which requires the addition 
of an N-type source and drain regions. 
MOSFET structure and channel formation 
 
 
Cross section of an NMOS without channel formed: OFF state 
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Cross section of an NMOS with channel formed: ON state 
A  metaloxidesemiconductor  field-effect  transistor  (MOSFET)  is  based  on  the  modulation  of 
charge  concentration  by  a  MOS  capacitance  between  a  body  electrode  and  a  gate  electrode 
located  above  the  body  and  insulated  from  all  other  device  regions  by  a  gate  dielectric  layer 
which in the case of a MOSFET is an oxide, such as silicon dioxide. If dielectrics other than an 
oxide  such  as  silicon  dioxide  (often  referred  to  as  oxide)  are  employed  the  device  may  be 
referred to as a metalinsulatorsemiconductor FET (MISFET). Compared to the MOS capacitor, 
the MOSFET includes two additional terminals (source and drain), each connected to individual 
highly  doped  regions  that  are  separated  by  the  body  region.  These  regions  can  be  either  p  or  n 
type, but they must both be of the same type, and of opposite type to the body region. The source 
and drain (unlike the body) are highly doped as signified by a '+' sign after the type of doping. 
If the MOSFET is an n-channel or nMOS FET, then the source and drain are 'n+' regions and the 
body  is  a  'p'  region.  As  described  above,  with  sufficient  gate  voltage,  holes  from  the  body  are 
driven away from the gate, forming an inversion layer or n-channel at the interface between the p 
region  and  the  oxide.  This  conducting  channel  extends  between  the  source  and  the  drain,  and 
current is conducted through it when a voltage is applied between source and drain. 
For  gate  voltages  below  the  threshold  value,  the  channel  is  lightly  populated,  and  only  a  very 
small subthreshold leakage current can flow between the source and the drain. 
If the MOSFET is a p-channel or pMOS FET, then the source and drain are 'p+' regions and the 
body  is  a  'n'  region.  When  a  negative  gate-source  voltage  (positive  source-gate)  is  applied,  it 
creates  a  p-channel  at  the  surface  of  the  n  region,  analogous  to  the  n-channel  case,  but  with 
opposite  polarities  of  charges  and  voltages.  When  a  voltage  less  negative  than  the  threshold 
value  (a  negative  voltage  for  p-channel)  is  applied  between  gate  and  source,  the  channel 
disappears and only a very small subthreshold current can flow between the source and the drain. 
The  source  is  so  named  because  it  is  the  source  of  the  charge  carriers  (electrons  for  n-channel, 
holes  for  p-channel)  that  flow  through  the  channel;  similarly,  the  drain  is  where  the  charge 
carriers leave the channel. 
The device may comprise a Silicon On Insulator (SOI) device in which a Buried OXide (BOX) is 
formed below a thin semiconductor layer. If the channel region between the gate dielectric and a 
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Buried Oxide (BOX) region  is  very thin, the  very thin channel region  is referred to as an Ultra 
Thin  Channel  (UTC)  region  with  the  source  and  drain  regions  formed  on  either  side  thereof  in 
and/or  above  the  thin  semiconductor  layer.  Alternatively,  the  device  may  comprise  a 
SEMiconductor  On  Insulator  (SEMOI)  device  in  which  semiconductors  other  than  silicon  are 
employed. Many alternative semicondutor materials may be employed. 
When  the  source  and  drain  regions  are  formed  above  the  channel  in  whole  or  in  part, they  are 
referred to as Raised Source/Drain (RSD) regions. 
Modes of operation 
The  operation  of  a  MOSFET  can  be  separated  into  three  different  modes,  depending  on  the 
voltages at the terminals. In the following discussion, a simplified algebraic model is used that is 
accurate only for old technology. Modern MOSFET characteristics require computer models that 
have rather more complex behavior. 
For an enhancement-mode, n-channel MOSFET, the three operational modes are: 
Cutoff, subthreshold, or weak-inversion mode 
When V
GS
 <V
th
:  
where V
th
 is the threshold voltage of the device. 
According  to  the  basic  threshold  model,  the  transistor  is  turned  off,  and  there  is  no 
conduction  between  drain  and  source.  In  reality,  the  Boltzmann  distribution  of  electron 
energies  allows  some  of  the  more  energetic  electrons  at  the  source  to  enter  the  channel 
and flow to the drain, resulting in a subthreshold current that is an exponential function of 
gatesource  voltage.  While  the  current  between  drain  and  source  should  ideally  be  zero 
when the transistor is being used as a turned-off switch, there is a weak-inversion current, 
sometimes called subthreshold leakage. 
In weak  inversion the current varies exponentially with gate-to-source bias  V
GS
 as given 
approximately by:
[3][4]
 
, 
where I
D0
 = current at V
GS
 = V
th
 and the slope factor n is given by 
n = 1 + C
D
 / C
OX
, 
with C
D
 = capacitance of the depletion layer and C
OX
 = capacitance of the oxide layer. In 
a  long-channel device, there  is  no drain  voltage dependence of the current once  V
DS
 > > 
V
T
,  but  as  channel  length  is  reduced  drain-induced  barrier  lowering  introduces  drain 
voltage  dependence  that  depends  in  a  complex  way  upon  the  device  geometry  (for 
example,  the  channel  doping,  the  junction  doping  and  so  on).  Frequently,  threshold 
voltage  V
th
  for  this  mode  is  defined  as  the  gate  voltage  at  which  a  selected  value  of 
current I
D0
 occurs, for example, I
D0
 = 1 A, which may not be the same V
th
-value used in 
the equations for the following modes. 
Some  micropower  analog  circuits  are  designed  to  take  advantage  of  subthreshold 
conduction.
[5][6][7]
  By  working  in  the  weak-inversion  region,  the  MOSFETs  in  these 
circuits deliver the highest possible transconductance-to-current ratio, namely: g
m
 / I
D
 = 1 
/ (nV
T
), almost that of a bipolar transistor.
[8]
 
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The subthreshold  IV  curve depends exponentially upon threshold voltage,  introducing  a 
strong  dependence  on  any  manufacturing  variation  that  affects  threshold  voltage;  for 
example:  variations  in  oxide  thickness,  junction  depth,  or  body  doping  that  change  the 
degree  of  drain-induced  barrier  lowering.  The  resulting  sensitivity  to  fabricational 
variations complicates optimization for leakage and performance.
[9][10]
 
 
 
MOSFET drain current vs. drain-to-source voltage for several values of  V
GS
  V
th
; the boundary 
between  linear  (Ohmic)  and  saturation  (active)  modes  is  indicated  by  the  upward  curving 
parabola. 
 
 
Cross  section  of  a  MOSFET  operating  in  the  linear  (Ohmic)  region;  strong  inversion  region 
present even near drain 
 
 
Cross section of a MOSFET operating  in the saturation (active) region; channel exhibits  pinch-
off near drain 
Triode mode or linear region (also known as the ohmic mode
[11][12]
) 
When V
GS
 >V
th
 and V
DS
 <( V
GS
 - V
th
 ) 
The transistor is turned on, and a channel  has been created which allows current to flow 
between the drain and the source. The MOSFET operates like a resistor, controlled by the 
gate  voltage  relative  to  both  the  source  and  drain  voltages.  The  current  from  drain  to 
source is modeled as: 
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where 
n
 is the charge-carrier effective mobility, W is the gate width, L is the gate length 
and  C
ox
  is  the  gate  oxide  capacitance  per  unit  area.  The  transition  from  the  exponential 
subthreshold region to the triode region is not as sharp as the equations suggest. 
Saturation or active mode
[13][14]
 
When V
GS
 >V
th
 and V
DS
 >( V
GS
 - V
th
 ) 
The  switch  is  turned  on,  and  a  channel  has  been  created,  which  allows  current  to  flow 
between the drain and source. Since the drain voltage is higher than the gate voltage, the 
electrons  spread  out,  and  conduction  is  not  through  a  narrow  channel  but  through  a 
broader, two- or three-dimensional current distribution extending away from the interface 
and  deeper  in  the  substrate.  The  onset  of  this  region  is  also  known  as  pinch-off  to 
indicate  the  lack  of  channel  region  near  the  drain.  The  drain  current  is  now  weakly 
dependent  upon  drain  voltage  and  controlled  primarily  by  the  gatesource  voltage,  and 
modeled very approximately as: 
      
The  additional  factor  involving  ,  the  channel-length  modulation  parameter,  models 
current  dependence  on  drain  voltage  due  to  the  Early  effect,  or  channel  length 
modulation.  According  to  this  equation,  a  key  design  parameter,  the  MOSFET 
transconductance is:  
, 
where  the  combination  V
ov
  =  V
GS
  -  V
th
  is  called  the  overdrive  voltage.
[15]
  Another  key 
design parameter is the MOSFET output resistance r
O
 given by:  
. 
r
out
  is  the  inverse  of  g
ds
  where  .  V
DS
  is  the  expression  in  saturation 
region. 
If    is  taken  as  zero,  an  infinite  output  resistance  of  the  device  results  that  leads  to 
unrealistic circuit predictions, particularly in analog circuits. 
As the channel length becomes very short, these equations become quite inaccurate. New 
physical  effects  arise.  For  example,  carrier  transport  in  the  active  mode  may  become 
limited  by  velocity  saturation.  When  velocity  saturation  dominates,  the  saturation  drain 
current  is  more  nearly  linear  than  quadratic  in  V
GS
.  At  even  shorter  lengths,  carriers 
transport  with  near  zero  scattering,  known  as  quasi-ballistic  transport.  In  addition,  the 
output current is affected by drain-induced barrier lowering of the threshold voltage. 
 
 
 
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Darlington transistor 
 
Circuit diagram of a Darlington pair using NPN transistors 
In  electronics,  the  Darlington  transistor  (often  called  a  Darlington  pair)  is  a  compound 
structure consisting of two  bipolar transistors (either  integrated or separated devices) connected 
in such a way that the current amplified by the first transistor is amplified further by the second 
one.'.'
[1]
  This  configuration  gives  a  much  higher  current  gain  (written  ,  h
fe
,  or  h
FE
)  than  each 
transistor  taken  separately  and,  in  the  case  of  integrated  devices,  can  take  less  space  than  two 
individual transistors because they can use a  shared collector. Integrated Darlington pairs come 
packaged  singly  in  transistor-like  packages  or  as  an  array  of  devices  (usually  eight)  in  an 
integrated circuit. 
The  Darlington  configuration  was  invented  by  Bell  Laboratories  engineer  Sidney  Darlington  in 
1953.  He  patented  the  idea  of  having  two  or  three  transistors  on  a  single  chip,  sharing  a 
collector.
[2]
 
A similar configuration but with transistors of opposite type (NPN and PNP) is the Sziklai pair, 
sometimes called the "complementary Darlington." 
Behaviour 
A  Darlington  pair  behaves  like  a  single  transistor  with  a  high  current  gain  (approximately  the 
product of the gains of the two transistors). In fact, integrated devices have three leads (B, C and 
E), broadly equivalent to those of a standard transistor. 
A general relation between the compound current gain and the individual gains is given by: 
 
If 
1
 and 
2
 are high enough (hundreds), this relation can be approximated with: 
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A typical modern device has a current gain of 1000 or more, so that only a small base current is 
needed  to  make  the  pair  switch  on.  However,  this  high  current  gain  comes  with  several 
drawbacks. 
One drawback is an approximate doubling of base-emitter voltage. Since there are two junctions 
between the base and emitter of the Darlington transistor, the equivalent base-emitter voltage  is 
the sum of both base-emitter voltages: 
 
For  silicon-based  technology,  where  each  V
BEi
  is  about  0.65  V  when  the  device  is  operating  in 
the active or saturated region, the necessary base-emitter voltage of the pair is 1.3 V. 
Another drawback of the Darlington pair is its increased saturation voltage. The output transistor 
is not allowed to saturate (i.e. its base-collector junction must remain reverse-biased) because its 
collector-emitter  voltage  is  now  equal  to  the  sum  of  its  own  base-emitter  voltage  and  the 
collector-emitter  voltage  of  the  first  transistor,  both  positive  quantities  in  normal  operation.  (In 
symbols,  V
CE2
  =  V
BE2
  +  V
CE1
,  so  V
C2
  >  V
B2
  always.)  Thus  the  saturation  voltage  of  a 
Darlington  transistor  is  one  V
BE
  (about  0.65  V  in  silicon)  higher  than  a  single  transistor 
saturation  voltage,  which  is  typically  0.1  -  0.2  V  in  silicon.  For  equal  collector  currents,  this 
drawback  translates  to  an  increase  in  the  dissipated  power  for  the  Darlington  transistor  over  a 
single transistor. 
Another  problem  is  a  reduction  in  switching  speed,  because  the  first  transistor  cannot  actively 
inhibit the base current of the second one, making the device slow to switch off. To alleviate this, 
the second transistor often has a resistor of a few hundred ohms connected between its base and 
emitter  terminals.
[1]
  This  resistor  provides  a  low  impedance  discharge  path  for  the  charge 
accumulated on the base-emitter junction, allowing a faster transistor turn-off. 
The  Darlington  pair  has  more  phase  shift  at  high  frequencies  than  a  single  transistor  and  hence 
can more easily become unstable with negative feedback (i.e., systems that use this configuration 
can have poor phase margin due to the extra transistor delay). 
Darlington  pairs  are  available  as  integrated  packages  or  can  be  made  from  two  discrete 
transistors; Q
1
 (the left-hand transistor in the diagram) can be a low power type, but normally Q
2
 
(on the right) will need to be high power. The maximum collector current I
C
(max) of the pair is 
that of Q
2
. A typical integrated power device is the 2N6282, which includes a switch-off resistor 
and has a current gain of 2400 at I
C
=10A. 
A Darlington pair can be sensitive enough to respond to the current passed by skin contact even 
at safe voltages. Thus it can form the input stage of a touch-sensitive switch. 
FET BIASING: 
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Unlike  BJTs,  thermal  runaway  does  not  occur  with  FETs,  as  already  discussed  in  our  blog. 
However,  the  wide  differences  in  maximum  and  minimum  transfer  characteristics  make  ID 
levels  unpredictable  with  simple  fixed-gate  bias  voltage.  To  obtain  reasonable  limits  on 
quiescent drain currents ID and drain-source voltage VDS, source resistor and potential divider 
bias  techniques  must  be  used.  With  few  exceptions,  MOSFET  bias  circuits  are  similar  to those 
used for JFETs. Various FET biasing circuits are discussed below: 
Fixed Bias. 
 
DC bias of a FET device needs setting of gate-source voltage V
GS
 to give desired drain current I
D
 
. For a JFET drain current is limited by the saturation current I
DS
. Since the FET has such a high 
input impedance that no gate current flows and the dc voltage of the gate set by a voltage divider 
or a fixed battery voltage is not affected or loaded by the FET. 
Fixed  dc  bias  is  obtained  using  a  battery  V
QG
.  This  battery  ensures  that  the  gate  is  always 
negative with respect to source and no current flows through resistor R
G
 and gate terminal that is 
I
G
 =0. The battery provides a voltage V
GS
 to bias the N-channel JFET, but no resulting current is 
drawn  from  the  battery  V
GG
.  Resistor  R
G
  is  included  to  allow  any  ac  signal  applied  through 
capacitor  C  to  develop  across  R
G
.  While  any  ac  signal  will  develop  across  R
G
,  the  dc  voltage 
drop across R
G
 is equal to I
G
 R
G 
i.e. 0 volt. 
The gate-source voltage V
GS
 is then 
V
GS
 = - v
G
  v
s
 =  v
GG
  0 =  V
GG
 
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The drain -source current I
D
 is then fixed by the gate-source voltage as determined by equation. 
This  current  then  causes  a  voltage  drop  across  the  drain  resistor  R
D
  and  is  given  as V
RD
  =  I
D
 
R
D and output voltage, Vout = VDD  ID RD
 
 
Self-Bias: 
 
This  is  the  most  common  method  for  biasing  a  JFET.  Self-bias  circuit  for  N-channel  JFET  is 
shown in figure. 
Since  no gate current flows through the reverse-biased gate-source, the  gate current I
G
 = 0 and, 
therefore,v
G
 = i
G
 R
G
 = 0 
The gate-source voltage is then 
V
Gs
 = V
G 
- V
s
 = 0  I
D
 R
s
 =  I
D
 R
s
  
So voltage drop across resistance  R
s
 provides the biasing  voltage V
Gg
  and  no external  source  is 
required for biasing and this is the reason that it is called self-biasing. 
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The operating point (that is zero signal I
D
 and V
DS
) can easily be determined from equation and 
equation given below : 
V
DS = 
V
DD
  I
D
 (R
D + 
R
S
) 
Thus  dc  conditions  of  JFET  amplifier  are  fully  specified. Self  biasing  of  a  JFET  stabilizes  its 
quiescent  operating  point  against  any  change  in  its  parameters  like  transconductance.  Let  the 
given JFET be replaced by another JFET having the double conductance then drain current will 
also  try  to  be  double  but  since  any  increase  in  voltage  drop  across  R
s
,  therefore,  gate-source 
voltage, V
GS
 becomes more negative and thus increase in drain current is reduced. 
Potential-Divider Biasing: 
 
fet-potential-divider-biasing 
A slightly modified form of dc bias is provided by the circuit shown in figure. The resistors R
Gl 
and  R
G2
  form  a  potential  divider  across  drain  supply  V
DD
.  The  voltage  V
2
  across  R
G2
  provides 
the  necessary  bias.  The  additional  gate  resistor  R
Gl
  from  gate  to  supply  voltage  facilitates  in 
larger adjustment of the dc bias point and permits use of larger valued R
S
. 
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The gate is reverse biased so that I
G
 = 0 and gate voltage 
V
G 
=V
2 
=
 
(V
DD
/R
 G1 + 
R
 G2 
) *R
G2
 
And  
V
GS
 = v
G
  v
s 
= V
G 
- I
D
 R
s
 
The operating point can be determined as  
I
D
 = (V
2
  V
GS
)/ R
S
 
And  
V
DS
 = V
DD
  I
D
 (R
D
 + R
S
) 
MOSFET-Metal Oxide Semiconductor Field Effect Transistor: 
 
Transistor, 
 
MOSFET-Schematic symbol   
Metal-oxide-semiconductor  field-effect  transistor  (MOSFET)  is  an  important  semiconductor 
device and is widely employed in many circuit applications. Since it is constructed with the gate 
terminal insulated from the channel, it is sometimes called insulated gate FET (IGFET). Like, a 
JFET, a MOSFET is also a three terminal (source, gate and drain) device and drain current in it is 
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also  controlled  by  gate  bias.  The  operation  of  MOSFET  is  similar  to  that  of  JFET.  It  can  be 
employed  in  any  of  the  circuits  covered  for  the  JFET  and,  therefore,  all  the  equations  apply 
equally well to the MOSFET and JFET in amplifier connections. However, MOSFET has lower 
capacitance and input impedance much more than that of a JFET owing to small leakage current. 
In  case  of  a  MOSFET the  positive  voltage  may  be  applied  to the  gate  and  still  the  gate  current 
remains zero. 
MOSFETs are of two types namely 
(i) Enhancement type MOSFET or E-MOSFET and 
(ii) Depletion enhancement MOSFET or DE-MOSFET.  
In  the  depletion-mode  construction  a  channel  is  physically  constructed  and  a  current  between 
drain  and  source  is  due  to  voltage  applied  across  the  drain-source  terminals.  The  enhancement 
MOSFET structure has no channel formed during its construction. Voltage is applied to the gate, 
in  this  case,  to  develop  a  channel  of  charge  carriers  so  that  a  current  results  when  a  voltage  is 
applied across the drain-source terminals. 
 
