Atomic Structure
Dr. Md. Lutfor Rahman
    SST, UMS
          Radioactivity
• Discovered by accident
• Becquerel
• Three types
 –alpha- helium nucleus (+2 charge,
  large mass)
 –beta- high speed electron
 –gamma- high energy light
    Rutherford’s Experiment
• Used helium to produce alpha particles.
• Aimed alpha particles at gold foil by drilling
  a hole in a lead block.
• Since the mass is evenly distributed in gold
  atoms, alpha particles should go straight
  through.
• Used gold foil because it could be made
  atoms thin.
                         Florescent
 Lead     Uranium          Screen
 block
                    Gold Foil
Experiment set-up
What he expected
Particles would pass through
 Because
Because, he thought the mass was
evenly distributed in the atom.
mass was evenly distributed
What he got
  How he explained it
• Atom is mostly empty
• Small dense, positive         +
  piece at center.
• Alpha particles
  are deflected by it if they
  get close enough.
What Rutherford Observed
               +
          Models of the Atom
• Dalton
  – Smallest indivisible particle
• Thomson
   – Included the electron into the atom
• Rutherford
  – Nuclear atom with a layer of electrons.
            Modern View
• The atom is mostly
  empty space.
• Two regions
• Nucleus- protons and
  neutrons.
• Electron cloud- region
  where you might find
  an electron.
       Max Plank added a twist
       with his Quantum Theory
In 1900, Plank proposed that:
atom energy is absorbed or liberated in packets
or chunks of energy. Plank called these
packages of energy "quanta".
In order for an atom to absorb a packet of energy,
it must absorb the whole packet or none at all.
              Enter Einstein
Plank's
      .
        critics were legion. It wasn't until
1902 that a young man who worked at a
telegraph office near Berlin designed an
experiment that would be known as the
"Photoelectric Effect".
This young man was Albert Einstein.
                 Enter Einstein
In his experiment Einstein showed that as the
frequency of radiation was directly proportional
to the energy that was absorbed by the electrons.
The math statement of this relationship is stated as
:
E = h
Where E is the energy, absorbed by the electrons,
h is Plank’s Constant and  is frequency of
 . . . FINALLY
Niels Bohr puts it all together
  Bohr added Plank’s quanta idea
 to the Rutherford’s atomic model.
             Bohr’s Theory
• He proposed that the electrons existed
  at set levels of energy, at fixed
  distances from the nucleus.
• If the atom absorbed energy, the
  electron jumped to a level further from
  the nucleus
             Bohr’s Theory
• If it radiated energy, it fell to a level
  closer to the nucleus.
• His model was a huge leap forward in
  making theory fit the experimental
  evidence that other physicists had
  found over the years.
     The Bohr Model of the Atom
• Nucleus     • In the center, contains protons & neutrons
• Protons     • positive, one atomic mass unit (amu)
• Neutrons • neutral, one amu
              • energy levels around nucleus
• Shells
              • negative, no effective mass
• Electrons
The Bohr Model of the Atom
                 e-
         e   -                   e-
                                      e-
                      Protons
                      positive
         e-                      e-
                      Neutrons
                      neutral
                                      e-
    e-
         e-                      e-
     The Bohr Model of the Atom
• The atomic number is the number of protons in
  an atom
• Each element has a unique atomic number
                        or
• Each element has a different number of protons
• When the light is passed through a prism only a
   few wavelengths are present in resulting
spectra
• These appear as lines separated by dark areas,
  and thus are called line spectra
• When the spectrum emitted by hydrogen gas
was
 passed through a prism and separated into its
 constituent wavelengths four lines appeared at
 characteristic wavelengths
• Bohr began with the assumption that electrons
  were orbiting the nucleus, much like the earth
  orbits the sun.
• From classical physics, a charge traveling in a
  circular path should lose energy by emitting
  electromagnetic radiation
• If the "orbiting" electron loses energy, it should
end up spiraling into the nucleus (which it does
not).
