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Thomson Moclel of Atm
Rutherford 's X- vou Scattering.
Distemce of Closest Approach
Impact Poramedter
Rutherford'!s Atom Mockef
Limi tation ob Rutherford 's
Atom model
Boh mock} of hyclrogen Ahm
Radius of Bohr's Stedionary Orbits
Velocity of eleehon fn Bohr's
Stotionanp orbit
Freguen of electron in Behr's
Stodiondny Ft
Total ener: of; elechor, in Bohr's
Stodionory orbi +
Onigin Of Spectyal Lines
Bohy's Explanction of specs-roul
Series. of Hydsegen — cutem
Enagy Level Lagram
De Byogtie's Explancition of Bob's
second postulede ot Quantizodion
Very. FEmportent QuestionsIn this Unit, we. Shall discuss the models
of atoms in Some cletoi). The first Contr bution
in Wis regarcl come from Deabion, who proposect
that matter is mace of atoms, een are indivisible
I.I. Themen proposes! a See foy the atom,
which JS mooalifieo! by Rutherford amd Later by
Niels Bohy-
Thomsen Model of Atom-
Accorcling to (ely “change moole}, every,
atom comist of @ positively chy s phone of
ACKUA Of the orc of To!’m in mgeel pe entire.
mars anol positive change of the cutom ake Uniform,
iatributted, Tnsiole. this sphare, the -elechons ane
embeded Like seady in a woteameln.or Uke
plums in a pudloling. The number of electron is such
thet +Hhreiv n o ee 4b eortol to the
positive. charge m. Thus the atom dd
elechically tt
a of Thomson Atom moolel -
(1) It Could not explain te
Owigin of Spectre Serer of
iy and other atoms,
obseaveal experimentally.
Gi) Tt Corl not explain He
ane scoHfering of x-
particles” from thin “meted
foils, a4 observed by Rutherford.Rutherfordis d-ray Scattering Experiment :
The cepenimendn| Setup used by Ruther ford
and hia Collaborators, Geiger and Marsden +s
Shown in Pig -
~s
~
‘
COLLIMATOR [=] \
OLD FOIL),
(10-8m thick) 4—» MOST-o
anne 4 pass
~Je “> STRAIGHT
7 ay
/ y 7 SCREEN
CAVITY J i] SS
ABOUT 1 in 8000-c a econ
IS REFLECTED BACK GerectORy
S 38 @ pleca of radioactive Source (es87'")
Contained in a deadl Covity. The X- particles emitted
by the Source are Collimated into a narnowo beam
with the help of @ lead slit ( Collimator).
The Collimated beam Gs allowed to fall om
a thin gold foil of thickness of the oxder of 2IxIOm.
The a particles Scottered in ifferent clivections are.
observed trv Q vrotetable. oletector Consisting of
a zine sulbh Screen and a micwscepe:
The A- particles produce bright flashes on the
ZnS Screen. These are observed in the microscope
and Countes! at U angles from the clirection
of incidence of the beam- Tre angle © of cteviation
of an a- particle from dts original olivection is Called
JAS Scocttering angle. e.Observations ~ a graph ud plotted between the
Scattering angle @ and the number of X- particles
N, Scattered at £0 for a large number of A- particles,
we find that - '
i) Most of the &- particles {s
pars shralginr throu ‘c!
the gold foil. Tt means 2
olo not Suffer any ,
3
caliision with gold atoms. 5
(ii) about 014% of git
ind a- particles statler 20 40 60 80 100 120 140 160 180
by more. than I. SCATTERING ANGLE (0°) =emmo-
Wii) About one A- particle in every Bo00 porticles
aftects by move than 3¢-
Ex planation - '
————_ Am a- partie 44 over Too mohe
massive than an elechon, and vin this experiment,
A- particle is travelling ot a high speed ; thureppre,
vey Ateong fore alone” could hove oleflected
Hed Lage angres. Tws Led Ruther foro] to
postulate that the entire positive che af the atom
must be Concentretecl In a tiny centyol Cove of
the abm This ding central Core of each atom
was Calleol atomic Hucleus.