Advantages of FET over BJT are: 
a) No minority carriers 
b) High input impedance 
c)  It is a voltage controlled device 
d) Better thermal stability 
Effect of Source and Drain Series Resistance 
-  The analysis so far neglects the effects of the source/drain series resistance, and the entire voltage is 
assumed to drop along the channel. 
-  However, for modern day MOSFETs, this effect cannot be ignored, due to smaller diffusion cross-sections 
and smaller drain currents. 
-  The extrinsic (measured) voltages  can be related to the intrinsic (device) voltages 
by the following equations:  
 
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where  are the source and drain resistances respectively. 
-  The extrinsic transconductance  is related to the intrinsic transconductance 
 
 
where  is the intrinsic drain conductance. 
-  Similarly, the extrinsic drain conductance  is related to the intrinsic drain conductance 
 
 
 
                                                           UNIT IV 
                                   AMPLIFIERS AND OSCILLATORS 
Differential amplifier 
A differential amplifier  is a type of  electronic amplifier that  multiplies the difference  between 
two inputs by some constant factor (the differential gain). 
                                                
                                       Differential amplifier symbol 
 
The  inverting and  non-inverting  inputs are distinguished  by  ""  and "+"  symbols (respectively) 
placed  in  the  amplifier  triangle.  V
s+
  and  V
s
  are  the  power  supply  voltages;  they  are  often 
omitted from the diagram for simplicity, but of course must be present in the actual circuit. 
 
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Differential Amplifiers:  
Differential  amplifier  is  a  basic  building  block  of  an  op-amp.  The  function  of  a  differential 
amplifier is to amplify the difference between two input signals.  
How the differential amplifier is developed? Let us consider two emitter-biased circuits as shown 
in fig. 1.  
 
                                                                   Fig. 1  
The  two transistors  Q
1
  and  Q
2
  have  identical  characteristics.  The  resistances  of  the  circuits  are 
equal, i.e. R
E1
 = R 
E2
, R
C1
 = R 
C2
 and the magnitude of +V
CC
 is equal to the magnitude of V
EE
. 
These voltages are measured with respect to ground.  
To make a differential amplifier, the two circuits are connected as shown in fig. 1. The two +V
CC
 
and V
EE
 supply terminals  are  made common  because they  are same. The two emitters are also 
connected  and  the  parallel  combination  of  R
E1
  and  R
E2
  is  replaced  by  a  resistance  R
E
.  The  two 
input signals  v
1
  &  v
2
 are applied  at the  base of Q
1
 and at the  base of Q
2
. The output voltage  is 
taken between two collectors. The collector resistances are equal and therefore denoted by R
C
 = 
R
C1
 = R
C2
.  
Ideally, the output voltage is zero when the two inputs are equal. When v
1
 is greater then v
2
 the 
output voltage with the polarity  shown appears. When  v
1
  is  less than  v
2
, the output voltage  has 
the opposite polarity.  
The differential amplifiers are of different configurations.  
The four differential amplifier configurations are following:  
1.  Dual input, balanced output differential amplifier. 
2.  Dual input, unbalanced output differential amplifier. 
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3.  Single input balanced output differential amplifier. 
4.  Single input unbalanced output differential amplifier. 
 
 
                                                                         Fig. 2  
These  configurations  are  shown  in  fig. 2, and are  defined by  number  of input  signals used  and the  way  an output 
voltage is measured. If use two input signals, the configuration is said to be dual input, otherwise it is a single input 
configuration.  On  the  other  hand,  if  the  output  voltage  is  measured  between  two  collectors,  it  is  referred  to  as  a 
balanced output because both the collectors are at the same dc potential w.r.t. ground. If the output is measured at 
one of the collectors w.r.t. ground, the configuration is called an unbalanced output.  
A  multistage  amplifier  with  a  desired  gain  can  be  obtained  using  direct  connection  between  successive  stages  of 
differential amplifiers. The advantage of direct coupling is that it removes the lower cut off frequency imposed by the 
coupling capacitors, and they are therefore, capable of amplifying dc as well as ac input signals.  
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Dual Input, Balanced Output Differential Amplifier:  
The  circuit  is  shown  in  fig.  1,  v
1
  and  v
2
  are  the  two  inputs,  applied  to  the  bases  of  Q
1
  and  Q
2
 
transistors. The output voltage  is  measured between the two collectors C
1
 and C
2
 , which are at 
same dc potentials.  
D.C. Analysis:  
To  obtain  the  operating  point  (I
CC
  and  V
CEQ
)  for  differential  amplifier  dc  equivalent  circuit  is 
drawn by reducing the input voltages v
1
 and v
2
 to zero as shown in fig. 3. 
 
                                        Fig. 3  
The  internal  resistances  of  the  input  signals  are  denoted  by  R
S
  because  R
S1
=  R
S2
.  Since  both 
emitter  biased  sections  of  the  different  amplifier  are  symmetrical  in  all  respects,  therefore,  the 
operating point for only one section need to be determined. The same values of I
CQ
 and V
CEQ
 can 
be used for second transistor Q
2
.  
Applying KVL to the base emitter loop of the transistor Q
1
.  
 
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The value of R
E
 sets up the emitter current in transistors Q
1
 and Q
2
 for a given value of V
EE
. The 
emitter current in Q
1
 and Q
2
 are independent of collector resistance R
C
.  
The  voltage  at the  emitter of  Q
1
  is  approximately  equal  to  -V
BE
  if  the  voltage  drop  across  R  is 
negligible. Knowing the value of I
C
 the voltage at the collector V
C
is given by  
          V
C
 =V
CC
  I
C
 R
C
 
and V
CE
 = V
C
  V
E
  
               = V
CC
  I
C
 R
C
 + V
BE
 
       V
CE
 = V
CC
 + V
BE
  I
C
R
C
       (E-2) 
From the two equations V
CEQ
 and I
CQ
 can be determined. This dc analysis applicable for all types 
of differential amplifier.  
Example - 1  
The following specifications are given for the dual input, balanced-output differential amplifier 
of fig.1:  
R
C
 = 2.2 k, R
B
 = 4.7 k, R
in 1
 = R
in 2
 = 50  , +V
CC
 = 10V, -V
EE
 = -10 V, 
dc
 =100 and V
BE
 = 
0.715V. 
Determine the operating points (I
CQ
 and V
CEQ
) of the two transistors.  
Solution:  
The value of I
CQ
 can be obtained from equation (E-1).  
 
        
The voltage V
CEQ
 can be obtained from equation (E-2).  
 
The values of I
CQ
 and V
CEQ
 are same for both the transistors. 
 
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Dual Input, Balanced Output Difference Amplifier:  
The  circuit  is  shown  in  fig.  1  v
1
  and  v
2
  are  the  two  inputs,  applied  to  the  bases  of  Q
1
  and  Q
2
 
transistors. The  output  voltage  is  measured  between  the  two  collectors  C
1
  and  C
2
,  which  are  at 
same dc potentials.  
 
Fig. 1  
A.C. Analysis :  
In previous lecture dc analysis has been done to obtain the operatiing point of the two transistors. 
To  find  the  voltage  gain  A
d
  and  the  input  resistance  R
i
  of  the  differential  amplifier,  the  ac 
equivalent circuit is drawn using r-parameters as shown in fig. 2. The dc voltages are reduced to 
zero and the ac equivalent of CE configuration is used.  
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Fig. 2  
Since the two dc emitter currents are equal. Therefore, resistance r'
e1
 and r'
e2
 are also equal and 
designated by r'
e
 . This voltage across each collector resistance is shown 180 out of phase with 
respect to the  input voltages  v
1
 and  v
2
. This  is same as  in CE configuration. The polarity of the 
output voltage is shown in Figure. The collector C
2
 is assumed to be more positive with respect 
to collector C
1
 even though both are negative with respect to to ground.  
Applying KVL in two loops 1 & 2.  
 
Substituting current relations,  
 
Again, assuming  R
S1
 / b and  R
S2
 / b are  very small  in  comparison with  R
E
 and r
e
' and therefore 
neglecting these terms,  
 
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Solving these two equations, i
e1
 and i
e2
 can be calculated.  
 
The output voltage V
O
 is given by 
V
O
 = V
C2
 - V
C1
 
      = -R
C
 i
C2
 - (-R
C
 i
C1
) 
      = R
C
 (i
C1
 - i
C2
) 
      = R
C
 (i
e1
 - i
e2
)  
Substituting i
e1
, & i
e2
 in the above expression 
 
Thus  a  differential  amplifier  amplifies  the  difference  between  two  input  signals.  Defining  the 
difference  of  input  signals  as  v
d
  =  v
1
    v
2
  the  voltage  gain  of  the  dual  input  balanced  output 
differential amplifier can be given by  
      (E-2) 
Differential Input Resistance:  
Differential  input  resistance  is  defined  as  the  equivalent  resistance  that  would  be  measured  at 
either  input  terminal  with  the  other terminal  grounded.  This  means  that the  input  resistance  R
i1
 
seen from the input signal source v
1
 is determined with the signal source v
2
 set at zero. Similarly, 
the  input signal  v
1
  is set at zero to determine the  input resistance R
i2
 seen  from the  input signal 
source v
2
. Resistance R
S1
 and R
S2
 are ignored because they are very small.  
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Substituting i
e1
, 
 
Similarly, 
 
The factor of 2 arises because the r
e
' of each transistor is in series.  
To  get  very  high  input  impedance  with  differential  amplifier  is  to  use  Darlington  transistors. 
Another ways is to use FET.  
Output Resistance:  
Output  resistance  is  defined  as  the  equivalent  resistance  that  would  be  measured  at  output 
terminal with respect to ground. Therefore, the output resistance R
O1
 measured between collector 
C
1
 and ground is equal to that of the collector resistance R
C
. Similarly the output resistance R
O2
 
measured at C
2
 with respect to ground is equal to that of the collector resistor R
C
.  
R
O1
 = R
O2
 = R
C
        (E-5) 
The  current  gain  of  the  differential  amplifier  is  undefined.  Like  CE  amplifier  the  differential 
amplifier is a small signal amplifier. It is generally used as a voltage amplifier and not as current 
or power amplifier.  
 
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Difference Amplifiers  
A dual input, balanced output difference amplifier circuit is shown in fig. 1. 
 
Fig. 1  
Inverting & Non  inverting Inputs:  
In differential amplifier the output voltage v
O
 is given by  
               V
O
  =  A
d
  (v
1
    v
2
) 
When      v
2
  =  0,  v
O
  =  A
d
  v
1
 
& when   v
1
 = 0, v
O
 = - A
d
 v
2
  
Therefore  the  input  voltage  v
1
  is  called  the  non  inventing  input  because  a  positive  voltage  v
1
 
acting alone produces a positive output voltage v
O
. Similarly, the positive voltage v
2
 acting alone 
produces a negative output voltage hence  v
2
  is called  inverting  input. Consequently  B
1
  is called 
noninverting input terminal and B
2
 is called inverting input terminal.  
Common mode Gain:  
A  common  mode  signal  is  one  that  drives  both  inputs  of  a  differential  amplifier  equally.  The 
common mode signal is interference, static and other kinds of undesirable pickup etc.  
The  connecting  wires  on  the  input  bases  act  like  small  antennas.  If  a  differential  amplifier  is 
operating  in  an  environment  with  lot  of  electromagnetic  interference,  each  base  picks  up  an 
unwanted  interference  voltage.  If  both  the  transistors  were  matched  in  all  respects  then  the 
balanced output would be theoretically zero. This is the important characteristic of a differential 
amplifier.  It  discriminates  against  common  mode  input  signals.  In  other  words,  it  refuses  to 
amplify the common mode signals.  
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The  practical  effectiveness  of  rejecting  the  common  signal  depends  on  the  degree  of  matching 
between  the  two  CE  stages  forming  the  differential  amplifier.  In  other  words,  more  closely  are 
the currents in the input transistors, the better is the common mode signal rejection e.g. If v
1
 and 
v
2
 are the two input signals, then the output of a practical op-amp cannot be described by simply  
v
0
 = A
d
 (v
1
  v
2
 )  
In practical differential amplifier, the output depends not only on difference signal but also upon 
the common mode signal (average).  
        v
d
 = (v
1
  v
d
 )  
and v
C
 =  (v
1
 + v
2
 )  
The output voltage, therefore can be expressed as  
v
O
 = A
1
 v
1
 + A
2
 v
2
  
Where A
1
 & A
2
 are the voltage amplification from input 1(2) to output under the condition that 
input 2 (1) is grounded.  
 
The voltage gain for the difference signal is A
d
 and for the common mode signal is A
C
.  
The  ability  of  a  differential  amplifier  to  reject  a  common  mode  signal  is  expressed  by  its 
common mode rejection ratio (CMRR). It is the ratio of differential gain A
d
 to the common mode 
gain A
C
.  
 
Date sheet always specify CMRR in decibels CMRR = 20 log CMRR.  
Therefore, the differential amplifier should be designed so that r is large compared with the ratio 
of the common mode signal to the difference signal. If r = 1000, v
C
 = 1mV, v
d
 = 1 m V, then  
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It  is  equal  to  first  term.  Hence  for  an  amplifier  with  r  =  1000,  a  1m  V  difference  of  potential 
between two inputs gives the same output as 1mV signal applied with the same polarity to both 
inputs.  
 
Dual Input, Unbalanced Output Differential Amplifier:  
In this case, two input signals are given however the output is measured at only one of the two-
collector  w.r.t.  ground  as  shown  in  fig.  2.  The  output  is  referred  to  as  an  unbalanced  output 
because the collector at which the output voltage is measured is at some finite dc potential with 
respect to ground..  
 
Fig. 2  
In other words, there is some dc voltage at the output terminal without any input signal applied. 
DC analysis is exactly same as that of first case.  
 
AC Analysis:  
The output voltage gain in this case is given by  
 
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The voltage gain is half the gain of the dual input, balanced output differential amplifier. Since at 
the output there is a dc error voltage, therefore, to reduce the voltage to zero, this configuration is 
normally followed by a level translator circuit.  
Differential amplifier with swamping resistors:  
By  using  external  resistors  R'
E
  in  series  with  each  emitter,  the  dependence  of  voltage  gain  on 
variations of r'
e
 can be reduced. It also increases the linearity range of the differential amplifier.  
Fig.  3,  shows  the  differential  amplifier  with  swamping  resistor  R'
E
.  The  value  of  R'
E
  is  usually 
large enough to swamp the effect of r'
e
.  
 
Fig. 3  
 
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Biasing of Differential Amplifiers 
Constant Current Bias:  
In the dc analysis of differential amplifier, we have seen that the emitter current I
E
 depends upon 
the value of  b
dc
. To make operating point stable I
E
 current should be constant irrespective value 
of b
dc
.  
For constant I
E
, R
E
 should be very large. This also increases the value of CMRR but if R
E
 value 
is  increased  to  very  large  value,  I
E
  (quiescent  operating  current)  decreases.  To  maintain  same 
value  of  I
E
,  the  emitter  supply  V
EE
  must  be  increased.  To  get  very  high  value  of  resistance  R
E
 
and constant I
E
, current, current bias is used.  
 
Figure 5.1  
Fig. 1, shows the dual input balanced output differential amplifier using a constant current bias. 
The  resistance  R
E
  is  replace  by  constant  current transistor  Q
3
. The  dc  collector  current  in  Q
3
  is 
established by R
1
, R
2
, & R
E
.  
Applying the voltage divider rule, the voltage at the base of Q
3
 is  
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Because the two halves of the differential amplifiers are symmetrical, each has half of the current 
I
C3
.  
 
The  collector  current,  I
C3
  in  transistor  Q
3
  is  fixed  because  no  signal  is  injected  into  either  the 
emitter or the base of Q
3
.  
Besides  supplying  constant  emitter  current,  the  constant  current  bias  also  provides  a  very  high 
source resistance since the ac equivalent or the dc source is ideally an open circuit. Therefore, all 
the performance equations obtained for differential amplifier using emitter bias are also valid.  
As seen  in I
E
  expressions, the current depends upon V
BE3
. If temperature changes, V
BE
 changes 
and  current  I
E
  also  changes.  To  improve  thermal  stability,  a  diode  is  placed  in  series  with 
resistance R
1
as shown in fig. 2.  
 
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Fig. 2 
This helps to hold the current I
E3
 constant even though the temperature changes. Applying KVL 
to the base circuit of Q
3
.  
 
Therefore, the current I
E3
 is constant and independent of temperature because of the added diode 
D. Without D the current would vary with temperature because V
BE3
 decreases approximately by 
2mV/ C. The diode has same temperature dependence and hence the two variations cancel each 
other and I
E3
 does not vary appreciably with temperature. Since the cut  in voltage V
D
 of diode 
approximately  the  same  value  as  the  base  to  emitter  voltage  V
BE3
  of  a  transistor  the  above 
condition cannot be satisfied with one diode. Hence two diodes are used in series for V
D
. In this 
case the common mode gain reduces to zero. 
 
