Atomic Structure and Discoveries
Atomic Structure and Discoveries
Atomic Structure
                                 Planck's                  SWE
                                 Quantum
         Rutherford’s             Theory
            Model
                                                                 Heisenberg’s
                                            de Broglie’s          Uncertainty
                        Bohr’s              hypothesis             principle
                        Model
J.J. Thomson’s
     Model
          Discovery of electron
Cathode rays
Cathode Anode
Cathode Anode
High voltage
 generator                       To Vacuum
                                   pump
                           Discovery of electron
 Observation and Characteristics
5. Cathode rays are deflected in          6. Cathode rays are deflected in
the presence of an electric field.       the presence of a magnetic field.
Anode + Anode
                                     Cathode
Cathode
                       -
   Discovery of electron
         Conclusions
                                                Anode   +
● Measured the charge (e) to mass
                                      Cathode
  (m) ratio of an electron.
● Electric & magnetic fields
  were applied perpendicular to
  each other & to the path of
  electrons
                                                        -
  e
  m       =    1.758820 × 1011 C/kg
Charge to mass ratio
Nature of        Material of
 the gas          Cathode
James Chadwick
     4             9               12           1
     2
       He++   +    4
                     Be            6
                                     C     +    0
                                                  n
             Raisin
            pudding
             model
 Plum
pudding               Watermelon
 model                  model
                          Thomson’s Model
                                                               Drawback:
Negatively                             Positively
Charged                                                 Not consistent with the
                                     Charged Matter
Electrons                                             results of later experiments
              Rutherford’s Experiment
Radioactive                                          ZnS
  Source                                            Screen
      Gold Foil
Observations of Rutherford’s Experiment
Gold Atoms
                 Nucleus
Observations of Rutherford’s Experiment
     1. Most of                                           4. Small
        them                 𝞪–particles               fraction was
      passed                                           deflected by
    undeflected                                         small angles
                                        3. Very few
                  2.Very small
                                           were
                  fraction was
                                       deflected by
                  deflected by
                                         180° (∼1 in
                  large angles
                                          20,000)
   Observation            Conclusion
 Most 𝞪-particles
                       Presence of large
passed through the
                         empty space
    foil without
                          in the atom.
    deflection.
                       Positive charge is
 Few 𝞪-particles
                       concentrated in a
were deflected by
                       very small region.
  small angles.
                       Small positively
Very few 𝞪-particles
                       charged core at
   (∼1 of 20,000)
                         the centre.
 deflected at 180°.
                     Nucleus
 Atom consists of
a small positively             It has negligible
 charged core at                     volume
the center which               compared to the
carries almost the                   volume
   entire mass                    of the atom.
   of the atom
                                  Nucleus
nucleons.
Nucleus is surrounded by
  revolving electrons.                               FElectrostatic   =   FCentripetal
         Drawbacks of Rutherford’s Model
q = n (1.6 x 10-19 C)
n = 1 , 2 , 3 ...
                                     q1 q2
                                                            1                   Nm2
F12      =         F21     =     K
                                      r2     K        =    4πƐ0     =    9 x 109
                                                                                 C2
 F12
       +q1                     +q2 F21
                                                                               C
                                                 Ɛ0       =   8.854 x 10-12
                                                                              Vm
             F12         F21
       +q1                     -q2
                    r
                                                 Ɛ0 =     Permittivity of vacuum
                Potential Energy
P.E. = qxV
            1   q1 q2                            q1 q2
P.E.   =   4πƐ0   r
                                    P.E.    =   K r
                   Closest Distance Of Approach
     1        3    2
                                    When two charged particles of
                                 similar nature approach each other,
         V𝛂                          the repulsion between them
m𝛂                                increases but due to initial kinetic
                        R
                                 energy, the particles come closer to
                                each other (Recall the bombarding of
                  R1             positively charged alpha particle on
 Closest distance of               gold foil where the alpha particle
                                    approaching positively charged
 approach( in alpha particle
                                        nucleus of gold atom).
 scattering by gold nucleus),
 R = √4KZe2/m𝝰 V𝝰
                   Closest Distance Of Approach
     1        3    2
                                  But at a certain distance between
                                 them, the relative velocity becomes
         V𝛂                      zero and after that due to repulsion,
m𝛂                               the particles starts going away from
                       R
                                  each other. This distance between
                                   the particles where velocity once
                  R1                becomes zero is called Closest
                                 distance of approach and can easily
                                 be calculated using conservation of
 Closest distance of approach,              energy concept.
 R = √4KZe2/m𝝰 V𝝰
                Electromagnetic Waves
Electric Field
 Oscillating
 Electric &
Magnetic field
                        Magnetic Field
       Properties of Electromagnetic Waves
Frequency Wavenumber
   Velocity                  Amplitude
           Characteristics of Electromagnetic waves
Crest
        Wavelengt                         Amplitude
           h                                           Mean
                                                      position
                    Trough
                        Velocity of the wave
                                         Frequency (𝛎)
      Wavelength (λ)
                                  Number of waves passing
                                 a given point in one second
   Distance between two              SI unit : Hertz (Hz), s-1
consecutive crests or troughs
         SI unit : m
                                                           1
                                     𝛎          =          T
Characteristics of Electromagnetic waves
Velocity (c or v)
              c        =          𝛎λ
       Characteristics of Electromagnetic waves
                                                  1
                                 𝛎      =         λ
 Consists of radiations
        having                   𝛎      =         c𝛎
different wavelength or
      frequency
                                                  1
                                 𝛎      =         T
Electromagnetic Spectrum
Decreasing        Increasing
             or
frequency         wavelength
            Electromagnetic Spectrum
Gamma rays
X-rays
                    Ultraviolet
Frequency                              Wavelength
decreases            Visible           decreases
                     Infrared
                    Microwave
                    Radiowave
                            Electromagnetic Spectrum
  Short                                                         Long
wavelength                                                    wavelength
   High                                                              Low
frequency                                                         frequency
                               Visible light
EM Radiation: Wave or Particle?