• Therefore, classical physical laws either don't
apply
 or are inadequate to explain the inner workings of
 the atom
• Bohr borrowed the idea of quantize energy from
Planck
• He proposed that only orbits of certain radii,
corresponding to defined energies, are "permitted"
• An electron orbiting in one of these "allowed" orbits:
• Has a defined energy state
• Will not radiate energy
• Will not spiral into the nucleus
If the orbits of the electron are restricted,
the energies that the electron can possess
are likewise restricted and are defined by
the equation:
Bohr Model of the H atom
          Z2           1                     2 2 e 4
E n  R  2   R    2            R 
          n            n                     0
                                                 4  h
                                                       22
                              radius(n) = n2a0
 R = 13.6 eV
                              a0 = Bohr radius = 0.529 Å
 = reduced mass (nucleus and electron)
Z = nuclear charge (1 for H)
e = charge of electron
0 = permittivity of a vacuum
h = Plank’s constant
Bohr
Model
H atom
                                                        1
n = principal  Energy, Size  SHELL   E n   1 3 .6  2 
                                                       n 
n = 1, 2, 3 …
                                          E1 = -13.6 eV
n = 1 : ground state
                                          E2 = -3.40 eV
n = 2 : first excited state
                                          E3 = -1.51 eV
n = 3 : second excited state
                                          E4 = -0.85 eV
                                          E5 = -0.54 eV
                                          •
                                          •
                                          •
                                          E = 0 eV
                       A. Waves
• Wavelength () - length of one complete wave
• Frequency () – Number of waves that pass a
  point during a certain time period
  – hertz (Hz) = 1/s
• Amplitude (A) - distance from the origin to the
  trough or crest
        A. Waves
                           greater
            crest
                         amplitude
                         (intensity)
A
                       origin
                    trough
                            greater
                          frequency
                            (color)
            B. EM Spectrum
                                                              H
L
                                                              I
O
                                                              G
W
                                                              H
E
                                                              E
N
                                                              N
E
          R O Y              G.         B     I      V
                                                              E
R
                                                              R
G
                                                              G
Y
    red    orange   yellow   green   blue   indigo   violet   Y
    B. EM Spectrum
H
                     L
I
                     O
G
                     W
H
                     E
E
                     N
N
                     E
E
                     R
R
                     G
G
                     Y
Y
          B. EM Spectrum
• Frequency and wavelength are
  inversely proportional
             c = 
  c: speed of light (3.00  108 m/s)
  : wavelength (m, nm, etc.)
  : frequency (Hz)
             B. EM Spectrum
• EX: Find the frequency of a photon with a
  wavelength of 434 nm.
GIVEN:                    WORK:
=?                     =c/
 = 434 nm
  = 4.34  10-7 m       = 3.00  108 m/s
                           4.34  10-7 m
c = 3.00  108 m/s
                        = 6.91  1014 Hz
            C. Quantum Theory
• Planck (1900)
  –Observed - emission of light from hot
   objects
  –Concluded - energy is
   emitted in small, specific
   amounts (quanta)
           C. Quantum Theory
• Quantum - minimum amount of energy change
• Energy can be released (or absorbed) by atoms
  only in "packets" of some minimum size.
• This minimum energy packet is called a quantum
            C. Quantum Theory
• The energy (E) of a quantum is related to its
  frequency () by some constant (h):
                      E = h
• h is known as "Planck's constant", and has a
  value of 6.63 x 10-34 Joule seconds (Js)
• Electromagnetic energy is always emitted or
  absorbed in whole number multiples of (h*)
           C. Quantum Theory
• Einstein (1905)
  –Observed - photoelectric effect
           C. Quantum Theory
• Light shining on a metallic surface can cause
  the surface to emit electrons
• For each metal there is a minimum frequency
  of light below which no electrons are emitted,
  regardless of the intensity of the light
            C. Quantum Theory
• The higher the light's frequency above this
  minimum value, the greater the kinetic
  energy of the released electron (s)
• By Planck's results Einstein (1905) was able
  to established the photoelectric effect
           C. Quantum Theory
• Einstein assumed that the light was a
  stream of tiny energy packets called
  Photons
• Each photon has an energy proportional to
  its frequency (E=h)
           C. Quantum Theory
• When a photon strikes the metal its energy
  is transferred to an electron
• A certain amount of energy is needed to
  overcome the attractive force between the
  electron and the protons in the atom
            C. Quantum Theory
• Thus, if the quanta of light energy absorbed
  by the electron are insufficient for the
  electron to overcome the attractive forces
  in the atom, the electron will not be ejected
  - regardless of the intensity of the light.