An &-particle Carries two units of positive
and has mass of a@ helium atom, Cc on
gold “nucleus = ze, whe Z of golol iu 79, As gold
nucleus is about So dimes heavier than an x-
particle , we aXsume thot it wold remain stable
in the Scattering Process.Thinepove, the yecto of ~-particle Gan be
Compute uain New ete D haw of motion amd
Coulomb force of repulsion between A~ cle
and gold nucleus ive.
whre ¥ iA the Mistance of A- povcticte tom the
centre of the nucleus. The mi ituole and olivection
of the force on an x~ particle cha Continuously
ab Jt approaches the nuctens first ond then
moves away from at.
—o 8518, ATOMIC
, a NUCLEUS
a {
tt
1
to a
lo 1
INCIDENT & PARTICLES
ON an wo
a
1
As shown in fig an - particle (1) tending
to Collide with the nucleus, slow down clue to
repulsive force of the nucleus, finally stops anal
As then repelleof back. This o- jche. thers fore
vetrar ots peth , Scodterimg prough 180".
The d-paxticles 2 and 2! tendling ao Wit the
nucleus ot ths peeiphiny, experience Shong
vepulaive force andl qe 1 eadtened through lange
angles (67390).
The &- particles Zand 2, which pass at a
stance from the nucleus experience small repulsive
forts ond get scattered trough small lea.The x-porticles which pars at Large olistances
fem the nucleus gr almost undeviated.
We Can show that the number af x - Particles
Scattered per unit awa NCO) cb Scattering angle
@ varies inwersely or Sint (2):
NW) % —SntCEy
Distance of Closest Approach -
tohen & - particle 4k divectec! towards the
nucleus , the Kinetic energy of A- particle goes on
olecreasing and mm twen electrical p lod
es on increasmg due 40 Coulomb’s repulsive force
between nucleus and oX- particle.
At a cartein clistance v from the nucleus,
KE. ef o- particle reduces to )
Impact Payameter ( b) -
ines] AA the Perpendicular distance
Tt js
of the inital velocity of « “porticie | & from tHe
Central Une of tre nucleus , when the particle
4h for Cuno pom the nucleus.
VELOCITY
VECTOR OF
@ PARTICLE
fe
cenRACONE ~~
0 DISTANCE (fm) =m TARGET
NUCLEUS:
When the im pact eee As Jonge 5 an
A - particle wil) cleviots a much smaller angk-
pear when impact p 48 Amal , force
perienced aa | and the a- particle oil Scatter
Hough a dange angle.
Rutheforol Coleuloted ana ically the velotion
between the im pact Fete fs Scattering angle
8, which wu given by-
1 z t 8 a
b = aes ES Cot fr [Re= amv ]Rutherforels Atom Model -
CL) Every atom Consist of a tiny central Core,
Called tre atomic nuceus In which the entire
positive charge and almost entire mars of the
atom are Concentrated.
@) The size of the nucleus ws of tre order of 10,
which 2s Amal a& Com parsol fo the size of
the atom whith is of the oreler of Jom.
@) The atomic nucleus is a number of electon’. As
atom ids electric: neutral, the total negocive
change. of elechons Aurrounding He nucleus 4s
equa} to toted positive. change ox the nucleus,
(4.) These elechons revolve around the nucleus in
Various civeuteord orbits. Tae cercripeted force
required by elechon for revolution is provided
by the electrostectic force ef attracton between
eechonA and the nuclens.
Enevay of the electyon in orbit -
Let Fe? Centripetal force requires) 4O Keep Q
revolving elechon in orbit
fe = elechostactic foree of cttraction behven the
revolving eaeckon and the nucleus
then for a narically Stoble orbit in @
hygchogen ete.
Fe — Fe
mv2>_._e-e > a. 22
¥ ATC Y= UA Amer
KrE. of the electron in the orbit = Le myv>Hence KE =e?
Be ¥
Potential encrgy of electron in orbit-
U = ece - -e2r
4N EY 4TLeG.¥
'. Total energy of eleehon in hurohagen atom —
E+ KE tU
ce =e et
SM En¥ ATILGoY
ov e = -<&
BMleor
Hence the Jotal energy of electron in orbit of
hydro atom is negotive. Hence, the electon ta
bound do the nucleus fe. the elechon +s not free
to eave the orbit around the nucleus.