Diffraction
             Interference
  EM Radiation: Wave or Particle?
Black-body radiation
Photoelectric effect
Where N ∈ + I
                    Low temperature
                     Low frequency
                   Longer wavelength
                    High temperature
                     High frequency
                   Shorter wavelength
  What is a black body?
Idealized system
                           Radiatively Black
Visually Black body vs
                                Body
            2
                              3000 K
            0
                 0     0.5     1       1.5   2    2.5      3
                         Wavelength (μm)
  Particle Nature of Radiation
                       Variation of
Quantisation
                      intensity with
 of Energy
                       wavelength
   Planck’s Quantum theory
E ∝ 𝝂Radiation E = nh𝝂
                                       c
  E      =       h𝝂        =       h
                                       λ        n = number of photons
                                                   = 0, 1, 2, 3, ….
      h = Planck’s constant
        = 6.626 × 10-34 Js
    One electron volt (eV)
1 eV = 1.6 × 10-19 J
                               12,400
    E (eV)       =              λ (Å)
(
E
      kJ
     mole    )   =   E   (     eV
                             particle   ) × 96.48
                Photoelectric Effect
                                       When radiation of
Metal plate       Photoelectrons    sufficient energy falls on
                                     the metal plate, there
                                       starts emission of
                                        electrons called
                                        photoelectrons.
                Observations
                 Instant transfer
                of energy to the
                electron when a
              photon of sufficient
             frequency strikes the
                   metal atom
            Threshold frequency (𝝂O)
Minimum frequency
                             Each metal has a
 required to eject a
                              characteristic
photoelectron from a
                           threshold frequency
   metal surface
                      Observations
Intensity of light
                                  Brightness of light
                         Observations
                      No electron is ejected,
                 regardless of the intensity of light
                                                        𝝂incident < 𝝂0
         K.E. is independent of
        the intensity of radiation
    Striking photon’s
          energy               =          h𝝂
     Work function              =          𝝓
                 Work Function (𝝓)
                                                                   1    2
EPhoton     -   𝝓   =   K.E.Max       h𝝂      =      h𝝂0      +    2
                                                                     mevmax
K.E.Max = h𝝂 - h𝝂0
                   c               c
K.E.Max    =      hλ       -      hλ
                                     o
                   Plotting K.E. vs Frequency
                                      K.E.Max   =   h𝝂      -   h𝝂0
K.E.
       ν0
            Frequency
Acceleration and Deceleration of Charged Particles
                          Acceleration:
           If a positive charge moves from higher to
             lower potential (like an electron moves
              from cathode to anode) or a negative
                charge moves from lower to higher
                            potential.
               Deceleration is just opposite to the
                           acceleration.
            Stopping potential(Vs)
             eVS      =     K.E.max
Accelerating potential voltage (V)
Minimum K.E. eV
Photocurrent (I)
                        Frequency
Photocurrent v/s Frequency of the Radiation
For ν > ν0
K.E.
                   Intensity
       Photocurrent vs Collector Plate Potential
          at different intensity of radiation
                                                  I : Intensity
                                                                               Photocurrent at
                           Photocurrent
                                                   I3 > I2 > I1              different intensity of
                                                                                radiation. Here
                                                    I3                      frequency of radiation
                                                    I2                             is same.
                                                    I1
                                                                  Saturation Current
Stopping potential
              -V0                         0
     Retarding Potential                      Collector Plate Potential
               Photocurrent vs Collector Plate Potential
                  at different intensity of radiation
                         Photocurrent
                                                         Photocurrent at different
                                                          frequencies of radiation.
                                            Saturation
                                                         Here intensity of radiation
                                             Current
𝛎3 > 𝛎2 > 𝛎1                                                      is same.
               𝛎3
                    𝛎2
                         𝛎1
      -V03 -V02 -V01                    0
       Retarding Potential Collector Plate Potential
Bohr Atomic Model
 Postulates
                                              n=3
             Stationary
                                                    n=2
               orbits
                                                          n=1
 Concentric circular orbits around the                          K   L   M
               nucleus
                                            n = 1, 2, 3...