Some  times  zener  diode  may  be  used  in  place  of  diodes  and 
resistance as shown in fig. 3. Zeners are available over a wide 
range  of  voltages  and  can  have  matching  temperature 
coefficient  
The voltage at the base of transistor Q
B
 is  
 
 
Fig. 3  
The  value  of  R
2
  is  selected  so  that  I
2
    1.2  I
Z(min)
  where  I
Z
  is  the  minimum  current  required  to 
cause the zener diode to conduct in the reverse region, that is to block the rated voltage V
Z
.  
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Current Mirror:  
The circuit in which the output current is forced to equal the input current is said to be a current 
mirror circuit. Thus  in a  current  mirror circuit, the output current is  a  mirror image of the  input 
current. The current mirror circuit is shown in fig. 4. 
 
Fig. 4  
Once the current I
2
 is set up, the current I
C3
 is automatically established to be nearly equal to I
2
. 
The current mirror is a special case of constant current bias and the current mirror bias requires 
of  constant  current  bias  and  therefore  can  be  used  to  set  up  currents  in  differential  amplifier 
stages. The current mirror bias requires fewer components than constant current bias circuits.  
Since Q3 and Q4 are identical transistors the current and voltage are approximately same   
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For satisfactory operation two identical transistors are necessary.  
Oscillators 
Oscillators:  
An oscillator may be described as a source of alternating voltage. It is different than amplifier.  
An  amplifier  delivers  an  output  signal  whose  waveform  corresponds  to  the  input  signal  but 
whose power level is higher. The additional power content in the output signal is supplied by the 
DC power source used to bias the active device.  
The amplifier can therefore be described as an energy converter, it accepts energy  from the DC 
power supply and converts it to energy at the signal frequency. The process of energy conversion 
is  controlled  by  the  input  signal,  Thus  if  there  is  no  input  signal,  no  energy  conversion  takes 
place and there is no output signal.  
The  oscillator,  on  the  other  hand,  requires  no  external  signal  to  initiate  or  maintain  the  energy 
conversion  process.  Instead  an  output  signals  is  produced  as  long  as  source  of  DC  power  is 
connected. Fig. 1, shows the block diagram of an amplifier and an oscillator.  
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Fig. 1 
Oscillators may be classified in terms of their output waveform, frequency range, components, or 
circuit configuration.  
If  the  output  waveform  is  sinusoidal,  it  is  called  harmonic  oscillator  otherwise  it  is  called 
relaxation oscillator, which include square, triangular and saw tooth waveforms.  
Oscillators employ  both active and passive components. The active components provide energy 
conversion mechanism. Typical active devices are transistor, FET etc.  
Passive  components  normally  determine  the  frequency  of  oscillation.  They  also  influence 
stability, which is a measure of the change in output frequency (drift) with time, temperature or 
other  factors.  Passive  devices  may  include  resistors,  inductors,  capacitors,  transformers,  and 
resonant crystals.  
Capacitors  used  in  oscillators  circuits  should  be  of  high  quality.  Because  of  low  losses  and 
excellent stability, silver mica or ceramic capacitors are generally preferred. 
An  elementary  sinusoidal  oscillator  is  shown  in  fig.  2.  The  inductor  and  capacitors  are reactive 
elements  i.e.  they  are  capable  of  storing  energy.  The  capacitor  stores  energy  in  its  electric 
field.Whenever  there  is  voltage  across  its  plates,and  the  inductor  stores  energy  in  its  magnetic 
field whenever current flows through it. Both C and L are assumed to be loss less. Energy can be 
introduced into the circuit by charging the capacitor with a voltage V as shown in fig. 2. As long 
as the switch S is open, C cannot discharge and so i=0 and V=0.  
 
Fig. 2  
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Now  S  is  closed  at t  = t
o
,  This  means  V  rises  from  0  to  V,  Just  before  closing  inductor  current 
was  zero  and  inductor  current  cannot  be  changed  instantaneously.  Current  increases  from  zero 
value sinusoidally and is given by  
 
The  capacitor  losses  its  charge  and  energy  is  simply  transferred  from  capacitor  to  inductor 
magnetic field. The total energy is still same. At t = t
1
, all the charge has been removed from the 
capacitor  plates  and  voltage  reduces  to  zero  and  at  current  reaches  to  its  maximum  value.  The 
current  for  t> t
1
  charges  C  in  the  opposite  direction  and  current  decreases.  Thus  LC  oscillation 
takes places. Both voltage and current are sinusoidal though no sinusoidal input was applied. The 
frequency of oscillation is   
 
 
The  circuit  discussed  is  not  a  practical  oscillator  because  even  if  loss  less  components  were 
available, one could not extract energy with out introducing an equivalent resistance. This would 
result in damped oscillations as shown in fig. 3. 
 
Fig. 3  
These oscillations decay to zero as soon as the energy in the tank is consumed. If we remove too 
much power  from the circuit, the energy  may  be  completely  consumed  before the  first cycle of 
oscillations can take place yielding the over damped response.  
It  is  possible  to  supply  energy  to  the  tank  to  make  up  for  all  losses  (coil  losses  plus  energy 
removed), thereby maintaining oscillations of constant amplitude. 
Since  energy  lost  may  be  related  to  a  positive  resistance,  it  follows  that  the  circuit  would  gain 
energy  if  an  equivalent  negative  resistance  were  available.  The  negative  resistance,  supplies 
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whatever  energy  the  circuit  lose  due  to  positive  resistance.  Certain  devices  exhibit  negative 
resistance characteristics, an increasing current for a decreasing voltage. The energy supplied by 
the negative resistance to the circuit, actually comes from DC source that is necessary to bias the 
device in its negative resistance region.  
Another  technique  for  producing  oscillation  is  to  use  positive  feedback  considers  an  amplifier 
with an input signal v
in
 and output v
O
 as shown in fig. 4. 
 
Fig. 4  
The amplifier is inverting amplifier and may be transistorized, or FET or OPAMP. The output is 
180 out of phase with input signal            v
O
= -A v
in
.(A is negative)  
Now a feedback circuit is added. The output voltage is fed to the feed back circuit. The output of 
the  feedback  circuit  is  again  180  phase  shifted  and  also  gets  attenuated.  Thus  the  output  from 
the  feedback  network  is  in  phase  with  input  signal  v
in
  and  it  can  also  be  made  equal  to  input 
signal.  
If this  is so, V
f
 can  be  connected directly and externally applied signal can  be removed and the 
circuit will continue to generate an output signal. The amplifier still has an input but the input is 
derived  from  the  output  amplifier.  The  output  essentially  feeds  on  itself  and  is  continuously 
regenerated. This is positive feedback. The over all amplification from v
in
 to v
f
 is 1 and the total 
phase shift is zero. Thus the loop gain A  is equal to unity.  
 
When  this  criterion  is  satisfied  then  the  closed  loop  gain  is  infinite.  i.e.  an  output  is  produced 
without any external input.  
v
O
 = A v
error
 
      = A (v in + v f )  
       = A (v
in
 +  v
O
)  
or    (1-A  )v
O
 = A v
in
  
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or     
When A  = 1, v
O
 / v
in
=   
The criterion A  = 1 is satisfied only at one frequency.This is known as backhausen criterion.  
The  frequency  at  which  a  sinusoidal  oscillator  will  operate  is  the  frequency  for  which  the  total 
phase shift introduced, as the signal proceeds form the input terminals, through the amplifier and 
feed  back  network  and  back  again  to  the  input  is  precisely  zero  or  an  integral  multiple  of  2p. 
Thus the frequency of oscillation is determined by the condition that the loop phase shift is zero.  
Oscillation will not be sustained, if at the oscillator frequency, A  <1 or A >1. Fig. 5, show the 
output for two different contions A  < 1 and A  >1.  
 
Fig. 5  
If  A  is  less than unity then  A  v
in
  is  less than  v
in
, and the output signal will die out, when the 
externally  applied  source  is  removed.  If  A>1  then  A  b  v
in
is  greater  than  v
in
  and  the  output 
voltage builds up gradually. If A  = 1, only then output voltage is sine wave under steady state 
conditions.  
In  a  practical  oscillator,  it  is  not  necessary  to  supply  a  signal  to  start  the  oscillations.  Instead, 
oscillations  are  self-starting  and  begin  as  soon  as  power  is  applied.  This  is  possible  because  of 
electrical noise present in all passive components.  
Therefore, as soon as the power  is applied, there  is already some  energy  in the circuit at  f
o
, the 
frequency  for  which  the  circuit  is  designed  to oscillate.  This  energy  is  very  small  and  is  mixed 
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with all the other  frequency components also  present, but  it  is there. Only at this  frequency the 
loop gain is slightly greater than unity and the loop phase shift is zero. At all other frequency the 
Barkhausen  criterion  is  not  satisfied.  The  magnitude  of  the  frequency  component  f
o
  is  made 
slightly higher each time it goes around the loop. Soon the f
o
 component is much larger than all 
other  components  and  ultimately  its  amplitude  is  limited  by  the  circuits  own  non-lineareties 
(reduction  of  gain  at  high  current  levels,  saturation  or  cut  off).  Thus  the  loop  gain  reduces  to 
unity and steady stage is reached. If it does not, then the clipping may occur.  
Practically, A is made slightly greater than unity. So that due to disturbance the output does not 
change but  if  A = 1 and due to some reasons  if  A decreases slightly than the oscillation  may 
die out and oscillator stop functioning. In conclusion, all practical oscillations involve:  
-  An active device to supply loop gain or negative resistance.  
-  A frequency selective network to determine the frequency of oscillation.  
-  Some type of non-linearity to limit amplitude of oscillations.  
Example - 1  
The gain of certain amplifier as a  function of  frequency  is  A (j)  =  -16  x 10
6
 /  j.  A  feedback 
path connected around it has (j  ) = 10
3
 / (20 x 10
3
 + j )
2
. Will the system oscillate? If so, at 
what frequency ?  
Solution:  
The loop gain is   
To determine, if the system will oscillate, we will first determine the frequency, if any, at which 
the phase angle of  equals to 0 or a multiple of 360. Using phasor algebra, we have  
 
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This expression will equal -360 if  , 
 
Thus, the phase shift around the loop is -360 at  = 2000 rad/s. We must now check to see if the 
gain magnitude |A | = 1 at  = 2 x 10
3
. The gain magnitude is  
 
Substituting  = 2 x 10
3
, we find  
 
Thus,  the  Barkhausen  criterion  is  satisfied  at    =  2  x  10
3
  rad/s  and  oscillation  occurs  at  that 
frequency (2 x 10
3
 / 2 = 318 .3 Hz).  
Harmonic Oscillators 
According to Barkhausen criterion, a feedback type oscillator, having A as loop gain, works if 
A is made slightly greater than unity. As discussed in previous lectures, all practical oscillations 
involve:  
-  An active device to supply loop gain or negative resistance.  
-  A frequency selective network to determine the frequency of oscillation.  
-  Some type of non-linearity to limit amplitude of oscillations.  
Harmonic Oscillator:  
One feedback type harmonic oscillator circuit is shown in fig. 1. 
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Fig. 1   Fig. 2  
The  dc  equivalent  circuit  is  shown  in  fig.  2.  The  dc  operating  point  is  set  by  selecting  V
CC
,  R
B
 
and R
E
. The ac equivalent circuit is also shown in fig. 3. 
 
Fig. 3  
The  transformer  provides  180  phase  shift  to  ensure  positive  feedback  so  that  at  the  desired 
frequency of oscillation, the total phase  shift  from v
in
 to v
x
  is  made equal to 0 and  magnitudes 
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are  made  equal  by  properly  selecting  the  turns  ratio.  R
E
  also  controls  and  stabilizes  the  gain 
through  negative  feedback.  C
2
  and  the  transformers  equivalent  inductance  make  up  a  resonant 
circuit that determines the frequency of oscillation.  
C
1
  is  used  to  block  dc  (Otherwise  the  base  would  be  directly  tied  to  V
CC
)  through  the  low  dc 
resistance  of  transformer  primary.  C
1
  has  negligible  reactance  at  the  frequency  of  oscillation, 
therefore it is not apart of the frequency-determining network, the same applies to C
2
.  
In this circuit, there is an active device suitably biased to provide necessary gain. Since the active 
device  produces  loop  phase  shift  180  (from  base  to  collector),  a  transformer  in  the  feedback 
loop  provides  an  additional  180  to  yield  to  a  loop  phase  shift  of  0.  The  feedback  factor  is 
equivalent  to  the  transformer's  turns  ratio.  There  is  also  a  turned  circuit,  to  determine  the 
frequency of oscillation.  
The  load  is  in parallel with C
2
  and the transformer. If the  load  is resistive, which  is usually the 
case,  the  Q  of  the  tuned  circuit  and  the  loop  gain  are  both  affected,  this  must  be  taken  into 
account when determining the minimum gain required for oscillation. If the load has a capacitive 
component, then the value of C
2
 should be reduced accordingly.  
 
The RC Phase Shift Oscillator:  
At  low  frequencies  (around  100  KHz  or  less),  resistors  are  usually  employed  to  determine  the 
frequency oscillation. Various circuits are used in the feedback circuit including ladder network.  
 
Fig. 4  
A block diagram of a ladder type RC phase shift oscillation is shown in fig. 4. It consists of three 
resistor R and C capacitors. If the phase shift through the amplifier is 180, then oscillation may 
occur at the frequency where the RC network produces an additional 180 phase shift.  
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To find the frequency of oscillation, let us neglect the loading of the phase shift network. Writing 
the KV equations,  
 
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For  phase  shift  equal  to  180o  between  V
x
  and  V
O
,  imaginary  term  of  V
x
  /  V
O
  must  be  zero.  
Therefore,   
This is the frequency of oscillation. Substituting this frequency in V
x
 / V
O
 expression.  
 
In order to ensure the oscillation,  initially |A| >1 and under study state A =1. This  means the 
gain  of  the  amplifier  should  be  initially  greater  than  29  (so  that  A  >1)  and  under  steady  stat 
conditions it reduces to 29.  
 
This  oscillator  can  be  realized  using  FET  amplifier  as  shown  in  fig.  5.  The  feedback  circuit  is 
same as discussed above. 
 
 
Fig. 5   Fig. 6  
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The  input  impedance of  FET  is  very  high  so that there  is  no  loading of the  feedback  circuit. In 
this circuit, the feedback is voltage series feedback.  
V
x
 =V
GS
 +V
S
                or            V
GS
 = V
x
 - V  
The  same  circuit  can  be  realizing  using  OPAMP.  The  circuit  is  shown  in  fig.  6.  The  input 
impedance  is  very  high  and  there  is  no  overloading  of  feedback  circuit.  The  OPAMP  is 
connected  in  an  inverting  configuration  and  drives  three  cascaded  RC  sections.  The  inverting 
amplifier  causes  a  180  phase  shift  in  the  signal  passing  through  it.  RC  network  is  used  in  the 
feedback to provide additional 180 phase shift. Therefore, the total phase shift in the signal, of a 
particular frequency, around the loop will equal 360 and oscillation will occur at that frequency. 
The  gain  necessary  to overcome  the  loss  in  the  RC  network  and  bring  the  loop  gain  up  to  1  is 
supplied by the amplifier. The gain is given by  
 
Note  that  input  resistor  to  the  inverting  amplifier  is  also  the  last  resistor  of  the  RC  feedback 
network.  
Example -1:  
Design a RC phase shift oscillator that will oscillate at 100 Hz.  
Solution:  
An RC phase shift oscillator using OPAMP is shown in fig. 7. OPAMP is used as an inverting amplifier and provides 
180 phase shift. RC network is used in the feedback to provide additional 180 phase shift.  
 
Fig. 7  
For an RC phase shift oscillator the frequency is given by  
 
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Let C = 0.5 F. Then 
 
Therefore, R
f
= 29 R = 29 (1300) = 37.7 k.  
The  completed  circuit  is  shown  in  fig.  7.  R
f
  is  made  adjustable  so  the  loop  gain  can  be  set 
precisely to 1.  
Example - 2 
For the network shown in fig. 8 prove that 
 
This  network  is  used  with  an  OPAMP  to  form  an  oscillator.  Show  that  the  frequency  of 
oscillation is f =1 /2RC and the gain must exceed 3.  
Solution:  
To find the frequency of oscillation, let us neglect the loading of the phase shift network. Writing 
the KV equations,  
 
From equation (E-3), 
 
 
Fig. 8  
Substituting I
1
 in equation (E-4),. 
 
Solving this equation we get, 
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Therefore, from equation (E-1), 
 
Putting  , we get, 
 
For  phase  shift  equal  to  180  between  v
f
  and  v
o
,  imaginary  term  of  v
f
  /  v
o
  must  be  zero. 
Therefore, 
 
This is the frquency of oscillation. Substituting this frequency in v
f
 / v
o
 expression, we get, 
 
This shows that 0 phase shift from v
o
 to v
f
 can be obtained if  
 
and the gain of the feedback circuit becomes 1/3. Therefore, oscillation takes place if the gain of 
the amplifier exceeds 3.  
 
Transistor Phase Shift Oscillator:  
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At  low  frequencies  (around  100  kHz  or  less),  resistors  and  capacitors  are  usually  employed  to 
determine  the  frequency  of  oscillation.  Fig.  1  shows  transistorized  phase  shift  oscillator  circuit 
employing RC network. If the phase shift through the common emitter amplifier is 180, then the 
oscillation may occur at the frequency where the RC network produces an additional 180 phase 
shift.  
Since  a  transistor  is  used  as  the  active  element, the  output  across  R of  the  feedback  network  is 
shunted by the relatively low input resistance of the transistor, because input diode is a forward 
biased diode  
 
Fig. 1  
Hence,  instead  of  employing  voltage  series  feedback,  voltage  shunt  feedback  is  used  for  a 
transistor phase shift oscillator. The load resistance R
L
 is also connected via coupling capacitor. 
The equivalent circuit using h-parameter is shown in fig. 2.  
 
Fig. 2  
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For the circuit, the  load resistance  R
L
  may  be  lumped  with R
C
 and the effective  load resistance 
becomes  R'
L
(=  R
C
  ||  R
L
).  The  two  h-parameters  of  the  CE  transistor  amplifier,  h
oe
  and  h
re
  are 
neglected.  
The capacitor C offers some impedance at the frequency of oscillation and, therefore, it is kept as 
it  is, while the coupling capacitor behaves  like ac short. The  input resistance of the transistor is 
R
i
h
ie
. Therefore the resistance R
3
 is selected such that R=R
3
+R
i
=R
3
+h
ie
. This choice makes the 
three R C selections alike and simplifies the calculation. The effect of biasing resistor R
1
 , R
2
, & 
R
E
on the circuit operation is neglected.  
Since  this  is  a  voltage  shunt  feedback,  therefore  instead  of  finding  V
R
  /V
O
,  we  should  find  the 
current gain of the feedback loop. 
 