Limitation of Rutherford Atom Model-
OD Accorcling to the Classical
EM theory, the revolving. Gechons
must yaoliokr energy in the fom
of EM Waves. As vewolvin elechon,
Loses continuously . it must é
spivod inwards and fin
into the nucleus but as” mattir
4A Atoble, we Cannot expect the
atoms sto Collapse-
Gi) As +e revolving elechons spival inwards, Heir
angular Velockties “ond hence tiv frequencies of
yewolution would chomge Continuously - Theredpre frequency
of EM Waves emitted must change Continuowsly.re , efoms shoud emyt continuous spectrum
but we observe ony a dine spectrum.
Bohyv Moeel of Hyclrogen Atom-
There ane three baaje postulates of +hia modif—
Q) Ev ator Consist of & cental core Coho!
nucleus, In which entire positive chi ond
almost entire mass. of the atom aw concentrated.
A surtoble number of “electrons revolve around
the nucleus in cive orbits. The cenhipehal
fore required for revolution is provided by the
elechrostatic forte of attraction between the Elechnn
and the nucleus.
Centripetal fore = Electrostatic fore. of attraction
my = LL. (222)
r a ad
ve mv= . Kzer k= Yaneo
~~ Oe zeLl
(2) A ccoroling ao Bohs, electron Can evelve. only
in certain ‘chscrets non radiating oxbits 4
Stodionareg orbits, for Which total angulor momentum
of the Awolving electron is an integral muttiple
of ham, whare” h ia plank's Constant.
Thus the argular momentum of a orbiting electron
44 quantised,
Here 1 ud Callecl principle Puantum number,
* The ehechon, while vevolving in such orbits,
Shell not tose enwrgy C-2- dts enngy woutel
Ste Constant.(3) The emission / absorbtion of vy ccs only
when an elechon PS form one $ ts S Specified
non - Yactlaking ‘ae Another - Hi fferance
in the ‘otal enon:
oy elechon in nthe tuo orbits
JA absorbec} cohen" the elechon jumps from an
immer #0 an outer. orbit amd emitted whin eketon
jumps from outer 4o the inner orbit.
hv = &-&
OCWAL VY As the uLn °
f yaciotinn emitted on
Jumpin: mm outer do! Inner orbit of eng
E. oa fr respectively.
Radius of @Behr's stationary Orbits—
We Know that for Atotion oy orbits -
= mh =n
Case ia oor,
By puting, the value of v in ray = ze?
> Mx We = Kzer
vr arch m* >
ye
= nthe = for hyehogen adem
470 mKe’ Ze
Tt shows tot - ran”
ce the raclius of stocionary, orbits ane in
a yatio 13 2S and so on be LiWi Glow.
cleanly the stodionany, orbits are not equally spaced.Velocity of electron in Bohr's Stationary Orbit -
As we Know that - _mv> = kze?
Yr re
ov y = kze> — )
mv>
and also y =_nh — ©)
atmv
by equation U1) and (2) we get —
Kze> =. nh 2 21kzer
mv? 2ITmMV or v nh
ana
As Vx+> hence the ovbited velocity of electron in
outer. orbits is smaller as compartol “do its Value in
the inner orbits:
Frequency of electron in Gohr's Stationary orbit -
Tt is the number of vewolutions completeo! per.
Secor by the ekcton In a Stationary orbit, araumd
the. nucleus. It is represented by vy.
As Vz rw = r(oanv)
ype = 2m kte2 = KzeX
ane rth: 27tr nhr
Kze®
> |v
The frequency of election in subsequent stationary
orbits 4s smallA as v «xt -Total Energy of electron in Gohr's Stationary Orbit
Kinetic. energy of election revelving ina stedionasy,
orbit is -
1 - 2 by .mv>. kze™
KG. of electron = Smv* = Se [*s ie
Potential energy of elechon = Potential x Change
PE. of electron = Kzex(-e) = —Kze>
Yr Y
Tote energy of electron in the orbit -
E = KE. + PE.
Ee: Lkze* _ Kze> = ~ kee?
2 -> + ar
by putting = _nth™ we. _
d 4 477m kze> at
E = -_20mk*zet
we
by Substituting the Standard values, we get
€ = -13-6 ey eat
n rn
Hence the toto) enrgy of elethon in aq stati orbit
ad ive, whith means thet the electron is beled to
the nucleus and ia not free to teave it
* when n=L then this state of lowest enngy of
the. atom Jb Cotbed groundl stoke. The enngy of this
stat. HSE, = -I3-6ey.