           C. Quantum Theory
• If the quanta of light energy absorbed are
  greater than the energy needed for the
  electron to overcome the attractive forces of
  the atom, then the excess energy becomes
  kinetic energy of the released electron.
           C. Quantum Theory
• An important feature of this experiment is that
  the electron is emitted from the metal with a
  specific kinetic energy (i.e. a specific speed).
C. Quantum Theory
           C. Quantum Theory
• Einstein (1905)
  –Concluded - light has properties of both
   waves and particles
         “wave-particle duality”
  –Photon - particle of light that carries a
   quantum of energy
            C. Quantum Theory
 The energy of a   photon is proportional to its
 frequency.
                E = h
   E: energy (J, joules)
   h: Planck’s constant (6.6262  10-34 J·s)
   : frequency (Hz)
             C. Quantum Theory
 • EX: Find the energy of a red photon with a
   frequency of 4.57  1014 Hz.
GIVEN:                   WORK:
E=?                      E = h
 = 4.57  1014 Hz       E = (6.6262  10-34 J·s)
h = 6.6262  10-34 J·s         (4.57  1014 Hz)
                         E = 3.03  10-19 J
Calculate the smallest amount of energy (i.e. one
quantum) that an object can absorb from yellow light
with a wavelength of 589 nm.
Energy quantum = h
So, we need to know the frequency 
         = c
          = c/
           = (3.00 x 108 m/s)/(589 x 10-9 m)
           = 5.09 x 1014 s-1
plugging into Planck's equation:
E = (6.63 x 10-34 Js)*( 5.09 x 1014 s-1)
E (1 quanta) = 3.37 x 10-19 J
           C. Quantum Numbers
• Four Quantum Numbers:
  – Specify the “address” of each electron in an atom
            C. Quantum Numbers
1. Principal Quantum Number ( n )
  – Energy level
  – Size of the orbital
  – n2 = no. of orbitals in
    the energy level
              C. Quantum Numbers
   corresponds to n from Bohr model
   describes energy level and size of orbital
   n = 1, 2, 3, ...
   as n increases,
     orbitals get larger
     orbital energy increases
           C. Quantum Numbers
2. Angular Momentum Quantum ( l )
  – Energy sublevel
  – Shape of the orbital
 s             p
                           d        f
               C. Quantum Numbers
    l = Orbital angular momentum quantum
   describes shape of orbital
   l can have integral values from 0 to n-1
   l values describe a specific shape of orbital:
         if    l=    0     1     2    3
                     s     p     d    f
             C. Quantum Numbers
   n    = no. of sublevels per level
   n2   = no. of orbitals per level
   Sublevel sets: 1s, 3p, 5d, 7f
        C. Quantum Numbers
3. Magnetic Quantum Number ( ml )
  – Orientation of orbital
  – Specifies the exact orbital
    within each sublevel
              C. Quantum Numbers
          ml = magnetic quantum
   describes orientation of orbital in space
   ml can have integral values from -l to +l
     C. Quantum Numbers
px           py           pz
          C. Quantum Numbers
• Orbitals combine to form a spherical shape.
                                          2s
    2px
      2py                           2pz
Quantum Number Relationships
   Orbital Energy Levels for Hydrogen
Orbitals with same n are degenerate (at same energy)
          C. Quantum Numbers
           Multi-Electron Atoms
   Schrödinger equation can be solved only for
    hydrogen atom (a one electron system)!
   For other multi-electron atoms, assume
    orbitals are hydrogen-like.
     Orbital Energy Levels in Multi-Electron Atoms
For multi-electron atoms, orbitals with same n are NOT degenerate
                    For same n, s < p < d < f
          C. Quantum Numbers
4. Spin Quantum Number ( ms )
  – Electron spin  +½ or -½
  – An orbital can hold 2 electrons that spin in
    opposite directions.