The simplified equivalent circuit is shown in fig. 3. 
 
Fig. 3  
Applying KVL,  
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Since I
3
 and I
b
 must be in phase to satisfy Barkhausen criterion, therefore  
 
Also initially I
3
 > I
b
, therefore, for oscillation to start, 
 
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Therefore, the two conditions must be satisfied for oscillation to start and sustain.  
Example - 1 
(a). Show that the OPAMP phase shifter shown in fig. 4  
. 
(b)  Cascade  two  identical  phase  shifters  of  the  type  sown  in  fig.  4.  Complete  the  loop  with  an 
inverting amplifier. Show that the system will   oscillate at the frequency  f = 1 / 2RC provided 
that the amplifier gain exceeds unity.  
(c)  Show  that  the  circuit  produces  two  quadrature  sinusoids  (sine  wave  differing  in  phase  by 
90).  
 
Fig. 4  
Solution:  
(a)The voltage the non-inverting terminal input of the OPAM is given by  
 
Since  the  differential  input  voltage  of  OPAMP  is  negligible  small,  therefore,  the  voltage  at the 
inverting terminal is also given by  
 
The input impedance of the OPAMP is very large, therefore,  
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or          V
i
 - 2V
2
 = -V
O
  
Substituting v
2
 in above equation, we get,  
 
Substituting X
C
, we get  
 
Therefore,   
and the phase angle between V
O
 and V
i
 is given by  
 
The magnitude of V
O
 / V
i
 is unity for all frequencies and the phase shift provided by this circuit 
is 0 for R = 0 and 180 for R > infinity.  
(b). If two such phase shifters are connected in cascade and an inverting amplifier with gain  is 
connected in the feedback loop, then the net loop gain becomes  
Loop gain = Gain of phase shifter 1 x Gain of phase shifter 2 x  
= 1 x 1x   
=   
Therefore, the oscillation takes place if gain  =1, but it is kept >1 so that the losses taking place 
in the amplifier can be compensated.  
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The total phase shift around the loop is given by  
total phase shift = -2 tan
-1
 (RC) - 2 tan
-1
(RC) + 180  
Further, for oscillation to take place the net phase shift around the loop would be 0.Therefore,  
-2 tan
-1
 (RC) - 2 tan
-1
(RC) + 180 =0 
or            RC = 1 
or            f = 1 / 2R C  
(c). The phase shift provided by amplifier in the feedback path is 180, therefore, the phase shift 
provided by the phase shifters should also be 180 to have 360 or 0 phase shift. Thus ,the phase 
shift provided by the individual shifter will be 90 as both are identical. Therefore, the sine wave 
produces by two phase shifters are 90 apart and the circuit produces two quadrature sinusoids.  
Wien Bridge Oscillator:  
The Wien Bridge oscillator is a standard oscillator circuit for low to moderate frequencies, in the 
range 5Hz to about 1MHz. It is mainly used in audio frequency generators.  
The  Wien  Bridge  oscillator  uses  a  feedback  circuit 
called a lead lag network as shown in fig. 1. 
At  very  low  frequencies,  the  series  capacitor  looks 
open to the input signal and there is no output signal. 
At  very  high  frequencies  the  shunt  capacitor  looks 
shorted,  and  there  is  no  output.  In  between  these 
extremes,  the  output  voltage  reaches  a  maximum 
value.  The  frequency  at  which  the  output  is 
maximized  is  called  the  resonant  frequency.  At  this 
frequency, the feedback fraction reaches a maximum 
value of 1/3.  
At very  low  frequencies, the phase angle  is positive, 
and the circuit acts like a lead network. On the other 
hand,  at  very  high  frequencies,  the  phase  angle  is 
negative,  and  the  circuit  acts  like  a  lag  network.  In 
between, there is a resonant frequency f
r
 at which the 
phase angle equals 0.  
The output of the lag lead network is  
 
Fig. 1  
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The gain of the feedback circuit is given by  
 
The phase angle between V
out
 and V
in
is given by  
 
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These  equations  shows  that  maximum  value  of  gain  occurs  at  X
C
  =  R,  and  phase  angle  also 
becomes 0. This represents the resonant  frequency of  load  lag  network.  Fig. 2, shows the gain 
and phase vs frequency.  
 
 
Fig. 2  
How Wien Bridge Oscillator Works: 
Fig.  3,  shows  a  Wien  Bridge  oscillator.  The  operational  amplifier  is  used  in  a  non-inverting 
configuration, and the lead-lag network provides the feedback. Resistors R
f
 and R
1
 determine the 
amplifier  gain  and  are  selected  to  make  the  loop  gain  equal  to  1.  If  the  feedback  circuit 
parameters are chosen properly, there will  be some  frequency at which there  is zero phase shift 
in  the  signal  fed  back  to  non  inverting  terminal.  Because  the  amplifier  is  non  inverting,  it  also 
contributes  zero  phase  shift,  so  the  total  phase  shift  around  the  loop  is  0  at  that  frequency,  as 
required for oscillation.  
The oscillator uses positive and  negative  feedback. The positive  feedback  helps the oscillations 
to  build  up  when  the  power  is  turn  on.  After  the  output  signal  reaches  the  desired  level  the 
negative  feedback  reduces  the  loop  gain  is  1.  The  positive  feedback  is  through  the  lead  lag 
network  to  the  non-inverting  input.  Negative  feedback  is  through  the  voltage  divider  to  the 
inverting input.  
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Fig. 3  
At power up, the tungsten lamp has a low resistance, and therefore, negative feedback is less. For 
this,  reason,  the  loop  gain  AB  is  greater  than  1,  and  oscillations  can  build  up  at  the  resonant 
frequency  f
r
.  As  the  oscillations  build  up, the  tungsten  lamp  heats  up  slightly  and  its  resistance 
increases. At the desired output level the tungsten lamp has a resistance R'. At this point  
 
Since  the  lead  lag  network  has  a  gain  (=B)  of  1/3,  the  loop  gain  AB  equals  unity  and  than  the 
output amplitude  levels off and  becomes constant. The  frequency of oscillation can  be adjusted 
by selecting R and C as  
 
The amplifier must have a closed loop cut off frequency well above the resonant frequency, f
r
.  
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Fig. 4  
Fig. 4, shows another way to represent Wein Bridge oscillator. The  lead  lag  network is the  left 
side of the bridge and the voltage divider is the right side. This ac bridge is called a Wein Bridge. 
The  error  voltage  is  the  output  of  the  Wein  Bridge.  When  the  bridge  approaches  balance,  the 
error voltage approaches zero.  
Example -1:  
Design a Wien-bridge oscillator that oscillates at 25 kHz.  
Solution:  
Let C
1
 = C
2
 = 0.001 F. Then, the frequency of oscillation is given by,  
 
or,   
Let R
1
 = 10 K. Then, 
 
or, R
f
 = 20K  
 
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Tuned Oscillator:  
A  variety  of  oscillator  circuits  can  be  built  using  LC  tuned  circuits.  A  general  form  of  tuned 
oscillator circuit is shown in  fig. 1. It is assumed that the active device used in the oscillator has 
very high input resistance such as FET, or an operational amplifier.  
 
 
Fig. 1   Fig. 2  
Fig. 2 shows  linear equivalent circuit of  fig. 1 using an amplifier with an open circuit gain  A
v
 
and  output  resistance  R
O
.  It  is  clear  from  the  topology  of  the  circuit  that  it  is  voltage  series 
feedback type circuit.  
The  loop  gain  of  the  circuit  A  can  be  obtained  by  considering  the  circuit  to  be  a  feedback 
amplifier  with  output taken  from  terminals  2  and  3  and  with  input terminals  1  and  3.  The  load 
impedance Z
L
 consists of Z
2
 in parallel with the series combination of Z
1
 and Z
3
. The gain of the 
the amplifier without feedback will be given by  
 
The feedback circuit gain is given by 
 
Therefore, the loop gain is given by  
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If the impedances are pure reactances (either inductive or capacitive), then Z
1
 = jX
1
, Z
2
= jX
2
 and 
Z
3
= jX
3
. Then  
 
For the loop gain to be real (zero phase shift around the loop),  
X
1
 + X
2
 + X
3
 = 0  
and       
Therefore, the circuit will oscillate at the resonant frequency of the series combination of X
1
, X
2
 
and X
3
. Since A    must be positive and at  leat unity  in  magnitude, then X
1
 and X
2
  must have 
the  same  sign  (A
v
  is  positive).In  other  words,  they  must  be  the  same  kind  of  reactance,  either 
both inductive or both capacitive.  
The Colpitts Oscillator:  
Wein bridge oscillator is not suited to high frequencies (above 1MHz). The main problem is the 
phase shift through the amplifier.  
The alternative is an LC oscillator, a circuit that can be used for frequencies between 1MHz and 
500MHz.  The  frequency  range  is  beyond  the  frequency  limit  of  most  OPAMPs.  With  an 
amplifier  and  LC  tank  circuit,  we  can  feedback  a  signal  with  the  right  amplitude  and  phase  is 
feedback to sustain oscillations. Fig. 3, shows the circuit of colpitts oscillator.  
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Fig. 3   Fig. 4  
The voltage divider bias sets up a quiescent operating point. The circuit then has a low frequency 
voltage gain of r
c
 / r'
e
 where r
c
 is the ac resistance seen by the selector. Because of the base and 
collector lag networks, the high frequency voltage gain is less then r
c
 / r'
e
.  
Fig. 4, shows a simplified ac equivalent circuit. The circulating or loop current in the tank flows 
through  C
1
  in  series  with  C
2
.  The  voltage  output  equals  the  voltage  across  C
1
.  The  feedback 
voltage v
f
 appears across C
2
. This  feedback  voltage drives the base and sustains the oscillations 
developed  across  the  tank  circuit  provided  there  is  enough  voltage  gain  at  the  oscillation 
frequency. Since the emitter is at ac ground the circuit is a CE connection.  
Most  LC  oscillators  use  tank  circuit  with  a  Q  greater than  10.  The  Q  of  the  feedback  circuit  is 
given by 
 
Because of this, the approximate resonant frequency is 
 
This  is  accurate  and  better  than  1%  when  Q  is  greater  than  1%.  The  capacitance  C  is  the 
equivalent capacitance the circulation current passes through. In the Colpitts tank the circulating 
current flows through C
1
 in series with C
2
.  
Therefore                  C = C
1
 C
2
 / (C
1
 +C
2
)  
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The required starting condition for any oscillator is A  > 1 at the resonant frequency or A > 1/ . 
The voltage gain A in the expression is the gain at the oscillation frequency. The feedback gain  
is given by  
 = v
f
 / v
out
 X
C1
 / X
C2
  
Because same current flow through C
1
 and C
2
, therefore  
 = C
1
/ C
2
;          A > 1/ v;           A> C
1
 / C
2
  
This is a crude approximation because it ignores the impedance looking into the base. An exact 
analysis would take the base impedance into account because it is in parallel with C
2
 .  
With small , the value of A is only slightly  larger than 1/. and the operation is approximately 
close  A.  When  the  power  is  switched  on,  the  oscillations  build  up,  and  the  signal  swings  over 
more  and  more  of  ac  load  line.  With  this  increased  signal  swing,  the  operation  changes  from 
small  signal  to  large  signal.  As  this  happen,  the  voltage  gain  decreases  slightly.  With  light 
feedback the value of A can decreases to 1 without excessive clapping.  
With  heavy  feedback, the  large  feedback signal drives the  base  into saturation and cut off. This 
charges  capacitor  C
3
  producing  negative  dc  clamping  at  the  base  and  changing  the  operation 
from class A to class C. The negative damping automatically adjusts the value of A to 1.  
Example - 1 
Design a Colpitts oscillator that will oscillate at 100 kHz.  
Solution:  
Let us choose R
1
 = R
f
 = 5 k and C = 0.001 F. From the frequency expression,  
 
The quality factor (Q) of the LC circuit is given by:  
 
Hartley Oscillator:  
Fig.  5,  shows  Hartley  oscillator  when  the  LC  tank  is  resonant,  the  circulating  current  flows 
through L
1
 in series with L
2
. Thus, the equivalent inductance is L = L
1
 + L
2
.  
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Fig. 5  
In  the  oscillator,  the  feedback  voltage  is  developed  by  the  inductive  voltage  divider,  L
1
  &  L
2
. 
Since  the  output  voltage  appears  across  L
1
  and  the  feedback  voltage  across  L
2
,  the  feedback 
fraction is  
 = V / V
out
 = X
L2
 / X
L1
 = L
2 
/ L
1
 
As usual, the loading effect of the base is ignored. For oscillations to start, the voltage gain must 
be greater than 1/ . The frequency of oscillation is given by 
 
Similarly, an opamp based Hartley oscillator circuit is shown in fig. 6.  
 
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Fig. 6  
 
Crystal Oscillator:  
Some crystals  found  in  nature exhibit the piezoelectric  effect  i.e.  when  an ac  voltage  is applied 
across  them,  they  vibrate  at  the  frequency  of  the  applied  voltage.  Conversely,  if  they  are 
mechanically  pressed,  they  generate  an  ac  voltage.  The  main  substances  that  produce  this 
piezoelectric effect are Quartz, Rochelle salts, and Tourmaline.  
Rochelle salts have greatest piezoelectric activity, for a given ac voltage, they vibrate more than 
quartz  or  tourmaline.  Mechanically,  they  are  the  weakest  they  break  easily.  They  are  used  in 
microphones, phonograph pickups, headsets and loudspeakers.  
Tourmaline shows the least piezoelectric activity but is a strongest of the three. It is also the most 
expensive and used at very high frequencies.  
Quartz  is  a  compromise  between  the  piezoelectric  activity  of  Rochelle  salts  and  the  strength  of 
tourmaline.  It  is  inexpensive  and  easily  available  in  nature.  It  is  most  widely  used  for  RF 
oscillators and filters.  
The  natural  shape  of  a  quartz  crystal  is  a  hexagonal  prism  with  pyramids  at  the  ends.  To  get  a 
useable  crystal  out  of  this  it  is  sliced  in  a  rectangular  slap  form  of  thickness  t.  The  number  of 
slabs we can get from a natural crystal depends on the size of the slabs and the angle of cut.  
 
Fig. 1  
For use in electronic circuits, the slab is mounted between two metal plates, as shown  in fig. 1. In 
this  circuit  the  amount  of  crystal  vibration  depends  upon  the  frequency  of  applied  voltage.  By 
changing the frequency, one can find resonant frequencies at which the crystal vibrations reach a 
maximum. Since the energy for the vibrations must be supplied by the ac source, the ac current is 
maximized  at  each  resonant  frequency.  Most  of  the  time,  the  crystal  is  cut  and  mounted  to 
vibrate  best  at  one  of  its  resonant  frequencies,  usually  the  fundamental  or  lowest  frequency. 
Higher  resonant  frequencies,  called  overtones,  are  almost  exact  multiplies  of  the  fundamental 
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frequency  e.g.  a  crystal  with  a  fundamental  frequency  of  1  MHz  has  a  overtones  of  2  MHz,  3 
MHz and so on. The formula for the fundamental frequency of a crystal is  
f = K / t.  
where K is a constant that depends on the cut and other factors, t is the thickness of crystal, f is 
inversely proportional to thickness t. The thinner the crystal, the more fragile it becomes and the 
more likely it is to break because of vibrations. Quartz crystals may have fundamental frequency 
up to  10  MHz.  To  get  higher  frequencies,  a  crystal  is  mounted  to  vibrate  on overtones;  we  can 
reach frequencies up to 100 MHz. 
AC Equivalent Circuit:  
When  the  mounted  crystal  is  not  vibrating,  it  is  equivalent  to  a  capacitance  C
m
,  because  it  has 
two metal plates separated by dielectric, C
m
 is known as mounting capacitance.  
 
Fig. 2  
When the crystal is vibrating, it acts like a tuned circuit. Fig. 2, shows the ac equivalent circuit of 
a  crystal  vibrating  at  or  near  its  fundamental  frequency.  Typical  values  are  L  is  henrys,  C  in 
fractions of a Pico farad, R in hundreds of ohms and C
m
 in Pico farads  
L
s
 = 3Hz,     C
s
 = 0.05 pf, R
s
 = 2K, C
m
 = 10 pf.  
The Q of the circuit is very very high. Compared with L-C tank circuit. For the given values, Q 
comes  out  to  be  3000.  Because  of  very  high  Q,  a  crystal  leads  to  oscillators  with  very  stable 
frequency values.  
The series resonant frequency f
S
 of a crystal is the sonant frequency of the LCR branch. At this 
frequency, the branch current reaches a maximum value because L
s
 resonant with C
S.
 
 
Above  f
S
,  the  crystal  behaves  inductively.  The  parallel  resonant  frequency  is  the  frequency  at 
which  the  circulating  or  loop  current  reaches  a  maximum  value.  Since  this  loop  current  must 
flow through the series combination of C
S
 and C
m
, the equivalent C
loop
 is  
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Since C
loop
 > C
S
, therefore, f
p
 > f
S
. 
Since  C
m
  >  C
S
,  therefore,  C
m
  ||  C
S
  is  slightly 
lesser  than  C
S
.  Therefore  f
P
  is  slightly  greater 
than f
S
. Because of the other circuit capacitances 
that  appear  across  C
m
  the  actual  frequency  will 
lie between f
S
 and f
P
. f
S
 and f
P
 are the upper and 
lower limits of frequency. The impedance of the 
crystal oscillator can  be plotted as a function of 
frequency as shown in fig. 3. 
At  frequency  f
S
,  the  circuit  behaves  like 
resistive  circuit.  At  f
P
  the  impedance  reaches  to 
maximum,  beyond  f
P
,  the  circuit  is  highly 
capacitive.  
The  frequency  of  an  oscillator  tends  to  change 
slightly  with  time.  The  drift  is  produced  by 
temperature, aging and other causes. In a crystal 
oscillator  the  frequency  drift  with  time  is  very 
small,  typically  less  than  1  part  in  10
6
  per  day. 
They  can  be  used  in  electronic  wristwatches.  If 
the drift  is 1 part  in 10
10
, a clock with this drift 
will take 30 years to gain or lose 1 sec.  
 