* > the minimum enngy required do pree, the
electron from the ground stote of hydrogen atom 48 I3Gev.
This id Called ionisation energy of hydrogen odom.* As n increases, the value of negective energy
clecreased be encrgy Ks progressiv' Jangex me
the outer orbits. es preg “y
Origin of Spectral Lines —
At room Lumperoture., most of the hyetrogen atoms
axe in ground state. when a hyclogen ator Yeevives
erurgy q proasses Auch as aldcheh ‘collisions or heat,
the atom mou require sufficient energy to yaise the
elechon to heghor @ stots Le from nel do n=2,
3,u,.-.. The atom CD Abn said tv be in an extited
state -
E2 —> PHOTON
~ Ay
From Hure excited statis, the elechon can fall
hack 40 a state of tower energy and emitting a photon
of particular energy (= olifference t enurgies of, the
fe stoter )). 7 tf 7 ong 4
Let E, and €, are the total of elechon
in the inner and outer orbit reapectivelyy
When an elechon jumps pom an outer. 40 an innex
orbit , the enrigy of radiation emitted Js giren by
hv = €,-€,
hv = _27?mk72et Fa a
we ne 7 |
he = _an?me eet Ft
a re nooor 2 2 _anmektete? PL
A on ne ne
Now avs Where VY Ub te wave numb of
radiation emitted -e. number of Complete wave in unit
Langth. stim whet
and = 2nmke = R (Rydberg Constant’)
or R = 1037 x10" m*
= zi _i
Hence P:R at” ve] For hydrogen
fo ne =n
Above. equation us called Rydberg formula for the
Spectrum of hyerogen otem.
*% By above formula tt ia Clear that wavelength /
frequencies [weve numbers of yadichions emith by
the excitedt hyelrogan atom ore not Continuous.
Thay hove specific valu» cupending upon the values
of Yn and no.
* Frequency of radiation emitted cohen the atom
makes transition from the higher ena gy Stote
(m2) +o the bwer energy. Atodz C1) —
vr &£& > 14
a v= Rela a3][Q) Find the watio of enngies of photons produad
SEE clue 40 teamition ef am electon of huplrogen acm
abs (a) Setond permittect energy Lvel 40
the fist Loved (b> the halghust peemittes| energy
Lavel “to Hie pirat permitted Jewel.
Sel. (4) Enengy of Photon released = E,-E;
= -3.4 = (-13-6) =lowev
(6b) The heighest permitted ei dwel to the first
wget es URSA fis
peemrtt = Ea- E,
= © - (13:6) = Iséev
Rokio o enuagies ek Photon = 1Je2 = @
b b 13-6 q
What is the ratio of radius of the ovbits
S§Er Coreaponoling to fist excited stat. and Grund
Stoke In a hyelrogen atem 7
Sol. For fivst excited stole N= 2
Groumd stot occuns for n= 1
y an?
Henee Y1 sf{mP = (zy
% (Ft) (+)
Wiw = 4tl
Gl Re wdiws of innermost elechon orbit of 4
CBE hydro atom 3s $:3K10" m, Wheat Js the mmdius
of orbit in the Second excited sto ?
Sek The radius of atom whose PHnciple Guantum
number JA v1, us given Yann
Hore ¥% Jb Yaclius of Mnermost’(n=1) orbit .
Fer second excited state n=3
Y = (39x 53x 101! = 4-77 x10 !?m,Bohr's Explanation of spectral series of
Hydyogen = Atom -
bohon an atomic. ox vopour at dow Pressure,
4s excited uasuodly bg ne an electric. Cuiiurt
thw at) the / vapowe emits yadictions of certain
Specific wor 6 This Kind of spectum dd
caltel “Line emission spectrum" and wt consists of 4
few Laight Airts on a clark background.
Detector
photographic plate)
High
voltage
Hydrogen gas
discharge tube
410nm = 434nm 468nm 656nm
bohon the white Lé 4A parsed through the
Same. [Vapour., we observe a ‘bri Lack#round
Cross by a few dark Ling signi ing the: missi
ee aa or “the wavelensth s that” are ahisotbedl
by gs. They form a& “Line absorption Spechum?