       Angular momentum of the
       electron in these orbits is
                                      h      Planck’s constant
     always an integral multiple of
                  h
                  2𝜋                  m         Mass of electron
v Velocity of electron
                                      r    Radius of orbit
                    Postulates
                                                  Energy (h𝜈)
                                                  absorbed
Electron can jump from lower to higher orbit by
    absorbing energy in the form of photon
        Energy
                      =        E3 - E2
       Absorbed
        Energy
       Released       =        E2 - E1
                      Postulates
ΔE = En2 - En1
                ΔE             E2 - E1
  𝝂      =       h
                        =        h
   Applicable only
      for single
   electron species
          like
   H, He+, Li2+, Be3+
Mathematical Analysis
                             Velocity of an electron
                                 in Bohr orbit
                                    Time period of an
       Calculating                electron in Bohr orbit
                                Frequency of an
                             electron in Bohr orbit
                     Energy of an electron
                         in Bohr orbit
 Postulate
FElectrostatic
On rearranging,
      mv2                 KZe2
       r
                  =                                      KZe2
                           r2           v2
                                                  =             i
                                                          mr
 Calculating the radius of Bohr orbit
According to Bohr's Postulates,
                                         On comparing equation (i) and (ii),
                         nh
      mvr        =       2π
                                                KZe2                n2h2
                                                 mr         =      4π2r2m2
                         nh
       v         =      2πrm
                                                                    n2h2
                                                   r        =
                                                                  4π2mKZe2
        2                n2h2
       v         =       2 2    2
                                    ii
                       4π r m
Calculating the radius of Bohr orbit
                            n2
      rn         =    0.529
                            Z
                               Å
                                       rn   ∝   n2
                                                1
           n = Energy level            rn   ∝   Z
        Z = Atomic number
               Calculation of velocity of an electron
                           in Bohr orbit
                      nh
      v       =      2π r m        i
Calculation of velocity of an electron
            in Bohr orbit
 Putting equation (ii) in equation (i),
                         nh   4π2mKZe2
     v          =       2πm
                            ×
                                n2 h2
                         2πKZe2
      v          =         nh
                                      Z ms-1
      vn         =      2.18 x 106
                                      n
vn ∝ Z
                    1
      vn    ∝       n
            Time period of Revolution (T)
                             Circumference           2πrn
        T         =                          =        vn
                                Velocity
                             n3 s                           n3
T   =       1.5 x 10   -16                       T     ∝
                             Z2                             Z2
             Frequency of Revolution (f )
                             1                vn
         f        =         T
                                   =          2πrn
                       Z2                                 Z2
f   =    6.6 x 10 15
                       3
                       n
                            Hz            f          ∝    n3
                Calculation of Energy of an electron
     Total energy (T.E.) of an electron revolving in
                   a particular orbit
                                                                    1
                                               K.E.         =         mv2
T.E. = K.E. + P.E.                                                  2
                                                                      2
                                                                  KZe
   K.E.   Kinetic energy                          P.E.   =      _
                                                                   r
             Potential
   P.E.                                                                  2
             energy                                      2           KZe
                                      T.E.    =        mv       +    _
                                                                       r
                                                        2
Calculation of Energy of an electron
           mv2             KZe2
            r       =       r2
                   mv2            KZe2
    K.E.     =      2      =       2r
Calculation of Energy of an electron
                                        1
        T.E.    =      K.E.       =     2
                                          P.E.
       Calculation of Energy of an electron
                                    KZe2
                      T.E.   =       2r
                                   2𝝿2me4K2   Z2
               T.E.     =        =    h2      n2
  Calculation of Energy of an electron
       Putting the value of constants we get:
                                             Z2
T.E.        =        En         =     13.6
                                             n2
                                                eV/atom
                   Z2
  En        ∝      n2
Z↑ En ↓
       n↑       En ↑
            Energy of an electron
            Distance of electron
                                   ↑
             from the nucleus
                  Energy           ↑
      Energy of an electron
                     Z2
En             -13.6 2 eV/atom
                     n
                                2 2
                         -11-18Z Z
E
Enn       -2.18
            -2.18x   x1010 2 2 erg/atom
                                    J/atom
                             nn
                      22
             -313.6 Z
                    Z    kcal/mol
En            -1312 22 kJ/mol
                    n
                    n
                             Z2
En        -2.18 x 10   -11
                                erg/atom
                             n2
                      2
             -313.6 Z   kcal/mol
En
                    n2
     Energy of an electron
At n = ∞
T.E. = 0
P.E. = 0
        K.E.   =   0
Energy Difference
                                                                   2
          ΔE       =        En
                                 2
                                                       En1
                                2                        2
           eV          _ 13.6 Z                  _ 13.6 Z
       ΔE atom     =          n2 2                          n1 2
                                         1 _ 1        eV
          ΔE       =     13.6 Z      2
                                         n1 2 n2 2   atom
                                           1 _ 1          J
          ΔE       =   2.18 x 10-18 Z2
                                           n1 2 n2 2    atom
Energy level diagram
                               E=0
n=∞
n=5
n=4                                  Higher
                                     energy
n=3
                                     states
n=2
                Ground state
n=1
Energy level diagram
n=∞                                                     E=0
n=5                                                     E5 = -0.54 eV
n=4                             ΔE = E4- E3 = 0.66 eV   E4 = -0.85 eV
n=3                                                     E3 = -1.51 eV
        ΔE = E3- E2 = 1.89 eV
n=2                                                     E2 = -3.4 eV
ΔE = E2- E1 = 10.2 eV
                  Ground state
n=1                                                     E1 = -13.6 eV
Definition For Single Electron
          Systems
                 Ground state (G.S.)
                                  1 _ 1          eV
                             2
       ΔE         =     13.6 Z
                                  n1 2 n2 2     atom
Putting n2 = ∞ & n1 = 1
                                         eV
       ΔE          =             13.6 Z2 atom
Ionisation energy (I.E.)