Fig. 3  
Crystals can be manufactured with values of f
s
 as low as 10 kHz; at these frequencies the crystal 
is  relatively  thick.  On  the  high  frequency  side,  f
s
  can  be  as  high  as  1-  MHz;  here  the  crystal  is 
very thin.  
The  temperature  coefficient  of  crystals  is  usually  small  and  can  be  made  zero.  When  extreme 
temperature stability is required, the crystal may be housed in an oven to maintain it at a constant 
temperature.  The  high  Q  of  the  crystal  also  contributes  to the  relatively  drift  free  oscillation  of 
crystal oscillators.  
 
Example - 1 
The parameters of the equivalent circuit of a crystal are given below:  
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L = 0.4 H, C
S
 = 0.06 pF, R = 5 k, C
m
 = 1.0 pF.  
Determine the series and parallel resonant frequencies of the crystal.  
Solution:  
With reference to fig. 2, the admittance of the crystal Y is given by  
 
where,   
 
and   
The resonant frequencies are obtained by putting B = 0. Thus,  
 
Consider the term C
S
 R
2
 / L
S
 = C
S
 R / [L R]. In a crystal, the time constant (L / R) is very much 
greater than C
S
 R. Thus the ratio  is  very  much  less than 1.  For the  values given, this ratio  is of 
the order of10
-6
. Neglecting this term in comparison with 2, we get two roots as  
 
where,  
s
  and  
p
  are  the  series  and  parallel  resonant  frequencies  respectively.  Substituting  the 
values, we get  
s
 = 6.45 M Hz. and 
p
 = 6.64 MHz  
Crystal Oscillators:  
Fig. 4, shows a colpitts crystal oscillator.  
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Fi. 4  
The  capacitive  voltage  divider  produces  the  feedback  voltage  for  the  base  of  transistor.  The 
crystal acts like an inductor that resonates with C
1
 and C
2
. The oscillation frequency is between 
the series and parallel resonant frequencies.  
Example-2:  
If the crystal of example-1  is used  in the oscillator circuit as shown  fig. 5, determine the values 
of R for the circuit to oscillate.  
 
Fig. 5  
Solution:  
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The  equivalent  circuit  of  crystal  (discussed  earlier)  shows  that  it  has  a  parallel  resonant  f
r
 
frequency  (
p
)  at  which  the  impedance  becomes  maximum.  The  amplified  signal  output of  the 
circuit  is  applied  across  the  potential  divider  consisting  of  R  and  the  crystal  circuit.  At  the 
resonant frequency the impedance of crystal becomes maximum (magnitude R) and thus the loop 
gain will  be greater than or equal to unity. At frequencies away  from 
p
 the  loop gain  becomes 
less than unity. The loop base shift is also zero around 
p
. Thus both the conditions required for 
sustained oscillations are satisfied and the circuit oscillates. 
The value of G of the crystal at  =
p
 is given by  
 
Thus the resistor R should be less than 5x10
6
 .  
 
 
 
 
 
                               UNIT V 
                                           PULSE CIRCUITS 
             
Clipper Circuits  
Clippers:  
Clipping  circuits  are  used  to  select  that  portion  of  the  input  wave  which  lies  above  or  below 
some reference level. Some of the clipper circuits are discussed here. The transfer characteristic 
(v
o
 vs v
i
) and the output voltage waveform for a given input voltage are also discussed.  
Clipper Circuit 1:  
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The  circuit  shown  in  fig.  3,  clips  the  input  signal  above  a 
reference voltage (V
R
). 
In this clipper circuit,  
          If  v
i
  <  V
R
,  diode  is  reversed  biased  and  does  not 
conduct. Therefore, v
o
 = v
i
  
and,   if v
i
 > V
R
, diode is forward biased and thus, v
o
= V
R
.  
The transfer characteristic of the clippers is shown in fig. 4. 
 
Fig. 3  
  
 
Fig. 4  
Clipper Circuit 2:  
The  clipper  circuit  shown  in  fig.  5  clips  the  input  signal 
below reference voltage V
R
. 
In this clipper circuit,  
              If v
i
 > V
R
, diode is reverse biased. v
o
 = v
i
 
and,    If v
i
 < V
R
, diode is forward biased. v
o
 = V
R
 
The transfer characteristic of the circuit is shown in fig. 6. 
 
Fig. 5 
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Fig. 6  
Clipper Circuit 3:  
To clip the input signal between two independent levels 
(V
R1
< V
R2
 ), the clipper circuit is shown in fig. 7. 
The diodes D
1
 & D
2
 are assumed ideal diodes.  
For this clipper circuit, when v
i
  V
R1
, v
o
=V
R1
 
and, v
i
  V
R2
, v
o
= V
R2
  
and, V
R1
 < v
i
 < V
R2
  v
o
 = v
i
 
The  transfer  characteristic  of  the  clipper  is  shown  in 
fig. 8. 
 
Fig. 7  
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Fig. 8  
 
Clipper Circuits  
Example  1:  
Draw the transfer characteristic of the circuit shown in fig. 9. 
 
Fig. 9  
Solution:  
When diode D
1
 is off,  i
1
 = 0, D
2
 must be ON.  
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and        v
o
 = 10 - 5 x 0.25 = 7.5 V 
v
p
 = v
o
 = 7.5 V 
Therefore, D
1
 is reverse biased only if v
i
 < 7.5 V 
If D
2
 is off and D
1
 is ON, i
2
 = 0  
 
and        v
p
 = 10 ( 0.04 v
i
 - 0.1 ) + 2.5 = 0.4 v
i
 + 1.5  
For D
2
 to be reverse biased, 
 
Between 7.5 V and 21.25 V both the diodes are ON. 
 
 
Fig. 10  
The transfer characteristic of the circuit is shown in fig. 10. 
 
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Clipper and Clamper Circuits  
Clippers:  
In  the  clipper  circuits,  discussed  so  far,  diodes  are  assumed  to  be  ideal  device.  If  third 
approximation circuit of diode  is used, the transfer characteristics of the clipper circuits  will  be 
modified.  
Clipper Circuit 4:  
Consider the clipper circuit shown in fig. 1 to clip the input signal above reference voltage  
   
Fig. 1   Fig. 2  
When v
i
 < (V
R
+ V
r
), diode D is reverse biased and therefore, v
o
= v
i
.  
and when v
i
 > ( V
R
 + V
r
 ), diode D is forward biased and conducts. The equivalent circuit, in this 
case is shown in fig. 2. 
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The current i in the circuit is given by  
 
The  transfer  characteristic  of  the  circuit  is 
shown in fig. 3. 
 
Fig. 3  
  Clipper Circuit 5:  
Consider the clipper circuit shown in fig. 4, which clips the input signal below the reference level 
(V
R
). 
If v
i
 > (V
R
  V
r
), diode D is reverse biased, thus v
O
 = v
i
 and when v
i
 < (v
R
 -V
r
), D condcuts and 
the equivalent circuit becomes as shown in fig. 5. 
   
Fig. 4   Fig. 5  
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Therefore, 
 
The  transfer  characteristic  of  the  circuit 
is shown in fig. 6. 
 
Fig. 6  
 
 
 
 
Clipper and Clamper Circuits  
Example - 1:  
  Find the output voltage v out of the clipper circuit of fig. 7(a) assuming that the diodes are  
a.  ideal.  
b.  V
on
 = 0.7 V. For both cases, assume R
F
 is zero. 
 
 
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Fig. 7(a)   Fig. 7(b)  
Solution:  
(a). When v
in
is positive and v
in
 < 3, then v
out
 = v
in
  
           and when v
in
 is positive and v
in
 > 3, then  
 
At vin = 8 V(peak), vout = 6.33 V.  
When vinis negative and vin > - 4, then vout = vin 
When vin is negative and vin < -4, then vout = -4V  
The resulting output wave shape is shown in fig. 7(b).  
(b). When VON = 0.7 V, vin is positive and vin < 3.7 V, then vout = vin  
When vin > 3.7 V, then  
 
When v
in
 = 8V, v
out
 = 6.56 V.  
When v
in
 is negative and v
in
 > -4.7 V, then v
out
 = v
in
  
When v
in
 < - 4.7 V, then v
out
 = - 4.7 V  
The resulting output wave form is shown in fig. 7(b). 
Clamper Circuits:  
Clamping  is  a  process  of  introducing  a  dc  level  into  a  signal.  For  example,  if  the  input  voltage 
swings  from  -10 V and  +10 V, a positive dc clamper, which  introduces +10 V  in the  input will 
produce the output that swings ideally from 0 V to +20 V.   The complete waveform is lifted up 
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by +10 V.  
Negative Diode clamper:  
A negative diode clamper is shown in fig. 8, which introduces a negative dc voltage equal to peak value of input in 
the input signal. 
 
 
                   Fig. 8                                Fig. 9  
Let the  input  signal  swings  form  +10  V  to  -10 
V.  During  first  positive  half  cycle  as  V  i  rises 
from 0 to 10 V, the diode conducts. Assuming 
an  ideal  diode,  its  voltage,  which  is  also  the 
output  must  be  zero  during  the  time  from  0  to 
t
1
.  The  capacitor  charges  during  this  period  to 
10 V, with the polarity shown.  
At that V
i
 starts to drop which means the anode 
of D is negative relative to cathode, ( V
D
 = v
i
 - 
v
c
  )  thus  reverse  biasing  the  diode  and 
preventing the capacitor from discharging.  Fig. 
9.  Since  the  capacitor  is  holding  its  charge  it 
behaves as a DC voltage source while the diode 
appears  as  an  open  circuit,  therefore  the 
equivalent  circuit  becomes  an  input  supply  in 
series  with  -10  V  dc  voltage  as  shown  in  fig. 
10,  and  the  resultant  output  voltage  is  the  sum 
 
                         Fig. 10  
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of instantaneous input voltage and dc voltage 
 (-10 V).  
  
 
Clamper Circuits  
Positive Clamper:  
The positive clamper circuit is shown in fig. 1, which introduces positive dc voltage equal to the 
peak of input signal. The operation of the circuit is same as of negative clamper.  
 
 
                        Fig. 1                                   Fig. 2  
Let the input signal swings form +10 V to -10 V. During first negative half cycle as V
i
 rises from 
0  to  -10  V,  the  diode  conducts.  Assuming  an  ideal  diode,  its  voltage,  which  is  also  the  output 
must be zero during the time from 0 to t
1
. The capacitor charges during this period to 10 V, with 
the polarity shown.  
After that V
i
 starts to drop which means the anode of D is negative relative to cathode, (V
D
= v
i
 - 
v
C
)  thus  reverse  biasing  the  diode  and  preventing  the  capacitor  from  discharging.  Fig.  2.  Since 
the capacitor is holding its charge it behaves as a DC voltage source while the diode appears as 
an open circuit, therefore the equivalent circuit becomes an input supply in series with +10 V dc 
voltage and the resultant output voltage is the sum of instantaneous input voltage and dc voltage 
(+10 V).  
To clamp the input signal by a voltage other than peak value, a dc source is required. As shown 
in fig. 3, the dc source is reverse biasing the diode.  
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The  input  voltage  swings  from  +10  V  to  -10  V.  In  the  negative  half  cycle  when  the  voltage 
exceed  5V  then  D  conduct.  During  input  voltage  variation  from  5  V  to  -10  V,  the  capacitor 
charges to 5 V with the polarity  shown  in  fig. 3. After that D becomes reverse  biased and open 
circuited. Then  complete ac signal  is  shifted upward by 5 V. The output waveform  is  shown  in 
fig. 4. 
 
 
                 Fig. 3                                              Fig. 4  
 
 
 
 
Clamper (electronics) 
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Positive unbiased voltage clamping shifts the amplitude of the input waveform so that all parts of 
it are greater than 0V 
A  clamper  is  an  electronic  circuit  that  prevents  a  signal  from  exceeding  a  certain  defined 
magnitude by shifting its DC value. The clamper does not restrict the peak-to-peak excursion of 
the signal,  but  moves  it up or down by a  fixed  value.  A  diode clamp (a  simple, common type) 
relies on a diode, which conducts electric current in only one direction;  resistors and capacitors 
in the circuit are used to maintain an altered dc level at the clamper output. 
General function 
A  clamping  circuit  (also  known  as  a  clamper)  will  bind  the  upper  or  lower  extreme  of  a 
waveform  to  a  fixed  DC  voltage  level.  These  circuits  are  also  known  as  DC  voltage  restorers. 
Clampers can  be constructed in both positive and  negative polarities.  When unbiased, clamping 
circuits  will  fix  the  voltage  lower  limit  (or  upper  limit,  in  the  case  of  negative  clampers)  to  0 
Volts.  These  circuits  clamp  a  peak  of  a  waveform  to  a  specific  DC  level  compared  with  a 
capacitively coupled signal which swings about its average DC level (usually 0V). 
Types 
Clamp circuits are categorised  by their operation; negative or positive and  biased  and unbiased. 
A positive clamp circuit outputs a purely  positive waveform  from an  input signal;  it offsets the 
input signal  so that all of the waveform  is greater than 0V.  A  negative clamp  is the opposite of 
this - this clamp outputs a purely negative waveform from an input signal. 
A bias voltage between the diode and ground offsets the output voltage by that amount. 
For example, an  input signal of peak  value 5V (V
IN
 = 5V) is applied to a positive clamp with a 
bias of 3V (V
BIAS
 = 3V), the peak output voltage will be 
V
OUT
 = 2V
IN
 + V
BIAS
 
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V
OUT
 = 2 * 5 + 3 
V
OUT
 = 13V 
Positive unbiased 
 
 
A positive unbiased clamp 
In the negative cycle of the input AC signal, the diode is forward biased and conducts, charging 
the  capacitor  to  the  peak  positive  value  of  V
IN
.  During  the  positive  cycle,  the  diode  is  reverse 
biased and thus does  not conduct. The output voltage  is therefore equal to the voltage stored in 
the  capacitor  plus  the  input  voltage  again,  so  V
OUT
  =  2V
IN
 
 
] Negative unbiased 
 
 
A negative unbiased clamp 
A negative unbiased clamp is the opposite of the equivalent positive clamp. In the positive cycle 
of  the  input  AC  signal,  the  diode  is  forward  biased  and  conducts,  charging  the  capacitor to the 
peak  value  of  V
IN
.  During  the  negative  cycle,  the  diode  is  reverse  biased  and  thus  does  not 
conduct. The output voltage is therefore equal to the voltage stored in the capacitor plus the input 
voltage  again,  so  V
OUT
  =  -2V
IN
 
 
Positive biased 
 
 
A positive biased clamp 
A positive biased voltage clamp is identical to an equivalent unbiased clamp but with the output 
voltage  offset  by  the  bias  amount  V
BIAS
.  Thus,  V
OUT
  =  2V
IN
  +  V
BIAS
 
 
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Negative biased 
 
 
A negative biased clamp 
A  negative  biased  voltage clamp  is  likewise  identical to an equivalent unbiased clamp  but with 
the output voltage offset in the negative direction by the bias amount V
BIAS
. Thus, V
OUT
 = -2V
IN
 
-  V
BIAS
 
 
 
Op-amp circuit 
 
 
Precision op-amp clamp circuit
[1]
 
The  figure  shows  an  op-amp  clamp  circuit  with  a  non-zero  reference  clamping  voltage.  The 
advantage here is that the clamping level is at precisely the reference voltage. There is no need to 
take into account the forward volt drop of the diode (which is necessary in the preceding simple 
circuits  as  this  adds  to  the  reference  voltage).  The  effect  of  the  diode  volt  drop  on  the  circuit 
output will be divided down by the gain of the amplifier, resulting in an insignificant error. 
Clamping for input protection 
Clamping  can  be  used  to  adapt  an  input  signal  to  a  device  that  cannot  make  use  of  or  may  be 
damaged by the signal range of the original input. 
Principles of operation 
The  schematic  of  a  clamper  reveals  that  it  is  a  relatively  simple  device.  The  two  components 
creating  the  clamping  effect  are  a  capacitor,  followed  by  a  diode  in  parallel  with  the  load.  The 
clamper circuit relies on a change in the capacitors time constant; this is the result of the diode 
changing current path with the changing input voltage. The magnitude of  R and C are chosen so 
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that  is  large  enough  to  ensure  that  the  voltage  across  the  capacitor  does  not  discharge 
significantly during the diode's "Non conducting" interval. During the first negative phase of the 
AC input voltage, the capacitor in the positive clamper charges rapidly. As V
in
 becomes positive, 
the  capacitor  serves  as  a  voltage  doubler;  since  it  has  stored  the  equivalent  of  V
in
  during  the 
negative cycle,  it provides  nearly that voltage during the positive cycle; this essentially doubles 
the voltage seen by the load. As V
in
 becomes negative, the capacitor acts as a battery of the same 
voltage  of  V
in
.  The  voltage  source  and  the  capacitor  counteract  each  other,  resulting  in  a  net 
voltage of zero as seen by the load. 
Biased versus non-biased 
By using a voltage source and resistor, the clamper can be biased to bind the output voltage to a 
different  value.  The  voltage  supplied  to the  potentiometer  will  be  equal  to the  offset  from  zero 
(assuming an  ideal diode)  in the case of either a  positive or negative clamper (the clamper type 
will  determine  the  direction  of  the  offset.  If  a  negative  voltage  is  supplied  to  either  positive  or 
negative,  the  waveform  will  cross  the  x-axis  and  be  bound  to  a  value  of  this  magnitude  on  the 
opposite  side.  Zener  diodes  can  also  be  used  in  place  of  a  voltage  source  and  potentiometer, 
hence setting the offset at the Zener voltage. 
Examples 
One common such clamping circuit is the DC restorer circuit in analog television receiver, which 
returns the  voltage of the  signal during the  back  porch of the  line  blanking period to 0V. Since 
the back porch  is  required to be at 0V on transmission, any DC or  low  frequency  hum that  has 
been induced onto the signal can be effectively removed via this method. 
Diode Clippers 
For  a  clipping  circuit  at  least  two  componentsan  ideal  diode  and  resistor  are  required  and 
sometimes a dc battery is also employed for fixing the clipping level. The diode acts as a closed 
switch  when  forward  biased  and  an  open  switch  when  reverse  biased.  The  input  waveform  can 
be clipped at different levels by simply changing the voltage of the battery and by interchanging 
the positions of the various elements. 
Depending on the orientation of the diode, the positive or negative region of the  input signal  is 
clipped off and accordingly the diode clippers may be positive or negative clippers.  
There  are  two  general  categories  of  clippers:  series  and  parallel  (or  shunt).  The  series 
configuration is defined as one where diode is in series with the load, while the shunt clipper has 
the diode in a branch parallel to the load. 
1. Positive Clipper  
The  clipper  which  removes  the  positive  half  cycles  of  the  input  voltage  is  called  the  positive 
clipper. The circuit arrangements for a positive clipper are illustrated in the figure given below. 
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Positive Series Clipper and Positive Shunt Clipper 
The  figure  illustrates  the  positive  series  clipper  circuit  (that  is,  diode  in  series  with  the  load). 
From the figure (a) it is seen that while the input is positive, diode D is reverse biased and so the 
output remains at zero that is, positive half cycle is clipped off. During the negative half cycle of 
the input, the diode is forward biased and so the negative half cycle appears across the output. 
Figure  (b)  illustrates  the  positive  shunt  clipper  circuit  (that  is,  diode  in  parallel  wit h  the  load). 
From the figure (b) it is seen that while input side is positive, the diode D is forward biased and 
conducts heavily (that is, diode acts as a closed switch). So the voltage drop across the diode or 
across the load resistance R
L
 is zero. Thus output voltage during the positive half cycles is zero, 
as shown in the output waveform. During the negative half cycles of the input signal voltage, the 
diode D is reverse  biased and  behaves as an open switch. Consequently the entire  input voltage 
appears across the diode or across the load resistance R
L
 if R is much smaller than R
L
 
Actually the circuit behaves as a voltage divider with an output voltage of [R
L
 / R+ R
L
] V
max 
= -
V
max 
when R
L 
>> R 
Note:  If  the  diode  in  figures  (a)  and  (b)  is  reconnected  with  reversed  polarity,  the  circuits  will 
become for a negative series clipper and negative shunt clipper respectively. The negative series 
and negative shunt clippers are shown in figures (a) and (b) as given below. 
 