It was founcl that missing wav s he He
Same a4 “the wa murent inthe emission
spectrum of the gas / vapour:
Bohr gave Wis theo of byclro ahm about
spectra] seties which had! observ experimentally
by. Voriows Acierttists. Bohr offere| a tHyorelicas
exphnotion of these spectro} series as follows :1. Lyman Series —
Bohr postulotias that Lyman Series is obtained
then an electron jumps to the first orbit Cn, =1)
from any outer. orbst (Nas 2,3,4-...)
Wave numbers 6 ectral Lints o an
seres were Calculodtec de J i
7 ALR-m]] O-28)
These valus of ye Lie in the “Ultra violet region”
of the spectrum.
2. Galmey Series -
Accercling fo Behr, Balmer Aries 3 obtained!
when an electron jumps to the secorel orbit (1,=2)
from omy outer. orbit (Mm = 3,4,5,----
Wave number of theue spectyol Lines were Caleubiteo|
a“ 3 J L
vos a[ 7] (na = 3,405----)
THA Set of Spectral Lines Lie in the visible part
of the spectrum,3. Paschen Series —
According 40 Bohr, Paschan series 4b
obtedinecl eohen om electron Jumps fo the Sx Orbit
(nie 3) from ang outer obit) (n.= 4,5;6,--):
Bohr calculoted the wave number of spectra}
Anes of Paschen sexier from the reletion:
¥ =R[& ~ 4] (nat sie...)
The value Of TF Lie in the infrared region
of the spectrum.
4 Brackett Series-
According to Bohr, Brackett Serien iB
obtained When an eclechon jumps to the 4th
omit C= 4) from ong. outer orbit (m= $6,7---)
Wave number] FF = R[ a ~# | (y= 5167,---)
Brackett Series Was cHidcoverscl Im the infrared
region of the Spectum,
S- Pfunel Series -
Accoroling. Ae Bohr Pfundl senies. 12 obtained
When om clechon jumps to the St orbit (n,=s)
from any outer. orbit (m= 6,7.8,---)
Wave number ve *R[ te = =] Nt 67 Bow
Pfund Sertes wos cHscovercl in the Infmrad region
of the spectrum,Energy Level Diagram -
A clagram which represents the doted
tes of electron in Afferent ee orbits
of em atom is Coblect the energy eR jagpran
In this clagram, total energies of elector
in various stationary orbits axe vepreserted by the
hofizortal
Lines drawn according to Some
Surtable. energy Scakt
E = -Jja¢
n>
putting n=41,2,%,---- We get the ensrgies of
electrons in Vardous Ateckiondarey- orbits as?
2 -IB6 2 Li, in
Ee, ef = 13 cey 5 EL 136 = -syey
2
= IBC 3s
Es see -bsiev 5 Ey = 128 = -OBsev
E - —136 2.6. - (126 2. -oO
sof == z-OSY CV Eo = Ee ese
Clearly ab n increases Ex becomes Luss negothive
until ‘at n=o , Enzo.
f Tre eae devel lagram Ga shown fn
Y fer Ayo! atom.” The height
ion Gorceapsrals co n= 2% and has Qeeoy co
Ths as the of the atom, when the elechon
is vemoyed (v= 00) from the nucleus and the
electron is. at vebl-
E= OePfund series
Brackett series
Paschen series
Balmer series
net
=14-0 Lyman series
* As n Increases energies of the excited state
Come Closer so :
TQ) calculate the waveltngth of Ha Line (nz 3)
cE i Balm series of hydeo odom, given
Rydberg Constant = R= 1.087 X107 m™
Sel: For Balmer Aeries, wavelength is given by-
tf" 4)
for Hx Line 2223, SO thot
eo 77a oa
+ = 1097 Xto ie 4
4 = os2y x07
a
A -—1 = 663 A°
OIS2UY Kpo!Ss Photons , with a corctinuows wee of
PES ane mace +0 pars tio ra hae
The fansitions — Shou hehe 5 diode. Poel
the spectyol absoxption Lines in Tha Coa Conus
spectrum.
° ne00
nes
n=4
-2 x n=3
zr
n=2
(ev) ~4
-6
-s I
-|0
-12
n=Lb
(A) Telentify the ctral sertes ef the ro;
emission spectrum, to which each of these Hee
Lints Corresponds.