I.E.H = 13.6 eV
I.E.He+ = 54.4 eV
  I.E.Li 2+   =   122.4 eV
             Ionisation potential (I.P.)
                I.P.He +   =   54.4 V
                        Excitation Energy
 Energy required to
move an electron from
                                                 Excitation
       n = 1 to                                  energy of
   any other state        For H atom             2nd state
                          n = 1 to n = 2
10.2 eV
                                    Excitation                    1st
                                    energy of                 excitation
                                     1st E.S.                  energy
                          Excitation potential
                                                         12.09 V
                                          Excitation                    2nd
                                          potential                  excitation
                                          of 2nd E.S.                potential
Binding or Separation energy
        Energy required to
 move an electron from any state to
               n=∞
                            From
Ionization Energy
                        n = 1 to n = ∞
                          From
 Binding Energy
                    any state to n = ∞
                      From n = 1 to
Excitation Energy
                     any other state
               Spectrograph
Spectroscopy
                              Spectrum
          Spectrogram
                 Spectroscopy
Spectroscopy      Spectrograph/
  Branch of      SpectroscopeIns    Spectrogram
                     trument
 science that                       Spectrum of
                 used to separate
deals with the     radiation of      the given
   study of          different         radiation
   spectra         wavelengths
Classification: Based on Origin
Emission
Spectra
                       Absorption
          Emission Spectrum
Continuous
Emission
Spectrum
                                Discrete
         Continuous Spectrum
Screen
Prism
Light Source
           Classification: Based on Nature
Line
Discrete
Emission                                    Band
Spectrum
                         Continuous
            Line Spectrum
               Line spectrum
                      Emission Spectra
                                         Screen
Light emitted by
gas
Prism
     Gas in Excited
        State in
       Discharge
      Tube at low
       Pressure
Application of Line Spectrum
      Molecular spectrum
 Classification : Based on Origin
Emission
Spectrum
                        Absorption
                Absorption Spectrum
-0.54 eV
                    3.4 eV
n=5
n=4                                                           -0.85 eV
n=3                                                           -1.51 eV
n=2 -3.4 eV
12.09 eV
12.75 eV
                                                   13.06 eV
                10.2 eV
      13.6 eV
n=1                                                           -13.6 eV
Rydberg’s Formula
                hc                                 1 _ 1         J
  ΔE     =      λ         =      2.18 x 10-18 Z2
                                                   n1 2 n2 2   atom
   1           2.18 x 10-18 Z2    1 _ 1
          =                                 m-1
   λ                 hc           n1 2
                                       n2 2
Rydberg’s Formula
     1                                        1 _ 1      -1
             =      1.09678 x 10 x Z7     2             m
     λ                                        n1 2 n2 2
     1                                    1 _ 1
                                                    cm-1
     λ       =              109678 x Z2
                                          n1 2 n2 2
                     1                        1 _ 1
                               =    RH Z2 x
                     λ                        n1 2 n2 2
   n1          1, 2, 3, ...                               912
                                                                      Å
                                        λ      =          1 _ 1
                                                    Z2
   n2    n1 + 1, n1 + 2, ...                              n1 2 n2 2
    Rydberg’s Formula
For H atom
1                      1 _ 1
λ
     =     RH x
                       n1 2 n2 2
n1 1, 2, 3, ...
    n2   n1 + 1, n1 + 2, ...
Spectral series of H atom
                                   1                     1 _ 1
                                   λ     =      RH x
                                                         12  n2 2
 1st spectral series.
Found in UV region
      by Lyman
                                        n1 = 1 (Final state)
                                           n2 = 2, 3, 4 …
                                       (Initial states, n2 > 1)
Lyman Series
       st
                                      n2 = ∞
     1 line of           2→1
 Lyman series (𝛂 line)
                               Wavelength               n12
                                               =
                               of last line             RH
     2nd line of
                         3→1
 Lyman series (𝛃 line)
                                                   1
                                λLyman    =        RH
 Last line of Lyman
                         ∞→1
 series (Series limit)
Lyman Series
 12400                           12400
         Å   ≤   λLyman      ≤             Å
  13.6                            10.2
Lyman Series
  Longest                                      12400
 wavelength
    line        =      λlongest or λmax    =            Å
                                               ΔEmin
  Shortest                                     12400
    line
 wavelength     =      λshortest or λmin   =            Å
                                                ΔEmax
              Where,      E in eV
                 Lyman Series
                  Series limit
  Limiting/last line of any spectral series
n=6
n=5
n=4
n=3
n=2
λmax λmin
n=1
             Lyman series
                         Balmer Series
1                     1 _ 1
λ
      =      RH x
                      22  n22
n1 = 2 (Final state)
        n2 = 3, 4, 5 …
    (Initial states, n2 > 2)
                   Balmer Series
n=∞
n=6
n=5
n=4
n=3
      λmax                         λmin
n=2
             Balmer series
n=1
           Paschen Series
       1                     1 _ 1