Negative Series Clipper and Negative Shunt Clipper 
In  the  above  discussion,  the  diode  is  considered  to  be  ideal  one.  If  second  approximation  for 
diode  is considered the  barrier potential (0.7 V  for silicon and 0.3 V  for Germanium) of diode, 
will be taken into account. Then the output waveforms for positive and negative clippers will be 
of the shape shown in the figure below. 
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Output Waveform  Positive Clipper and Negative Clipper 
2. Biased Clipper 
Sometimes it is desired to remove a small portion of positive or negative half cycles of the signal 
voltage. Biased clippers are employed for this purpose. The circuit diagram for a biased negative 
clipper  (that  is  for  removing  a  small  portion  of  each  negative  half  cycle)  is  illustrated  in  figure 
(a). 
 
Biased Negative Clipper 
The action of the circuit is explained below. When the input signal voltage is  positive, the diode 
D  is reverse-biased and  behaves as an open-switch, the entire positive half cycle appears across 
the load, as illustrated by output waveform [figure (a)]. When the input signal voltage is negative 
but does not exceed battery voltage V, the diode D remains reverse-biased and most of the input 
voltage appears across the output. When during the negative half cycle of input signal, the signal 
voltage  exceeds  the  battery  voltage  V,  the  diode  D  is  forward  biased  i.e  conducts  heavily.  The 
output voltage is equal to  V and stays at  V as long as the input signal voltage is greater than 
battery voltage V  in  magnitude. Thus a biased negative clipper removes  input voltage when the 
input  signal  voltage  exceeds  the  battery  voltage.  Clipping  can  be  changed  by  reversing  the 
battery and diode connections, as illustrated in figure (b). 
 
Biased Positive Clipper 
Some  of  other  biased  clipper  circuits  are  given  below  in  the  figure.  While  drawing  the  wave-
shape of the output basic principle discussed above are followed. The diode has been considered 
as an ideal one. 
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Biased Clipper Circuits 
 
Different Clipping Circuits 
3. Combination Clipper 
When  a  portion  of  both  positive  and  negative  of  each  half  cycle  of  the  input  voltage  is  to  be 
clipped (or removed), combination clipper is employed. The circuit for such a clipper is given in 
the figure below. 
 
Combination Clipper 
The  action  of  the  circuit  is  summarized  below.  For  positive  input  voltage  signal  when  input 
voltage exceeds battery voltage + V
1 
diode D
1
 conducts heavily while diode D
2
 is reversed biased 
and  so  voltage  +  V
1
  appears  across  the  output.  This  output  voltage  +  V
1
  stays  as  long  as.  the 
input  signal  voltage  exceeds  +  V
1
.  On  the  other  hand  for  the  negative  input  voltage  signal,  the 
diode D
1
 remains reverse biased and diode D
2
 conducts heavily only when input voltage exceeds 
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battery voltage V
2
 in magnitude. Thus during the negative half cycle the output stays at   V
2
 so 
long as the input signal voltage is greater than -V
2
. 
Drawbacks of Series and Shunt Diode Clippers  
In series clippers, when diode is in off position, there should be no transmission of input signal 
to output.  But  in  case  of  high  frequency  signals  transmission  occurs  through  diode  capacitance 
which is undesirable. This is the drawback of using diode as a series element in such clippers. 
In  shunt  clippers,  when  diode  is  in  the  off  condition,  transmission  of  input  signal  should  take 
place to output. But in case of high frequency input signals, diode capacitance affects the circuit 
operation adversely and the signal gets attenuated (that is, it passes through diode capacitance to 
ground). 
Multivibrator 
A multivibrator is an electronic circuit used to implement a variety of simple two-state systems 
such  as  oscillators,  timers  and  flip-flops.  It  is  characterized  by  two  amplifying  devices 
(transistors, electron tubes or other devices) cross-coupled by resistors and capacitors. 
There are three types of multivibrator circuit: 
-  astable,  in which the circuit  is  not stable  in  either stateit continuously oscillates  from 
one state to the other. Due to this, it does not require an input (Clock pulse or other). 
-  monostable, in which one of the states is stable, but the other is notthe circuit will flip 
into  the  unstable  state  for  a  determined  period,  but  will  eventually  return  to  the  stable 
state. Such a circuit is useful for creating a timing period of fixed duration in response to 
some external event. This circuit is also known as a one shot. A common application is in 
eliminating switch bounce. 
-  bistable,  in  which  the  circuit  will  remain  in  either  state  indefinitely.  The  circuit  can  be 
flipped  from  one  state  to  the  other  by  an  external  event  or  trigger.  Such  a  circuit  is 
important as the fundamental building block of a register or memory device. This circuit 
is also known as a latch or a flip-flop. 
In  its  simplest  form  the  multivibrator  circuit  consists  of  two  cross-coupled  transistors.  Using 
resistor-capacitor networks within the circuit to define the time periods of the unstable states, the 
various  types  may  be  implemented.  Multivibrators  find  applications  in  a  variety  of  systems 
where  square  waves  or timed  intervals  are  required.  Simple  circuits  tend  to  be  inaccurate  since 
many factors affect their timing, so they are rarely used where very high precision is required. 
Before the advent of low-cost integrated circuits, chains of multivibrators found use as frequency 
dividers. A free-running multivibrator with a frequency of one-half to one-tenth of the reference 
frequency  would  accurately  lock  to  the  reference  frequency.  This  technique  was  used  in  early 
electronic  organs,  to  keep  notes  of  different  octaves  accurately  in  tune.  Other  applications 
included  early  television  systems,  where  the  various  line  and  frame  frequencies  were  kept 
synchronized by pulses included in the video signal. 
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Astable multivibrator circuit 
 
 
Figure 1: Basic BJT astable multivibrator 
This circuit shows a typical simple astable circuit, with an output from the collector of Q1, and 
an inverted output from the collector of Q2. 
Basic mode of operation 
The  circuit  keeps  one  transistor  switched  on  and  the  other  switched  off.  Suppose  that  initially, 
Q1 is switched on and Q2 is switched off. 
State 1: 
-  Q1 holds the bottom of R1 (and the left side of C1) near ground (0 V). 
-  The right side of C1 (and the base of Q2) is being charged by R2 from below ground to 
0.6 V. 
-  R3  is  pulling  the  base  of  Q1  up,  but  its  base-emitter  diode  prevents  the  voltage  from 
rising above 0.6 . 
-  R4  is charging the right side of C2 up to the power supply  voltage (+V). Because  R4  is 
less than R2, C2 charges faster than C1. 
When  the  base  of  Q2  reaches  0.6  V,  Q2  turns  on,  and  the  following  positive  feedback  loop 
occurs: 
-  Q2 abruptly pulls the right side of C2 down to near 0 V. 
-  Because  the  voltage  across  a  capacitor  cannot  suddenly  change,  this  causes  the  left  side 
of C2 to suddenly fall to almost V, well below 0 V. 
-  Q1 switches off due to the sudden disappearance of its base voltage. 
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-  R1 and R2 work to pull both ends of C1 toward +V, completing Q2's turn on. The process 
is stopped by the B-E diode of Q2, which will not let the right side of C1 rise very far. 
This now takes us to State 2, the mirror image of the initial state, where Q1 is switched off and 
Q2  is switched on. Then R1 rapidly pulls C1's  left side toward +V, while R3  more slowly pulls 
C2's left side toward +0.6 V. When C2's left side reaches 0.6 V, the cycle repeats. 
 
Multivibrator frequency 
The  period  of  each  half  of  the  multivibrator  is  given  by  t =  ln(2)RC.  The  total  period  of 
oscillation is given by: 
T = t
1
 + t
2
 = ln(2)R
2
 C
1
 + ln(2)R
3
 C
2
 
 
where... 
-  f is frequency in hertz. 
-  R
2
 and R
3
 are resistor values in ohms. 
-  C
1
 and C
2
 are capacitor values in farads. 
-  T is period time (In this case, the sum of two period durations). 
For the special case where 
-  t
1
 = t
2
 (50% duty cycle) 
-  R
2
 = R
3
 
-  C
1
 = C
2
 
 
Initial power-up 
When the circuit is first powered up, neither transistor will be switched on. However, this means 
that  at this  stage  they  will  both  have  high  base  voltages  and  therefore  a tendency  to  switch  on, 
and inevitable slight asymmetries will mean that one of the transistors is first to switch on. This 
will  quickly  put  the  circuit  into  one  of  the  above  states,  and  oscillation  will  ensue.  In  practice, 
oscillation always occurs for practical values of R and C. 
However, if the circuit is temporarily held with both bases high, for longer than it takes for both 
capacitors to charge fully, then the circuit will remain in this stable state, with both bases at 0.6 
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V,  both  collectors  at  0  V,  and  both  capacitors  charged  backwards  to  0.6  V. This  can  occur  at 
startup  without  external  intervention,  if  R  and  C  are  both  very  small.  For  example,  a  10  MHz 
oscillator  of  this  type  will  often  be  unreliable.  (Different  oscillator  designs,  such  as  relaxation 
oscillators, are required at high frequencies.) 
Period of oscillation 
Very roughly, the duration of state 1 (low output) will be related to the time constant R
2
C
1
 as it 
depends  on  the  charging  of  C1,  and  the  duration  of  state  2  (high  output)  will  be  related  to  the 
time constant R
3
C
2
 as it depends on the charging of C2. Because they do not need to be the same, 
an asymmetric duty cycle is easily achieved. 
However, the duration of each state also depends on the initial state of charge of the capacitor in 
question,  and  this  in  turn  will  depend  on  the  amount  of  discharge  during  the  previous  state, 
which  will  also  depend  on  the  resistors  used  during  discharge  (R1  and  R4)  and  also  on  the 
duration  of  the  previous  state,  etc.  The  result  is  that  when  first  powered  up,  the  period  will  be 
quite long as the capacitors are initially fully discharged, but the period will quickly shorten and 
stabilise. 
The period will also depend on any current drawn from the output and on the supply voltage. 
Protective components 
While not fundamental to circuit operation, diodes connected in series with the base or emitter of 
the  transistors  are  required  to  prevent  the  base-emitter  junction  being  driven  into  reverse 
breakdown when the supply voltage is in excess of the  V
eb
 breakdown voltage, typically around 
5-10  volts  for  general  purpose  silicon  transistors.  In  the  monostable  configuration,  only  one  of 
the transistors requires protection. 
 
 
 
Figure 2: Basic BJT monostable multivibrator. 
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Figure 3: Basic BJT bistable multivibrator. 
Non-electronic astables 
Astable oscillators are usually thought of as electronic circuits, but need not be. Bimetallic strips 
are  used  which  switch  an  electric  current  on  as  they  cool  and  off  as  they  heatflashing 
Christmas and car indicator lights may use this mechanism. 
Monostable multivibrator circuit 
When triggered by an input pulse, a monostable multivibrator will switch to its unstable position 
for a period of time, and then return to its stable state. The time period monostable multivibrator 
remains  in  unstable  state  is  given  by  t =  ln(2)R
2
C
1
.  If  repeated  application  of  the  input  pulse 
maintains  the  circuit  in  the  unstable  state,  it  is  called  a  retriggerable  monostable.  If  further 
trigger pulses do not affect the period, the circuit is a non-retriggerable multivibrator. 
Bistable multivibrator circuit 
Suggested values: 
-  R1, R2 = 10 k 
-  R3, R4 = 10 k 
This latch circuit is similar to an astable multivibrator, except that there is no charge or discharge 
time,  due  to  the  absence  of  capacitors.  Hence,  when  the  circuit  is  switched  on,  if  Q1  is  on,  its 
collector  is  at  0  V.  As  a  result,  Q2  gets  switched  off.  This  results  in  more  than  half  +V  volts 
being  applied  to  R4  causing  current  into  the  base  of  Q1,  thus  keeping  it  on.  Thus,  the  circuit 
remains  stable  in  a  single  state  continuously.  Similarly,  Q2  remains  on  continuously,  if  it 
happens to get switched on first. 
Switching of state can be done via Set and Reset terminals connected to the bases. For example, 
if Q2 is on and Set is grounded momentarily, this switches Q2 off, and makes Q1 on. Thus, Set is 
used to "set" Q1 on, and Reset is used to "reset" it to off state. 
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Astable Multivibrator 
Introduction 
Now  that  we  have  seen  the  bistable  multivibrator  and  then  modified  it  to  form  a  monostable 
multivibrator,  the  next  question  is,  Can  we  modify  it  further  to  use  capacitor  coupling  on  both 
sides? And what would happen if we did? 
Well, of course we can do this; the further question would be, Do we want to? And that depends 
on what happens when we build the circuit this way. 
Since  the  use  of  one  capacitor  prevents  the  circuit  from  remaining  stable  in  one  of  its  two 
possible states, it seems likely that with both sides coupled this way the circuit will be unable to 
remain stable in either state. That is in fact the case, and in this experiment we will construct and 
demonstrate this circuit. 
Schematic Diagram 
 
As  shown  in  the  schematic  diagram  here,  the  astable  multivibrator  simply  extends  the 
modification  that  converted  the  bistable  multivibrator  to  a  monostable  version  of  the  circuit. 
Now, both transistors are coupled to each other through capacitors. Whichever transistor is  off at 
any moment cannot remain off indefinitely; its base will become forward biased as that capacitor 
charges  towards  +5  volts.  Once  that  happens,  that  transistor  will  turn  on,  thereby  turning 
the other one off. 
 
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3-6 Figure 3-3.Astable Multivibrator.  
When  an  input  signal  to one  amplifier  is  large  enough, the  transistor  can  be  driven  into  cutoff, 
and  its  collector  voltage  will  be  almost  V 
CC
.  However,  when  the  transistor  is  driven  into 
saturation, its collector voltage will be about 0 volts. A circuit that is designed to go quickly from 
cutoff to saturation will produce a square or rectangular wave at its output. This principle is used 
in  multivibrators. Multivibrators are classified according to the  number of steady (stable) states 
of  the  circuit.  A  steady  state  exists  when  circuit  operation  is  essentially  constant;  that  is,  one 
transistor remains in conduction and the other remains cut off until an external signal is applied. 
The  three  types  of  multivibrators  are  the  ASTABLE,  MONOSTABLE,  and  BISTABLE.  The 
astable  circuit  has  no  stable  state.  With  no  external  signal  applied,  the  transistors  alternately 
switch  from  cutoff  to  saturation  at  a  frequency  determined  by  the  RC  time  constants  of  the 
coupling circuits. The  monostable  circuit  has one  stable state; one transistor conducts while the 
other  is  cut  off.  A  signal  must  be  applied  to  change  this  condition.  After  a  period  of  time, 
determined by the internal RC components, the circuit will return to its original condition where 
it remains until the next signal arrives. The bistable multivibrator has two stable states. It remains 
in one of the stable states until a trigger is applied. It then FLIPS to the other stable condition and 
remains  there  until  another  trigger  is  applied.  The  multivibrator then  changes  back  (FLOPS)  to 
its first stable state.  
Q1.    What  type  circuit  is  used  to  produce  square  or  rectangular  waves?  Q2.    What  type  of 
multivibrator does not have a stable state? Q3.   What type of multvibrator has one stable state? 
Q4.   What type of multivibrator has two stable states? 
                               Astable  Multivibrator  An  astable  multivibrator  is  also  known  as  a  FREE-
RUNNING  MULTIVIBRATOR.  It  is  called  free-  running  because  it  alternates  between  two 
different output voltage  levels during the time  it  is on. Theoutput remains  at each  voltage  level 
for  a  definite  period  of  time.  If  you  looked  at  this  output  on  an  oscilloscope,  you  would  see 
continuous square or rectangular waveforms. The astable multivibrator has two outputs, but NO 
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inputs.  Let's  look  at  the  multivibrator  in  figure  3-3  again.  This  is  an  astable  multivibrator.  The 
astable  multivibrator is said to oscillate. To understand why the astable  multivibrator oscillates, 
assume that transistor Q1 saturates and transistor Q2 cuts off when the circuit is energized. This 
situation is shown in figure 3-4. We assume Q1 saturates and Q2 is in cutoff because the circuit 
is symmetrical; that is, R1 = R4, R2 = R3, C1 = C2, and Q1 = Q2. It is impossible to tell which 
transistor  will  actually  conduct  when  the  circuit  is  energized.  For  this  reason,  either  of  the 
transistors  may  be  assumed  to  conduct  for  circuit  analysis  purposes.  Figure  3-4.Astable 
multivibrator  (Q1  saturated).  Essentially,  all  the  current  in  the  circuit  flows  through  Q1;  Q1 
offers almost no resistance to current flow. Notice that capacitor C1 is charging. Since Q1 offers 
almost  no  resistance  in  its  saturated  state,  the  rate  of  charge  of  C1  depends  only  on  the  time 
constant of R2 and C1 (recall that TC = RC). Notice that the right-hand  side of capacitor C1  is 
connected to the base of transistor Q2, which  is  now at cutoff. Let's analyze what is  happening. 
The  right-hand  side  of  capacitor  C1  is  becoming  increasingly  negative.  If  the  base  of  Q2 
becomes  sufficiently  negative,  Q2  will  conduct.  After  a  certain  period  of  time,  the  base  of  Q2 
will  become  sufficiently  negative  to  cause  Q2  to  change  states  from  cutoff  to  conduction.  The 
time  necessary  for  Q2  to  become  saturated  is  determined  by  the  time  constant  R2C1.  The  next 
state is shown in figure 3-5. The negative voltage accumulated on the right side on capacitor C1 
has  caused  Q2  to  conduct.  Now  the  following  sequence  of  events  takes  place  almost 
instantaneously. Q2 starts conducting and quickly saturates, and the voltage at output 2 changes 
from  Vapproximately 
CC
 to approximately 0 volts. This change  in  voltage  is coupled through 
C2 to the base of Q1, forcing Q1 to cutoff. Now Q1 is in cutoff and Q2 is in saturation. This is 
the circuit situation shown in figure 3-6.  
 