(b) Which of these Lines Covrespord s to the
absorption of yadiation ef maximum wavelength 2
Sol.
Sol. Ca) Lst spectrum epresert Lyman series
because, in this Spectrum, elechorn jumps
$OM N=aL Ao N=2,
Inc spectrum epresert Balmar Serits
because im this Spectrum, electron jumps
fom n=2 +o n=3,.
IDvrd Spectrum veprarsents Padchen series
aS tre elechon jumps pam n=% to n=4 in
this Spectrum.
Ce) Spectrod Line Ot (Paschen Series) Grvesponds
to the absoxption of radiation of, Maximum warelergtin.G) @) Te erengy dwiels of an atom ore Shown
cE in fig. vahich of Haem coil result In the
2) emission of a Photon of wavelength 275 nm?
Uo) thich transition Corvesponds 4o emission of
vadiation ef maximum wavelength ?
A ow
© cs -2ey
-tse
—loevy
Sol, (Q) When A= 2TISNM = 27TSKITFM ten
es hv che = 6exisS4x anio®
A 27s x16?
Ee = aS ev
+ Transition B& will veautt in the emission of
photon of Az 27S nm,
(6) Maximum wavelen hos mimimum
Transition A provicles energy of 2ev, coh
4 mynrnum.
De Brg sey Explanation of RBohr's
Second “postulate of Quantization
TRe Second postulate of Bohr model sags thal:
an, momentum of electron orbiting anound the
nucleus iA quardizecl
Le. mvy = Th fohtre = 1,2,3..1
Lous cle Broglie expainec| Hus purale -
Accorcling to de ie, the elechon inits civcular
orbit, a proposed! by Bohr, must be Sean as a particle
wave.We Know thet when a shing hixed ad tun ends
4s plucked, a lenge Number of wavelen are. excited.
But only those “waves which have nodes ot the two
ends from the ‘tondling Waves and Survive.
It means that in Q string, Standing wees
eae when fotal chistance travellicof by a wave down
Atring and back Us ami integer mule ple. of the
pave ¢
Waves With othr wavetengins inters eve With them-
selves upon reflection and r ontbectes vanish
quickly.
Hence according to of Broghke, a stationary
orbit is that bohich Gcortaina arr a fegtol number’ of
de Broglie waves arsociaticl with the revolving. clechon,
For an electron revolving in nth circular orbit of
Yadius Y,
For the permissible oxbit , anv =n
According +o ole Brogli = bh
cco" g to cle rage A 7
tohere. V dd speeol. of clechon revolving In vith orbit
any = nh = =z nh
rm 7 > mvy = nh
230Hence om momentum of elechon revolving in
nth orbit “must be an | multiple of West »
which Js the quantim Cenclition proposes! by Bele
in second postulate.
Limitation of Behr's Theory -
(LD This theory is icoble 40 Simplest atom
dike drogen Noi cl. The ne ells in Case
of atoms of otur elements for cahigh ark.
@) The theory oes not explain why orbits of elechons
one taken as circular , while eMipteal orbits are
also possible»
GB.) Bohr's theo doe not s oO ing about tHe
relodive akersl Hee of spect tal gins
+) Bohr's Hwory coer not take Into account the wave
properties of electrons,Very Important Questions
L Mark Questions-
Ql. Weaibe the expreasion for Bhor's raclius In
WWyetregen outorn Cretki ante , 01)
Q.2. Stote Bhor's quantisation cenditon for
oLapining Stahionory orbits,
C Rese 2008, CBSE 2olo, 03’)
@.3. In the Rutherford scodttering experrment, the
stance. of Closest Approach for an a-particle
is ce. Th x-particle 1s veplaced by a proton,
hovo much Kinetic envrgy in Comparison to 4~
portcle will at require“ to have the. same
distance. of Closest approach clo ?
Hint + Proton CH"), A-Particle (Het) CcBs€ 2003 2000)
Qa. In hyeleo cutom , if the elechon is replaced
by a Pp cle. which 2 206 times heavier bub
Os the Same change, how would rts radius
Change ia CeBSE 2002, 08)
Qa.s- TR mengy of the electron im the und
‘stoke ‘of 3 a odom is +136 ev. a
(er) Whot hoes “the negoctive sign signify ?