       λ
             =      RH x
                             32  n22
n1 = 3 (Final state)
               n2 = 4, 5, 6 …
           (Initial states, n2 > 3)
               Paschen Series
n=∞
n=6                    λmin
n=5
n=4   λmax
n=3
n=2
             Paschen series
n=1
           Brackett Series
       1                     1 _ 1
       λ
             =      RH x
                             42  n22
n1 = 4 (Final state)
               n2 = 5, 6, 7 …
           (Initial states, n2 > 4)
             Brackett Series
n=∞
n=6                 λmin
n=5   λmax
n=4
n=3
n=2
             Brackett series
n=1
            Pfund Series
       1                     1 _ 1
       λ
             =      RH x
                             52  n22
n1 = 5 (Final state)
                n2 = 6, 7, 8 …
           (Initial states, n2 > 5)
              Pfund Series
n=∞
                   λmin
n=6   λmax
n=5
n=4
n=3
n=2
             Pfund series
n=1
           Humphrey Series
       1                      1 _ 1
       λ
              =      RH x
                              62  n22
n1 = 6 (Final state)
                 n2 = 7, 8, 9 …
            (Initial states, n2 > 6)
             Humphrey Series
n=∞
n=7   λmax        λmin
n=6
n=5
n=4
n=3
n=2
         Humphrey series
n=1
Line Spectrum of Hydrogen
n=∞
n=7
n=6
n=5
n=4
n=3
n=2
                     Balmer   Paschen Brackett Pfund Humphrey
                     series    series  series series   series
n=1
      Lyman series
Maximum Number of Spectral Lines
                  =
     Maximum number of different
          types of photons
Maximum Lines for the transition from 4 to 1
             4 to 3
             4 to 2   3 to 2
             4 to 1   3 to 1   2 to 1
       n=4
       n=3
n=2
       n=1
Maximum Lines for the transition from 5 to 1
      5 to 4
      5 to 3   4 to 3
      5 to 2   4 to 2   3 to 2
      5 to 1   4 to 1   3 to 1   2 to 1
n=5
n=4
n=3
n=2
n=1
                 Maximum Number of Lines
Δn nH - nL
    In Lyman series
       (nHigher > 1)        =      nHigher - 1       For a particular
                                                          series
   In Paschen series
       (nHigher > 3)        =      nHigher - 3
Maximum Number of Lines
  In Brackett series
     (nHigher > 4)     =   nHigher - 4
   In Pfund series
      (nHigher > 5)    =   nHigher - 5
 In Humphrey series
     (nHigher > 6)     =   nHigher - 6
                                Example
Number of spectral lines in Lyman series
            from 4th shell              = nH - 1 = 4 - 1 = 3
                  n=4
                  n=3
n=2
                  n=1
                 Example
      4 to 3
      3 to 2
      2 to 1     4 to 2     3 to 1     4 to 1
n=4
n=3
n=2
n=1
                                            Dual Nature
                                             of Matter
  Important
Developments
                                           Heisenberg’s
                                        Uncertainty Principle
   h
λ=
   p
           Wave
       associated with
          moving
          particles
          h
How λ =       ?
          p
           de Broglie Hypothesis
                                       hc
Planck’s equation       E          =   λ
  Einstein’s Mass
Energy relationship
                        E          =   mc2
                de Broglie Hypothesis
Equating both
                  hc
                  λ
                          =       mc2
For photon
                                  h
                  λ       =       mc
                                   h
For matter        λ       =        mv
de Broglie Wavelength (λ)
                    h               h
         λ      =   mv       =      p
      Momentum                    Velocity
  p                      v
      of particle                of particle
         Mass                    Planck’s
  m                      h
      of particle                constant
de Broglie Wavelength (λ)
                            h
              λ       =     p
          0
                  p
Relativistic Mass
mO
       m            =
                             √1-( )  v   2
                                     c
       Velocity
                              Velocity
v     w.r.t.            c
                              of light
    the observer
     Dynamic
m                       mO   Rest mass
      mass
     Relativistic Mass
                                     √1-( )
                                         v   2
m0         =           m        Χ
                                         c
If v = c
mO = 0
      Experimental verification of
        de Broglie’s prediction
                                  1
                    λ    ∝        m
de Broglie’s Equation & Kinetic Energy
                           1
           K.E.     =        mv2
                           2
m2v2 = 2 K.E. × m
         mv         =     √ 2 K.E. x m
        de Broglie’s Equation & Kinetic Energy
de Broglie                      h                  h
 equation
               λ        =       mv          =      p
Since mv = √ 2 K.E. x m
                                     h
                        λ =
                              √2 K.E. × m
          de Broglie’s Equation & Kinetic Energy
 A charged particle
accelerated from rest
 across a potential
                               | K.E. |    =       |qV|
   difference of V
∵ mv = √ 2m × K.E.
        ∴           mv     =     √ 2m × q V
de Broglie’s Equation & Kinetic Energy
                                     h
               λ         =         2m × q V
                               √
                                       Charge on a
         λ    Wavelength (m)   q
                                        particle (C)
                                  r
                                               An integral number of
                                           complete wavelengths must
                                           fit around the circumference
                                                    of the orbit.
Electron exist      Electron don’t exist
Circumference,        Circumference,
    2πr = nλ              2πr ≠ nλ
                   Electron as a Wave
When electrons                              nh
 are in phase,
                   2𝜋r          =           mv
Bohr’s Postulate                            nh
    verified        mvr          =           2𝜋
                         n = Energy level
 Heisenberg’s Uncertainty Principle (H.U.P.)