3-8  Figure  3-5.Astable  multivibrator.  Figure  3-6.Astable  multivibrator.  (Q2 
saturated). Notice that figure 3-6 is the mirror image of figure 3-4. In figure 3-6 the left side of 
capacitor C2 becomes more negative at a rate determined by the time constant R3C2. As the left 
side of C2 becomes more negative, the base of Q1 also becomes more negative. When the base 
of  Q1  becomes  negative  enough  to  allow  Q1  to  conduct,  Q1  will  again  go  into  saturation.  The 
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resulting  change  in  voltage  at  output  1  will  cause  Q2  to  return  to  the  cutoff  state.  Look  at  the 
output  waveform  from  transistor  Q2,  as  shown  in  figure  3-7.  The  output  voltage  (from  either 
output  of  the  multivibrator)  alternates  from  approximately  0  volts  to    Vapproximately 
CC
, 
remaining in each state for a definite period of time. The time may range from a microsecond to 
as much as a second or two.  VIn some applications, the time period of higher voltage ( 
CC
) and 
the  time  period  of  lower  voltage  (0  volts)  will  be  equal.  Other  applications  require  differing 
higher-  and  lower-voltage  times.  For  example,  timing  and  gating  circuits  often  have  different 
pulse widths as shown in figure 3-8.   
 
3-9  Figure  3-7.Square  wave  output  from  Q2.  Figure  3-8.Rectangular  waves. 
FREQUENCY  STABILITY.Some  astable  multivibrators  must  have  a  high  degree  of 
frequency  stability.  One  way  to obtain  a  high  degree  of  frequency  stability  is  to  apply  triggers. 
Figure  3-9,  view  (A),  shows  the  diagram  of  a  triggered,  astable  multivibrator.  At  time  T0,  a 
negative  input  trigger  to  the  base  of  Q1  (through  C1)  causes  Q1  to  go  into  saturation,  which 
drives Q2 to cutoff. The circuit will remain in this condition as long as the base voltage of Q2 is 
positive. The length of time the base of Q2 will remain positive is determined by C3, R3, and R6. 
Observe the parallel paths for C3 to discharge. Figure 3-9A.Triggered astable multivibrator 
and output. 
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 View (B) of figure 3-9 shows the waveforms associated with the circuit. At time T1, Q2 comes 
out of cutoff and goes into saturation. Also, Q1 is caused to come out of saturation and is cut off. 
The  base  voltage  waveform  of  Q1  shows  a  positive  potential  that  is  holding  Q1  at  cutoff.  This 
voltage would normally hold Q1 at cutoff until a point between T2 and T3. However, at time T2 
another  trigger  is  applied  to  the  base  of  Q1,  causing  it  to  begin  conducting.  Q1  goes  into 
saturation  and  Q2  is  caused  to  cut  off.  This  action  repeats  each  time  a  trigger  (T2,  T4,  T6)  is 
applied.  
r  
Figure 3-9B.Triggered astable multivibrator and output.  
 
 
The  prt  of  the  input  triggers  must  be  shorter  than  the  natural  free-running  prt  of  the  astable 
multivibrator,  or the  trigger  prf  must  be  slightly  higher  than  the  free-running  prf  of  the  circuit. 
This is to make certain the triggers control the prt of the output. 
 
 
 Monostable  Multivibrator  The  monostable  multivibrator  (sometimes  called  a  ONE-SHOT 
MULTIVIBRATOR)  is  a  square-  or  rectangular-wave  generator  with  just  one  stable  condition. 
With no input signal (quiescent condition) one amplifier conducts and the other is in cutoff. The 
monostable  multivibrator  is  basically  used  for  pulse  stretching.  It  is  used  in  computer  logic 
systems  and  communication  navigation  equipment.  The  operation  of  the  monostable 
multivibrator  is  relatively  simple.  The  input  is  triggered  with  a  pulse  of  voltage.  The  output 
changes  from  one  voltage  level  to  a  different  voltage  level.  The  output  remains  at  this  new 
voltage  level  for  a  definite  period  of  time.  Then  the  circuit  automatically  reverts  to  its  original 
condition and remains that way until another trigger pulse is applied to the input. The monostable 
multivibrator  actually  takes  this  series  of  input  triggers  and  converts  them  to  uniform  square 
pulses,  as  shown  in  figure  3-10.  All  of  the  square  output  pulses  are  of  the  same  amplitude  and 
time duration. 
 
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Figure 3-10.Monostable multivibrator block diagram.  
 
 
The  schematic  for  a  monostable  multivibrator  is  shown  in  figure  3-11.  Like  the  astable 
multivibrator, one transistor conducts and the other cuts off when the circuit is energized.  
 
 
 
               Figure 3-11.Monostable multivibrator schematic.  
 
Recall that when the astable multivibrator was first energized, it was impossible to predict which 
transistor  would  initially  go  to  cutoff  because  of  circuit  symmetry.  The  one-shot  circuit  is  not 
symmetrical like the astable multivibrator. Positive voltage V
BB
 is applied through R5 to the base 
of Q1. This positive voltage causes Q1 to cut off. Transistor Q2 saturates because of the negative  
Vvoltage applied  from 
CC
 to its base through R2. Therefore, Q1 is cut off and Q2  is saturated 
before a trigger pulse is applied, as shown in figure 3-12. The circuit is shown in its stable state.  
 
 
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                      Figure 3-12.Monostable multivibrator (stable state).  
 
Let's take a more detailed look at the circuit conditions in this stable state (refer to figure 3-12). 
As stated above, Q1 is cut off, so no current flows through R1, and the collector of Q1   Vis at 
CC
. Q2 is saturated and has practically no voltage drop across it, so its collector is essentially at 0 
volts. R5 and R3 form a voltage divider from V
BB
 to the ground potential at the collector of Q2. 
The tie point between these two resistors will be positive. Thus, the base of Q1 is held positive, 
ensuring that Q1 remains cutoff. Q2 will remain saturated because the base of Q2 is very slightly 
negative as  a result of the    Vvoltage drop across R2. If the  collector of Q1  is  near 
CC
 and the 
base of Q2 is near ground, C1 must be charged to nearly V
CC
 volts with the polarity shown. Now 
that all the components and voltages have been described for the stable state, let us see how the 
circuit operates (see  figure 3-13). Assume that a negative pulse  is applied at the  input terminal. 
C2 couples this voltage change to the base of Q1 and starts Q1 conducting. Q1 quickly saturates, 
and  its  collector  voltage  immediately  rises  to  ground  potential.  This  sharp  voltage  increase  is 
coupled  through  C1  to  the  base  of  Q2,  causing  Q2  to  cut  off;  the  collector  voltage  of  Q2 
immediately drops to V
CC
. The  voltage divider formed by R5 and R3 then holds the base of Q1 
negative, and Q1 is locked in saturation 
 
 
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                                 Figure 3-13.Monostable multivibrator (triggered). 
 
The one-shot multivibrator has now been turned on by applying a pulse at the input. It will turn 
itself off after a period of time. To see how it does this, look at figure 3-13 again. Q1 is held in 
saturation by the negative voltage applied through R3 to its base, so the circuit cannot be turned 
off  here.  Notice  that  the  base  of  Q2  is  connected  to  C1.  The  positive  charge  on  C1  keeps  Q2 
cutoff.  Remember  that  a  positive  voltage  change  (essentially  a  pulse)  was  coupled  from  the 
collector  of  Q1  when  it  began  conducting  to  the  base  of  Q2,  placing  Q2  in  cutoff.  When  the 
collector of Q1 switches from -V
CC
 volts to 0 volts, the charge on C1 acts like a battery with its 
negative terminal on the  collector of Q1, and  its  positive terminal  connected to the base of  Q2. 
This  voltage  is  what  cuts  off  Q2.  C1  will  now  begin  to  discharge  through  Q1  to  ground,  back 
through    V
CC
,  through  R2  to  the  other  side  of  C1.  The  time  required  for  C1  to  discharge 
depends on the RC time constant of C1 and R2. Figure 3-14 is a timing diagram that shows the 
negative  input  pulse  and  the  resultant  waveforms  that  you  would  expect  to  see  for  this  circuit 
description. 
 
 
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                          Figure 3-14.Waveforms of a monostable multivibrator (triggered). 
 
The only part of the operation not  described so far is the short C1 charge time that occurs right 
after  Q1  and  Q2  return  to  their  stable  states.  This  is  simply  the  time  required  for  C1  to  gain 
electrons on its left side. This charge time is determined by the R1C1 time constant.  
 
Another version of the monostable multivibrator is shown in figure 3-15. View (A) is the circuit 
and view (B) shows the associated waveforms. In its stable condition (T0), Q1 is cut off and Q2 
is  conducting.  The  input  trigger  (positive  pulse  at  T1)  is  applied  to  the  collector  of  Q1  and 
coupled by C1 to the base of Q2 causing Q2 to be cut off.   VThe collector voltage of Q2 then 
goes 
CC
. The  more  negative  voltage at the collector of Q2  forward  biases Q1 through R4.  With 
the  forward  bias,  Q1  conducts,  and  the  collector  voltage  of  Q1  goes  to  about  0  volts.  C1  now 
discharges and keeps Q2 cut off. Q2 remains cut off until C1 discharges enough to allow Q2 to 
conduct again (T2). When Q2 conducts again, its collector voltage goes toward 0 volts and Q1 is 
cut off. The circuit returns to its quiescent state and has completed a cycle. The circuit remains in 
this stable state until the next trigger arrives (T3). 
 
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Figure 3-15A.Monostable miltivibrator and waveshapes. Schematic.  
 
 
3-14 Figure 3-15B.Monostable miltivibrator and waveshapes. Waveshapes  
 
 
 
Note  that  R3  is  variable  to  allow  adjustment  of  the  gate  width.  Increasing  R3  increases  the 
discharge time for C1 which increases the cutoff time for Q2. Increasing the value of R3 widens 
the  gate.  To  decrease  the  gate  width,  decrease  the  value  of  R3.  Figure  3-16  shows  the 
relationships  between  the  trigger  and  the  output  signal.  View  (A)  of  the  figure  shows  the  input 
trigger;  views  (B)  and  (C)  show  the  different  gate  widths  made  available  by  R3.  Although  the 
durations  of  the  gates  are  different, the  duration  of  the  complete  cycle  remains  the  same  as  the 
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pulse repetition time of the triggers. View (D) of the figure illustrates that the trailing edge of the 
positive alternation is variable. 
 
 
 
 
 
 
 Figure 3-16.Monostable multivibrator waveforms with a variable gate.  
 
The  reason  the  monostable  multivibrator  is  also  called  a  one-shot  multivibrator  can  easily  be 
seen.  For  every  trigger  pulse  applied  to  the  multivibrator,  a  complete  cycle,  or  a  positive  and 
negative  alternation  of  the  output,  is  completed.  Q5.    In  an  astable  multivibrator,  which 
components determine the pulse repetition frequency? 
Schmitt trigger 
 
The effect of using a Schmitt trigger (B) instead of a comparator (A). 
In  electronics,  a  Schmitt  trigger  is  a  comparator  circuit  that  incorporates  positive  feedback.In 
the  non-inverting  configuration,  when  the  input  is  higher  than  a  certain  chosen  threshold,  the 
output  is  high;  when  the  input  is  below  a  different (lower)  chosen  threshold,  the  output  is  low; 
when the input is between the two, the output retains its value. The trigger is so named because 
the  output  retains  its  value  until  the  input  changes  sufficiently  to  trigger  a  change.  This  dual 
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threshold  action  is  called  hysteresis,  and  implies  that the  Schmitt  trigger  has  some  memory.  In 
fact, the Schmitt trigger is a bistable multivibrator. 
Schmitt  trigger  devices  are  typically  used  in  open  loop  configurations  for  noise  immunity  and 
closed loop positive feedback configurations to implement multivibrators. 
Invention 
The  Schmitt trigger  was  invented  by  US  scientist  Otto  H.  Schmitt  in  1934  while  he  was  still  a 
graduate student,
[1]
 later described in his doctoral dissertation (1937) as a "thermionic trigger".
[2]
 
It was a direct result of Schmitt's study of the neural impulse propagation in squid nerves.
[2]
 
Symbol 
The  symbol  for  Schmitt  triggers  in  circuit  diagrams  is  a  triangle  with  an  inverting  or  non-
inverting hysteresis symbol. The symbol depicts the corresponding ideal hysteresis curve. 
 
 
Standard Schmitt trigger 
    
 
 
Inverting  Schmitt  trigger  (WRONG  IMAGE!  Should 
have a circle at the right point of the triangle indicating 
inversion! 
Implementation 
A  Schmitt trigger  can  be  implemented  with  a  simple  tunnel  diode,  a  diode  with  an  "N"-shaped 
currentvoltage  characteristic  in  the  first  quadrant.  An  oscillating  input  will  cause  the  diode  to 
move  from one rising  leg of the  "N" to the other  and  back  again as the  input crosses the rising 
and  falling  switching  thresholds.  However,  the  performance  of  this  Schmitt  trigger  can  be 
improved with transistor-based devices that make explicit use of positive feedback to implement 
the switching. 
Comparator implementation 
Schmitt triggers are commonly  implemented using a comparator
[nb  1]
 connected to have positive 
feedback (i.e., instead of the usual negative feedback used in operational amplifier circuits). For 
this  circuit,  the  switching  occurs  near  ground,  with  the  amount  of  hysteresis  controlled  by  the 
resistances of R
1
 and R
2
: 
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The  comparator  extracts  the  sign  of  the  difference  between  its  two  inputs.  When  the  non-
inverting  (+)  input  is  at  a  higher  voltage  than  the  inverting  ()  input,  the  comparator  output 
switches to +V
S
, which is its high supply voltage. When the non-inverting (+) input is at a lower 
voltage  than  the  inverting  ()  input,  the  comparator  output  switches  to  -V
S
,  which  is  its  low 
supply  voltage.  In  this  case,  the  inverting  ()  input  is  grounded,  and  so  the  comparator 
implements  the  sign  function   its  2-state  output  (i.e.,  either  high  or  low)  always  has  the  same 
sign as the continuous input at its non-inverting (+) terminal. 
Because  of  the  resistor  network  connecting  the  Schmitt  trigger  input,  the  non-inverting  (+) 
terminal of the comparator, and the comparator output, the Schmitt trigger acts like a comparator 
that  switches  at  a  different  point  depending  on  whether  the  output of  the  comparator  is  high  or 
low. For very negative inputs, the output will be low, and for very positive inputs, the output will 
be  high,  and  so  this  is  an  implementation  of  a  "non-inverting"  Schmitt  trigger.  However,  for 
intermediate  inputs,  the  state  of  the  output  depends  on  both  the  input  and  the  output.  For 
instance,  if  the  Schmitt  trigger  is  currently  in  the  high  state,  the  output  will  be  at  the  positive 
power supply rail (+V
S
). V
+
 is then a voltage divider between V
in
 and +V
S
. The comparator will 
switch when V
+
=0 (ground). Current conservation shows that this requires 
 
and so V
in
 must drop below  to get the output to switch. Once the comparator output has 
switched to V
S
, the threshold becomes  to switch back to high. 
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Typical hysteresis curve (which matches the curve shown on a Schmitt trigger symbol) 
So this circuit creates a switching  band centered around zero, with trigger  levels  . The 
input voltage must rise above the top of the band, and then below the bottom of the band, for the 
output  to  switch  on  and  then  back  off.  If  R
1
  is  zero  or  R
2
  is  infinity  (i.e.,  an  open  circuit),  the 
band collapses to zero width, and it behaves as a standard comparator. The output characteristic 
is  shown  in  the  picture  on  the  right.  The  value  of  the  threshold  T  is  given  by  and  the 
maximum value of the output M is the power supply rail. 
A practical Schmitt trigger configuration is shown below. 
 
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The output characteristic has exactly the same shape of the previous basic configuration, and the 
threshold values are the same as well. On the other hand, in the previous case, the output voltage 
was  depending  on  the  power  supply,  while  now  it  is  defined  by  the  Zener  diodes  (which  could 
also be replaced with a single double-anode Zener diode). In this configuration, the output levels 
can  be  modified  by  appropriate  choice  of  Zener  diode,  and  these  levels  are  resistant  to  power 
supply  fluctuations  (i.e.,  they  increase  the  PSRR  of  the  comparator).  The  resistor  R
3
  is  there  to 
limit the current through the diodes, and the resistor R
4
 minimizes the input voltage offset caused 
by the comparator's input leakage currents (see Limitations of real op-amps). 
Schmitt trigger with two transistors 
In the positive-feedback configuration used  in the  implementation of a Schmitt trigger,  most of 
the  complexity  of  the  comparator's  own  implementation  is  unused.  Hence,  it  can  be  replaced 
with two cross-coupled transistors (i.e., the transistors that would otherwise implement the input 
stage of the comparator). An example of such a 2-transistor-based configuration is shown below. 
The chain R
K1
 R
1
 R
2
 sets the base voltage for transistor T2. This divider, however, is affected by 
transistor T1, providing  higher  voltage  if T1  is open. Hence the threshold  voltage  for switching 
between the states depends on the present state of the trigger. 
 