(6) How much 4s reguireol to take an
electron in Hate ben Growl the. ground state
to the first excited stat ? eee2 Mark Questions -
QL. The und stode ener. of; dvogen atom
AA -15.6ev, The Photn emitted clu the
tromition of electron from n=2 to net Stodh
is inciclant on the photosensitive Moterial of
Unknown work functOn. The photoelechons ane
emrtted from materials with a maximum
Kinetic energy of Bev. Codcutake the thitsheld
weveltngy of the materiel used,
Answer - As Séles nm. Cease 2008)
Q2, Using. Bohr's postulates for chosen atom,
shove SHhat the -totol eneagy (Ee) of the
electron In the stocion stot, Con be
expresses] ak the Sum of KineHe energy (K)
and potertHed CU), Where Ks -2uU-
Hence oledute the expression for te total
energy In the nth enengy devel ob- bugalrugen
chem. (cRSE 2002, (2)
@.3. CA Using Bhor's seconcl postulate ef quan
tizedon of orbital angutor mementum show
thod the Civeum ference of the eleckon in
tne nto ovbital ctote In hgolro odom is
n dimes the Az-broglie wavelength arxsouated
with th.
(b) The ekectron In agen oto ld inthally
in the third! excitect stat... whet 2b the
maximum number of Spectro Lines vcohich Car
be emitteco| when it finally moves to the
ground Stoke ? ( Pelt 20/2, RBSE 2006)
Answer: (6) 1-23Qu Me und state energy of hydro: octomn
is eee If an checked pleas! Q@ Srransrtion
fom om e Aurel ~0- 85 ev Fo -1S1L eV,
Codculete the ~ wavelen, of the Spechal Une
emitter To which Series of hyolregen spechum
aows this woavelengty belong ?
(casE 2001, 12)
Qs. Ina Geiger Marsden experiment colcutate tre
Autonce of Closeat approach to the nucleus
of Z=Bo, When om o- particle of Bmev enngy
Incident on it befpre Jt Comer reat and reverse.
its direction:
How udll the dustance of closest approach be.
affect-ed when the Kinehic energy of the a-
partde is cloubled Cense 2003, 09)
Anawer- So = 2-88 K10!2 mm '
Qb, Stedt the baste assumptions of the
Rutherford model of the otom. Explain in brief
why +Hhis mock con not account wv the Stability
of “an atom ? CDelhi 200 2,10)
@-1 Using the Bohr's postulotes, olerive He
expression for tHe —
(a) Speect of the electron im the nth orbit,
(eo) radius of the nt arbit of tHe elector
in Wydregen dom, CR@se 2007, 10)
G8. Tae OF the elechon in the groundl
Stott of Ja 136 ev, Coleutode the
energy of He p trod woutd be emitted
if} the elechon weu do make a transition
Corresponeling. to the emission of the fivat
Link of the (a) Lyman series
(b) Bodmer seniera of Hw hydro; ectrum
Arswe- (a) lozev (bd 1.9 i) aa eae 20eg)@8. Re Und stock. ©. dx otom
Te ts emenyd of leystregen
Ca) Lohot 4a the KE. of an elect in the 24
excites| stecte?
(b) Th the elechon jumps to the ground stotte
the 2nd excited stote, colewlate the
wavelenety ef the spectral tine emitted.
Pmawer ©) Sev (b) A= 10304 (cease 2003, 08)
Blo. The energy duels of an atom ate @
shoon jn Sige beled
2 oev
£ D -2ev
-4-s5ev
-loev
lei) Which of trem will weautt in the transition
of a photon of wavelength 21s nm 2?
() which transition Covvespors to emission of
radiation of maximum wav 2
Answer: (a4) tramiton B Ce@se 2eol; 09)
(od transition A.
Qu Ca) Usin Atulotes of Bhoris Heo Q
hyetrogen hee, show ies me ot
Ci) The tadius of obits increase as n>
Gi) The total energy of the elechon Increases
Ob Sm vole n Js the pAlndpal quantum
number of the atm.
(6) Codeulode the wavelength of Ha dine in
Balmer series of hydro: otom, given that
—l
Ryolberg Constant = 1-097 x107 m7.
Amswe- (b) A = 6563 AY ‘(case 2002, 06)