Werner Heisenberg
Heisenberg’s Uncertainty Principle
                                           h
                Δx . Δp        ≥          4𝜋
                                           h
               Δx . m . Δv     ≥          4𝜋
              Uncertainty in            Uncertainty in
         Δx                        Δp
                position                 momentum
               Mass of                  Uncertainty in
         m                         Δv
               particle                  velocity
         Principle of Optics
Since Δx = λ
 For accurate
                Δx   0       λ   0
   position
For a photon
                                     E       =       hc
                                                     λ
                                     λ   0       E    ∞
Heisenberg’s Uncertainty Principle
Similarly
For an electron
                                       h
        Δx . m . Δv     ≥             4𝜋
                                    6.626 × 10-34 Js
         Δx . Δv       =          4 × 3.14 × 9.1 × 10-31 kg
         Δx . Δv       ≅                10-4 m2s-1
Heisenberg’s Uncertainty Principle
                              h
    Δx . Δp       ≥          4𝜋
Δp                                 h
Δt
   . Δx . Δt      ≥               4𝜋
 Δp
    = Rate of change in momentum = F
 Δt
Energy - Time Variant of H.U.P.
                                h
  F . Δx . Δt        ≥         4𝜋
                                h
    ΔE . Δt          ≥         4𝜋
ΔE Uncertainty in Energy
     Δt       Uncertainty in Time
          Significance of the Uncertainty Principle
● x, y, z = Cartesian coordinates
● h = Planck’s constant
                 z
                                         x      =        r sin𝜃 cosɸ
                            P
                     r                   y      =        r sin𝜃 sinɸ
z = r cos𝜃 𝜃
             O                      y
                                         z      =          r cos𝜃
             ɸ
                 rs
                     in
                       𝜃
    x                       Pl
                       Wavefunction
When SWE is solved for H like species, the obtained values
of 𝚿 could be factorized into one containing only ‘r’ and the
                  other containing (𝜃, ɸ).
                              n, l                 l, ml
                  Schrodinger Wave Equation
n l ml s
    ✔        ✔           ✔             х
          What is an Orbital?
             3D region            Probability of
Orbital      around the         finding an electron
              nucleus              is maximum
              What is an Orbital?
    Set of four
numbers required       2    Azimuthal Quantum number ( l )
   to define an
  electron in an       3    Magnetic Quantum Number ( ml )
 atom completely
                                    n = 1, 2, 3...
Describes the size
 of electron wave           Represented as K, L, M, N,...
& the total energy
  of the electron    Angular momentum in any                nh
                              shell                  =      2π
         Azimuthal Quantum Number (l )
                                  l         =          0 to (n - 1)
                                            =
    Boundary Surface Diagram
Example
              Shape : Spherical
 Classification of Orbitals
                       p
Orbital
                       d
                       f
                     Shape of Orbitals
Orbital Shape
s Spherical
p Dumb bell
   Collection of
  similar shaped
orbitals of same n.
    Subshell
l Subshell Description
0 s Sharp
1 p Principal
2 d Diffused
3 f Fundamental
4         g       Generalised
  Subshell Representations
                            Subshell
   n              l
                            notation
   1              0             1s
2 0, 1 2s, 2p
3 0, 1, 2 3s, 3p, 3d
Orbital angular                                  h
momentum (L)      =          l (l + 1) ħ   ħ=
                                                2π
                      Orbital angular
       Subshell
                       momentum
           s                0
p 2 ħ
           d                6 ħ
        Magnetic Quantum Number (ml )
 For d
subshel,             ml = -2, -1, 0, 1, 2
  l=2
Magnetic Quantum Number (ml )
       Maximum number of
       orbitals in a subshell
                                        =               2l + 1
s 1
                  f                           7
      s - orbital
  Shape : Spherical
Non-directional in nature
                       x
                p - orbital
z z z
y y y
x x x
pz                py                 px
                   d - orbital
                    z                      z                         z
                         y                       y                           y
                             x
                                                                                     Non axial
                                                     x                           x
                                                                                     d-orbitals
   Maximum number of
  electrons in a subshell       =        2 (2l + 1)
Subshell s p d f
l 0 1 2 3
   Number of electrons      2       6   10     14
                Spin Quantum Number (s or ms)
Spin of an electron
                                               1                  1
                                        s= + 2            s=      2
Proposed by George Uhlenbeck (left)
    and Samuel Goudsmit (Right)
  Spin Quantum Number (s)
Spin magnetic
moment (μ)        =       √n(n+2) B.M.
Spin angular          h
momentum         =   2π
                        √s(s+1)
Maximum Spin            1 n
of an atom (S)   =      2
  Spin
multiplicity     =    2 |S| + 1
   Orbit and Orbital
Orbit Orbital
Orbit Orbital
Aufbau Principle
                                          Pauli’s Exclusion
              Rules
                                             Principle
                                       Hund’s Rule of
                                     Maximum Multiplicity
Aufbau Principle
  Electrons are
 filled in various
orbitals in order of
 their increasing
     energies
Energies of Subshells of H-like Species
                                                         Order of
   1s < 2s = 2p < 3s = 3p = 3d < 4s = 4p = 4d = 4f < …
                                                         Energy
         Energies of Subshells of H-like Species
4s 4p 4d 4f
                                     Degenerate Orbitals:
         3s     3p         3d
Energy
1s < 2s
2s < 2p
5p > 4d
2p < 3p
    3d       <       4p
Energies of Subshells of Multi electron Species
4p
                             3d
                 4s
                      3p
                 3s
        Energy
                      2p
                 2s
                 1s
Energies of Subshells of Multi electron Species
H-like v/s Multi-electron species
                                    Electrons experience
    Only attractive forces are    attractive forces towards
      present between the          the nucleus as well as
    nucleus and the electron.    repulsive forces from other
                                          electrons.