For NPN transistors as shown, when the  input voltage is well  below the shared emitter voltage, 
T1 does not conduct. The base  voltage of transistor T2 is determined by the  mentioned divider. 
Due to negative feedback, the voltage at the shared emitters must be almost as high as that set by 
the  divider  so  that  T2  is  conducting,  and  the  trigger  output  is  in  the  low  state. T1  will  conduct 
when  the  input  voltage  (T1  base  voltage)  rises  slightly  above  the  voltage  across  resistor  R
E
 
(emitter voltage). When T1 begins to conduct, T2 ceases to conduct, because the voltage divider 
now provides lower T2 base voltage while the emitter voltage does not drop because T1 is now 
drawing current across R
E
.  With T2  now not conducting the trigger has transitioned to the high 
state. 
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With the trigger now in the high state, if the input voltage lowers enough, the current through T1 
reduces, lowering the shared emitter voltage and raising the base voltage for T2. As T2 begins to 
conduct, the voltage across R
E
 rises, further reducing the T1 base-emitter potential and T1 ceases 
to conduct. 
In the high state, the output voltage is close to V+, but in the low state it is still well above V. 
This  may  not  be  low  enough  to  be  a  "logical  zero  "  for  digital  circuits.  This  may  require 
additional amplifiers following the trigger circuit. 
The circuit can be simplified: R
1
 can be replaced with a short circuit connection, connecting the 
T2 base directly to the T1 collector, and R
2
 can  be taken out and replaced with an open circuit. 
The key to its operation is that less current flows through R
E
 when T1 is switched on (as a result 
of  input current into its base) than when T1  is off, because turning T1 on turns T2 off, and T2, 
when  on,  provides  more  current  through  R
E
  than  does  T1.  With  less  current  entering  R
E
,  the 
voltage across it will be lower, and so once current gets going into T1, the input voltage must go 
lower  to  turn  T1  back  off  as  now  its  emitter  voltage  has  been  lowered.  This  Schmitt  trigger 
buffer can also be turned into a Schmitt trigger inverter and another resistor saved in the process, 
by replacing R
K2
 with a short connection, and connecting V
out
 to the emitter of T2 instead of its 
collector. In this case however, a larger value of resistance should be used for R
E
 as it now serves 
as  the  pull-down  resistor  on  the  output,  lowering  the  voltage  on  the  output  when  the  output 
should be low, instead of a serving as only a small resistance which is only intended to develop a 
small voltage across it that actually adds to the output voltage when it should be at a digital low. 
Applications 
Schmitt  triggers  are  typically  used  in  open  loop  configurations  for  noise  immunity  and  closed 
loop positive feedback configurations to implement multivibrators. 
Noise immunity 
One  application  of  a  Schmitt  trigger  is  to  increase  the  noise  immunity  in  a  circuit  with  only  a 
single  input  threshold.  With  only  one  input  threshold,  a  noisy  input  signal  near  that  threshold 
could  cause  the  output  to  switch  rapidly  back  and  forth  from  noise  alone.  A  noisy  Schmitt 
Trigger input signal near one threshold can cause only one switch in output value, after which it 
would have to move beyond the other threshold in order to cause another switch. 
For  example,  in  Fairchild  Semiconductor's  QSE15x  family  of  infrared  photosensors
[3]
,  an 
amplified  infrared  photodiode  generates  an  electric  signal  that  switches  frequently  between  its 
absolute lowest value and its absolute highest value. This signal is then  low-pass filtered to form 
a  smooth  signal  that  rises  and  falls  corresponding  to  the  relative  amount  of  time  the  switching 
signal is on and off. That filtered output passes to the input of a Schmitt trigger. The net effect is 
that the output of the Schmitt trigger only passes from low to high after a received infrared signal 
excites the photodiode for longer than some known delay, and once the Schmitt trigger is high, it 
only moves low after the infrared signal ceases to excite the photodiode for longer than a similar 
known  delay.  Whereas  the  photodiode  is  prone  to  spurious  switching  due  to  noise  from  the 
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environment,  the  delay  added  by  the  filter  and  Schmitt  trigger  ensures  that  the  output  only 
switches when there is certainly an input stimulating the device. 
 Devices that include a built-in Schmitt trigger 
As discussed in the example above, the Fairchild Semiconductor QSE15x family of photosensors 
use  a  Schmitt  trigger  internally  for  noise  immunity.  Schmitt  triggers  are  common  in  many 
switching circuits for similar reasons (e.g., for switch debouncing). 
The  following  7400  series  devices  include  a  Schmitt  trigger  on  their  input  or  on  each  of  their 
inputs: 
-  7413: Dual Schmitt trigger 4-input NAND Gate 
-  7414: Hex Schmitt trigger Inverter 
-  7418: Dual Schmitt trigger 4-input NAND Gate 
-  7419: Hex Schmitt trigger Inverter 
-  74121: Monostable Multivibrator with Schmitt Trigger Inputs 
-  74132: Quad 2-input NAND Schmitt Trigger 
-  74221: Dual Monostable Multivibrator with Schmitt Trigger Input 
-  74232: Quad NOR Schmitt Trigger 
-  74310: Octal Buffer with Schmitt Trigger Inputs 
-  74340: Octal Buffer with Schmitt Trigger Inputs and three-state inverted outputs 
-  74341: Octal Buffer with Schmitt Trigger Inputs and three-state noninverted outputs 
-  74344: Octal Buffer with Schmitt Trigger Inputs and three-state noninverted outputs 
-  74(HC/HCT)7541 Octal Buffer with Schmitt Trigger Inputs and Three-State Noninverted 
Outputs 
-  SN74LV8151 is a 10-bit universal Schmitt-trigger buffer with 3-state outputs 
A number of 4000 series devices include a Schmitt trigger on inputs, for example: 
-  4093: Quad 2-Input NAND 
-  40106: Hex Inverter 
-  14538: Dual Monostable Multivibrator 
-  4020: 14-Stage Binary Ripple Counter 
-  4024: 7-Stage Binary Ripple Counter 
-  4040: 12-Stage Binary Ripple Counter 
-  4017: Decade Counter with Decoded Outputs 
-  4022: Octal Counter with Decoded Outputs 
-  4093: Quad Dual Input NAND gate 
Dual  Schmitt  input  configurable  single-gate  CMOS  logic,  AND,  OR,  XOR,  NAND,  NOR, 
XNOR 
-  NC7SZ57 Fairchild 
-  NC7SZ58 Fairchild 
-  SN74LVC1G57 Texas Instruments 
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-  SN74LVC1G58 Texas Instruments 
Use as an oscillator 
A  Schmitt  trigger  is  a  bistable  multivibrator,  and  it  can  be  used  to  implement  another  type  of 
multivibrator, the relaxation oscillator. This is achieved by connecting a single resistorcapacitor 
network  to  an  inverting  Schmitt  trigger   the  capacitor  connects  between  the  input  and  ground 
and  the  resistor  connects  between  the  output  and  the  input.  The  output  will  be  a  continuous 
square wave whose frequency depends on the values of R and C, and the threshold points of the 
Schmitt  trigger.  Since  multiple  Schmitt  trigger  circuits  can  be  provided  by  a  single  integrated 
circuit (e.g. the 4000 series CMOS device type 40106 contains 6 of them), a spare section of the 
IC can be quickly pressed into service as a simple and reliable oscillator with only two external 
components. 
 
Output and capacitor waveforms for comparator-based relaxation oscillator. 
For example, the comparator-based implementation of a relaxation oscillator is shown below. 
 
Here, a comparator-based Schmitt trigger is used in its inverting configuration. That is, the input 
and  ground  are  swapped  from  the  Schmitt  trigger  shown  above,  and  so  very  negative  signals 
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correspond  to  a  positive  output  and  very  positive  signals  correspond  to  a  negative  output. 
Additionally, slow  negative  feedback  is added with an  RC  network. The result, which  is  shown 
on the right, is that the output automatically oscillates  from  V
SS
 to V
DD
 as the  capacitor charges 
from one Schmitt trigger threshold to the other. 
Yviuv_tiov tovoioto  
The  UJT  as  the  name  implies,  is  characterized  by  a  single  pn  junction.  It  exhibits  negative 
resistance characteristic that makes it useful in oscillator circuits.  
The symbol for UJT is shown in fig. 1. The UJT is having three terminals base1 (B1), base2 (B2) 
and emitter (E). The UJT is made up of an N-type silicon bar which acts as the base as shown in 
fig. 2. It is very lightly doped. A P-type impurity is introduced into the base, producing a single 
PN junction called emitter. The PN junction exhibits the properties of a conventional diode.  
  
  
 
  
                Fig. 1 
 
                            Fig .2  
A complementary UJT is formed by a P-type base and N-type emitter. Except for the polarity of 
voltage and current the characteristic is similar to those of a conventional UJT.  
A simplified equivalent circuit for the UJT is shown in  fig. 3. V
BB
 is a source of biasing voltage 
connected  between  B2  and  B1.  When  the  emitter  is  open, the  total  resistance  from  B2  to  B1  is 
simply the resistance of the silicon bar, this is known as the inter base resistance R
BB
. Since the 
N-channel  is  lightly  doped,  therefore  R
BB
  is  relatively  high,  typically  5  to  10K  ohm.  R
B2
  is  the 
resistance between B2 and point a', while R
B1
 is the resistance from point a' to B1, therefore the 
interbase resistance R
BB
 is  
R
BB
 = R
B1
 + R
B2
  
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                                                              Fig. 3 
The  diode  accounts  for the  rectifying  properties  of  the  PN  junction.  V
D
  is  the  diode's  threshold 
voltage. With the emitter open, I
E
 = 0, and I
1
 = I 
2
 . The interbase current is given by  
I
1
 = I
2
 = V
BB
 / R 
BB
 .  
Part of  V
BB
  is  dropped  across  R
B2
  while  the  rest  of  voltage  is  dropped  across  R
B1
.  The  voltage 
across R
B1
 is  
V
a
 = V
BB
 * (R
B1
 ) / (R
B1
 + R
B2
 )  
The ratio R
B1
 / (R
B1
 + R
B2
 ) is called intrinsic standoff ratio  
 = R
B1
 / (R
B1
 + R
B2
 ) i.e. V
a
 =  V
BB
 .  
The ratio  is a property of UJT and it is always less than one and usually between 0.4 and 0.85. 
As long as I
B
 = 0, the circuit of behaves as a voltage divider.  
Assume  now  that  v
E
  is  gradually  increased  from  zero  using  an  emitter  supply  V
EE
  .  The  diode 
remains  reverse  biased  till  v
E
  voltage  is  less  than    V
BB
  and  no  emitter  current  flows  except 
leakage current. The emitter diode will be reversed biased.  
When v
E
 = V
D
 + V
BB
, then appreciable emitter current begins to flow where V
D
 is the diode's 
threshold  voltage.  The  value  of  v
E
  that  causes,  the  diode  to  start  conducting  is  called  the  peak 
point voltage and the current is called peak point current I
P
.  
V
P
 = V
D
 +  V
BB
.  
 
 
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Uni-junction transistor  
The  graph  of  fig.  4  shows  the  relationship  between 
the  emitter  voltage  and  current.  v
E
  is  plotted  on  the 
vertical  axis  and  I
E
  is  plotted  on  the  horizontal  axis. 
The  region  from  v
E
  =  0  to  v
E
  =  V
P
  is  called  cut  off 
region  because  no  emitter  current  flows  (except  for 
leakage). Once  v
E
 exceeds the peak point voltage, I
E
 
increases, but v 
E
 decreases. up to certain point called 
valley  point  (V
V
  and  I
V
).  This  is  called  negative 
resistance  region.  Beyond  this,  I
E
  increases  with  v
E
 
this is the saturation region, which exhibits a positive 
resistance characteristic.  
The  physical  process  responsible  for  the  negative 
resistance  characteristic  is  called  conductivity 
modulation. When the v
E
 exceeds V
P
 voltage, holes from P 
emitter  are  injected  into  N  base.  Since  the  P  region  is 
heavily  doped  compared  with  the  N-region,  holes  are 
injected to the lower half of the UJT.  
 
Fig. 4  
The  lightly  doped  N  region  gives  these  holes  a  long  lifetime.  These  holes  move  towards  B1  to 
complete  their  path  by  re-entering  at  the  negative  terminal  of  V
EE
.  The  large  holes  create  a 
conducting  path  between  the  emitter  and  the  lower  base.  These  increased  charge  carriers 
represent  a  decrease  in  resistance  R
B1
,  therefore  can  be  considered  as  variable  resistance.  It 
decreases up to 50 ohm.  
Since    is  a  function  of  R
B1
  it  follows  that  the  reduction  of  R
B1
  causes  a  corresponding 
reduction in intrinsic standoff  ratio. Thus as  I
E
 increases, R
B1
 decreases,   decreases, and 
V
a
 decreases. The decrease in V 
a
 causes more emitter current to flow which causes further 
reduction  in  R
B1
,  ,  and  V
a
.  This  process  is  regenerative  and  therefore  V
a
  as  well  as  v
E
 
quickly  drops  while  I
E
  increases.  Although  R
B
  decreases  in  value,  but it  is  always  positive 
resistance.  It  is  only  the  dynamic  resistance  between  V
V
  and  V
P
.  At  point  B,  the  entire 
base1  region  will  saturate  with  carriers  and  resistance  R
B1
  will  not  decrease  any  more.  A 
further increase in I
e
 will be followed by a voltage rise.  
The diode threshold voltage decreases with temperature and R
BB
 resistance increases with 
temperature because Si has positive temperature coefficient.  
 
 
 
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Uni-junction transistor  
UJT Relaxation Oscillator:  
The  characteristic  of  UJT  was  discussed  in  previous  lecture.  It  is  having  negative  resistance 
region. The negative dynamic resistance region of UJT can be used to realize an oscillator.  
The circuit of UJT relaxation oscillator is shown in fig. 1. It includes two resistors R
1
 and R
2
 for 
taking two outputs R
2
 may be a few hundred ohms and R
1
 should be less than 50 ohms. The dc 
source V
CC
 supplies the necessary bias. The interbase voltage V
BB
 is the difference between V
CC
 
and the voltage drops across R
1
 and R
2
. Usually  R
BB
  is  much  larger than R
1
 and R
2
 so that V
BB
 
approximately  equal to V. Note, R
B1
 and R
B2
 are inter-resistance of UJT while R
1
 and R
2
  is the 
actual resistor. R
B1
 is in series with R
1
 and R
B2
 is in series with R
2
 .  
 
                                    Fig. 1  
As  soon  as  power  is  applied  to  the  circuit  capacitor  begins  to  charge  toward  V.  The  voltage 
across C, which is also V
E
 , rises exponentially with a time constant  
 = R C  
As  long  as  V
E
  <  V
P
,  I
E
  =  0.  the  diode  remains  reverse  biased  as  long  as  V
E
  <  V
P
  .  When  the 
capacitor  charges  up  to  V
P
  ,  the  diode  conducts  and  R
B1
  decreases  and  capacitor  starts 
discharging. The reduction in R 
B1
 causes capacitor C voltage to drop very quickly to the valley 
voltage V
V
 because of the fast time constant due to the low value of R
B1
 and R
1
. As soon as V
E
 
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drops  below  V
a
  +  V
D
  the  diode  is  no  longer  forward  biased  and  it  stops  conduction.  It  now 
reverts to the previous state and C begins to charge once more toward V
CC
 .  
The emitter voltage is shown in fig. 2, V
E
 rises exponentially toward V
CC
 but drops to a very low 
value  after  it  reaches  V
P
.  The  time  for  the  V
E
  to  drop  from  V
P
  to  V
V
  is  relatively  small  and 
usually neglected. The period T can therefore be approximated as follows:  
 
Fig. 2 
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Uni-junction transistor  
There  are  two  additional  outputs  possible  for  the  UJT  oscillation  one  of  these  is  the  voltage 
developed at B1 due to capacitor discharge while the other is voltage developed at B2 as shown 
in fig. 3. 
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When  UJT  fires  (at  t  =  T)  V
a
  drops,  causing  a 
corresponding  voltage  drop  at  B2.  The  duration  of 
outputs  at  B1  and  B2  are  determined  by  C  discharge 
time.  
If  R
1
  is  very small, C  discharges  very quickly and very 
narrow  pulse  is  produced  at  the  output.  If  R
1
  =  0, 
obviously no pulses appear at B1.  
If R
2
 = 0,  no pulse  can  be generated at B2. If  R
1
  is too 
large,  its  positive  resistance  may  swamp  the  negative 
resistance  and  prevent  the  UJT  form  switching  back 
after it has fired.  
R
2
,  in  addition  to  providing  a  source  of  pulse  at  B2,  is 
useful  for  temperature  stabilization  of  the  UJT's  peak 
point voltage .  
V
P
 = V
D
 +  V
BB
.  
As  the  temperature  increases,  V
p
  decreases.  The 
temperature  coefficient  of  R
BB
  is  positive.  R
s
  is 
essentially  independent  of  temperature.  It  is  therefore 
possible  to  select  R
2
  so  that    V
BB
  increases  with 
temperature  by  the  same  amount  as  V
D
  decreases.  This 
provides  a  constant  V
P
  and,  in  turn,  frequency  of 
oscillation.  
 
Figure 31.3  
Selection of R and C:  
In the circuit, R is required to pass only the capacitor charging current. At the instant when V
P
 is 
reached;  R  must  supply  the  peak  current.  It  is  therefore,  necessary,  that  the  current  through  R 
should be slightly greater than the peak point.  
 
Once  the  UJT  fires,  V
E
  drops  to  the  valley  voltage  V
V
  .  I
E
  should  not  be  allowed  to  increases 
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beyond the valley point I
V
, otherwise the UJT is taken into saturation region and does not switch 
back, R therefore must be selected large enough to ensure that  
 
As long as R is chosen between these extremes, reliable operation results.  
 
 
 
 
 
 
 
 
 
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