   One-electron species
                          There is only attractive
                               force here
             n=2
                   n=1
Attraction
      Multiple-electron species
                          Outer Electron
                                           Attractive Force
Shielding Electron
Repulsion
Attraction
            Pauli’s Exclusion Principle
                               No two electrons
                                in an atom can
                                have the same
                                 set of all four
                                   quantum
                                   numbers
Wolfgang Pauli
Pauli’s Exclusion Principle
Wrong
                             Right
       Subshell electron capacity
s2 ⥮
p6 ⥮ ⥮ ⥮
d10 ⥮ ⥮ ⥮ ⥮ ⥮
f14   ⥮     ⥮    ⥮    ⥮   ⥮   ⥮   ⥮
Hund’s Rule of Maximum Multiplicity
            Friedrich Hund
        Hund’s Rule of Maximum Multiplicity
                                     Electron-nucleus interaction is
                                               improved
             Electronic Configuration
                              H     ↿
                                   1s1
 Distribution
                              He   ⥮
of electrons in
                                   1s2
  orbitals of
   an atom
                              Li   ⥮      ↿
                                   1s2   2s1
Electronic Configuration of Various Elements
 Be   ⥮     ⥮                 N    ⥮     ⥮     ↿    ↿    ↿
      1s2   2s2                    1s2   2s2       2p3
 B    ⥮     ⥮     ↿            O   ⥮     ⥮     ⥮    ↿    ↿
      1s2   2s2       2p1          1s2   2s2       2p4
 C    ⥮     ⥮     ↿    ↿       F   ⥮     ⥮     ⥮    ⥮    ↿
      1s2   2s2       2p2          1s2   2s2       2p5
Electronic Configuration of Various Elements
Ne   ⥮     ⥮     ⥮    ⥮    ⥮
     1s2   2s2       2p6
Na   ⥮     ⥮     ⥮    ⥮    ⥮    ↿
     1s2   2s2       2p6       3s1
Mg   ⥮     ⥮     ⥮    ⥮    ⥮   ⥮
     1s2   2s2       2p6       3s2
             Simplified Electronic Configuration
                           Configuration of Sodium:
                  Na      ⥮          ⥮     ⥮     ⥮     ⥮      ↿
                          1s2        2s2         2p6         3s1
Ne
Simplified configuration: Na Ne ↿
                                                       3s1
                       Electronic Configuration
   a)   21
          Sc      1s2 2s2 2p6 3s2 3p6 4s2 3d1
                  [Ar] 4s2 3d1                    45
                  [Ar] 3d1 4s2                    21   Sc
                                                  Scandium
           ↿                           ⥮
                       3d1             4s2
                                       1      1
          Total spin               +     or -
                                       2      2
                          Electronic Configuration
   b)    Fe
        26
                      1s2 2s2 2p6 3s2 3p6 4s2 3d6
                      [Ar] 4s2 3d6                     56
                      [Ar] 3d6 4s2                     26   Fe
                                                            Iron
             ⥮    ↿        ↿    ↿   ↿       ⥮
                          3d6               4s2
                                            4      4
             Total spin                 +     or -
                                            2      2
              Exceptions
                            Not
  Cr   [Ar] 4s2 3d4
24
                           Correct
                                         52
                                          Cr
                                         24
 Cr
24
        [Ar] 4s1 3d5       Correct
                            Not
29
  Cu    [Ar] 4s2 3d9
                           Correct
                                          63
                                           Cu
                                          29
 Cu
29
        [Ar] 4s1 3d10      Correct
     Exactly half filled &        Stability of half filled & fully filled
fully filled orbitals make the                   orbitals
 configuration more stable
                                                       Consequently, their
                                                   shielding of one another is
                                                         relatively small
      Symmetrical               Symmetry
     distribution of             leads to
       electrons                 stability         Electrons are more strongly
                                                     attracted by the nucleus
Electrons in                         Different
                        Equal
 the same                             spatial          Have less energy
                       energy
  subshell                          distribution       and more stability
     Exchange Energy
a b
↿ ↿ ↿ ↿ ↿ ↿ ↿ ↿ ↿ ↿
           c                                 d
  ↿    ↿    ↿     ↿    ↿       ↿    ↿    ↿       ↿   ↿
Cations
Ions
                         Anions
Electronic Configuration of Cations
  Na    ⥮     ⥮     ⥮    ⥮    ⥮    ↿
        1s2   2s2       2p6       3s1
  Na+   ⥮     ⥮     ⥮    ⥮    ⥮
        1s2   2s2       2p6       3s0
    Electronic Configuration of Cations
29
     Cu :   Ar   ⥮     ⥮     ⥮    ⥮    ⥮   ⥮    ⥮     ⥮   ⥮       ↿
                 3s2        3p6                3d10           4s1
 Cu+ :
29
            Ar   ⥮     ⥮     ⥮    ⥮    ⥮   ⥮    ⥮     ⥮   ⥮
                 3s2        3p6                3d10           4s0
             F       ⥮     ⥮     ⥮   ⥮     ↿
                     1s2   2s2       2p5
                 _
             F       ⥮     ⥮     ⥮   ⥮     ⥮
                     1s2   2s2       2p6
Schrodinger Wave Equation (SWE)
● x, y, z = Cartesian coordinates
● h = Planck’s constant
                        n,
                        n, ll                l,l, m
                                                  ml
                                                   l
Physical Significance of 𝚿
                            Amplitude of the
                             electron wave
     Physical
   significance              Can be +ve or -ve
       of 𝚿
                            As such there is no
                             significance of 𝚿
    Physical significance of 𝚿2
                          Probability of finding an
     𝚿2                   electron per unit volume or
                          probability density
              Probability density
                     4                   4 3
 dV      =           3
                         𝜋 (r + dr)3 -
                                         3
                                           𝜋r       =        4𝜋r2 . dr
Radial probability
density on a layer
                         ×      Volume of that layer     =       𝚿R2 . 4𝜋r2 . dr
𝚿2.dV = 0
∵ dV can’t be zero
     ⟹          𝚿2        =        0
        Nodes
Radial Node
Nodes
                Angular Node
                   Node
⟹    𝚿(r)      =    0     or   𝚿(𝜃,ɸ)   =   0
                   Radial Node
      Plane or a surface
     passing through the         𝚿𝜃, Φ or 𝚿2𝜃, Φ is zero
           nucleus
                        Angular node
Radial Node vs Angular Node
1s       2s                  3s
     Angular Nodes of ‘p’ orbitals
z                                    z
         y                                y
                    z
             x
                                              x
                           y
px                                   pz
                               x
                    py
      Angular Nodes of ‘d’ orbitals
 z                                    z
                                            y
              y             x
                      z
          x
dzx                                   dxy
                                x
                  y
                      dyz
Angular Nodes of ‘d’ orbitals
   z
                          z
                                y
                 y
                                    x
             x
 dx2-    2               dz 2
        y
            Comparison of Penetration Power
                3d
                       3p
                               3s
                      r
Comparison of Penetration Power
                             Radial Wave
                         function (𝚿) against r
                           Radial Probability
Plots                     density (𝚿2) against r
𝚿 ΨR2
                     r           r
           4𝜋r2ΨR2
                     r
          Radial Probability of 2s
                            Node
  𝚿                   ΨR2
          r                   r
4𝜋r2ΨR2
          r
              Radial Probability of 3s
𝚿 ΨR2
                                         r
          r
4𝜋r2ΨR2
          r
Radial Probability of 2p
𝚿 ΨR2
          r                r
4𝜋r2ΨR2
          r
Radial Probability of 3p
              3p
𝚿                  ΨR2
          r                r
4𝜋r2ΨR2
          r
              Radial Probability of 3d
              3d
𝚿                       ΨR2
          r                      r
4𝜋r2ΨR2
3d
          r
                         Analysis: 𝚿 Plots
1s 2p 3p 3d
             𝚿                         𝚿            𝚿
𝚿
r r r r
        2s                    3s
𝚿                𝚿
    r                              r
                         Analysis: 𝚿2 Plots
1s 2p 3p 3d
r r r r
2s 3s
𝚿R2 𝚿R2
      r                       r
    4𝜋r2ΨR2          4𝜋r2ΨR2
r
                 r
                           1s
            2s
       2
                      4𝜋r2ΨR2
    4𝜋r   ΨR2
r
                           2p
3s
                     4𝜋r2ΨR2
                 r
                           3p
                                Analysis: 𝚿2.4𝜋r2 Plots
                     4𝜋r2ΨR2
                 r
                           3d
                  (ΨR2) 4𝜋r2
1s
             r
2s
                   (ΨR2) 4𝜋r2
     Node
             r
3s
     Nodes
                 (ΨR2) 4𝜋r2
             r
                                     Nodes
Ψ2        Ψ2        Node   Ψ2
      r         r                r
     1s        2s               3s
         Radial Wavefunction of Hydrogenic Atoms
                    3/2                    1/2               l
              2Z           (n - l - 1)!        -Zr/na0 2Zr        2l + 1      2Zr
Rnl(r)   =    na0         2n [(n + l)!]3     e         na0
                                                                 Ln - l - 1
                                                                              na0
                 Laguerre Polynomial
                                       Z
           where 𝜌 = 2kr and kn =
                                      a0n
                                  1s orbital
                                                                         2Zr
                         R (1s)       =    K1σ e- σ/2   where,   σ   =   n a0
                               4𝜋r2𝚿R2
𝚿R        𝚿R2
     r             r                     r
                                 2s orbital
                                                    - σ/2
                    R (2s)       =        K2(2 - σ) e
                              4𝜋r2𝚿R2
𝚿R                Node
              2
         𝚿R
     r             r                    r
       p-orbitals
                                               - σ/2
                         R (2p)     =     K3σ e
                                    4𝜋r2𝚿R2
𝚿R          𝚿R2
     r              r                         r
                                3p orbital
                                                         - σ/2
                   R (3p)       =        K4(4 - σ) σ e
                                        4𝜋r2𝚿R2
𝚿R         𝚿R2
                      r                           r
     r
                          Radial node
                          xy nodal plane
                               Nodes in p-orbital
                                    3pz orbital
                                        z
                 2pz orbital
                     z
                                                     Radial node
                                                  xy nodal plane
xy nodal plane                                    (Angular node)
(Angular node)
Nodes in d-orbitals
x y
                                                   - σ/2
                         R (3d)     =      K5σ 2 e