          C. Quantum Numbers
  ms = electron spin quantum number
ms = +½   or   -½
      spin-up spin-
 down
                 
        C. Quantum Numbers
         Rules for Electrons
• Aufbau Principle
• Pauli Exclusion Principle
• Hund’s Rule
        C. Quantum Numbers
         Aufbau Principle
Aufbau is German for “building up”
Electrons enter orbitals of
lowest energy first.
                 General Rules
• Aufbau Principle
  – Electrons fill the
    lowest energy
    orbitals first.
  – “Lazy Tenant
    Rule”
     C. Quantum Numbers
   Pauli Exclusion Principle
An atomic orbital may at
most describe two electrons.
          C. Quantum Numbers
• Pauli Exclusion Principle
  – No two electrons in an atom can have the same
    4 quantum numbers.
  – Each e- has a unique “address”:
   1. Principal Q. N.         energy level
                              sublevel (s,p,d,f)
     
                              orbital
   2. Ang. Mom. Q. N.
                              electron
     
               General Rules
• Pauli Exclusion Principle
  – Each orbital can hold TWO electrons with opposite
   spins.
      C. Quantum Numbers
          Hund’s Rule
When electrons occupy orbitals
of equal energy,
 – one electron enters each orbital
 – until all the orbitals contain one
  electron with parallel spins.
                General Rules
• Hund’s Rule
  – Within a sublevel, place one e- per orbital before
    pairing them.
  – “Empty Bus Seat Rule”
    WRONG                              RIGHT
Electron Configuration
     Notation for Electron Distribution
Here we see the           Principle Quantum Number
electron configuration
for the element
HELIUM 
                         1s
                          2     Number of Electrons
                 Angular Momentum
  Principle quantum number ‘n’
 The large number "1" refers to the
principle quantum number "n"
              1s   2
which stands for the energy level.  It tells
us that the electrons of helium occupy
the first energy level of the atom.
 Angular momentum quantum number I
   The letter "s" stands for the angular
 momentum quantum number "l". 
                   1s   2
It tells us that the two electrons of the helium
electron occupy an "s" or spherical orbital.
         Total Number of Electrons
  The exponent "2" refers to the total number
  of electrons in that orbital or sub-shell. 
                     1s    2
In this case, we know that there are two electrons in the
spherical orbital at the first energy level.
Principle Quantum Number (n) and Sublevels
• The number of sublevels that an energy level
  can contain is equal to the principle quantum
  number of that level.
                         Sublevels
• The second energy level would have two sublevels,
• The third energy level would have three sublevels. 
• The first sublevel is called an s sublevel. 
• The second sublevel is called a p sublevel. 
• The third sublevel is called a d sublevel and
• the fourth sublevel is called an f sublevel. 
Although energy levels that are higher than 4 would contain
additional sublevels, these sublevels have not been named because no
known atom in its ground state would have electrons that occupy
   them
    Total Number of Orbital and Electrons per
                 Energy Level
• An easy way to calculate the number of orbitals
  found in an energy level is to use the formula n2. 
• For example, the third energy level (n=3) has a total
  of 32, or nine orbitals. 
• This makes sense because we know that the third
  energy level would have 3 sublevels; an s sublevel
  with one orbital, a p sublevel with 3 orbitals and a d
  sublevel with 5 orbitals.  1 + 3 + 5 = 9, so the formula
  n2 works!
Orbital Energy Levels in Multi-Electron Atoms
THE ULTIMATE TOOL
                  THE TOOL
• Remember to start at the beginning of each
  arrow, and then follow it all of the way to
  the end, filling in the sublevels that it passes
  through.  In other words, the order for filling
  in the sublevels becomes;
  1s, 2s, 2p, 3s, 3p, 4s, 3d, 4p, 5s, 4d, 5p, 6s, 4f,
  5d, 6p, 7s, 5f, 6d,7p.
                    Notation
• Orbital Diagram
 O
 8e-    1s              2s           2p
 Electron Configuration
             1s 2s 2p
                    2        2   4
                     Notation
• Longhand Configuration
   S 16e 1s 2s 2p 3s 3p
             -         2    2       6       2   4
 Core Electrons            Valence Electrons
 Shorthand Configuration
   S 16e         -
                      [Ne] 3s 3p2       4
              Periodic Patterns
    s
1
                                            p
2
3               d (n-1)
4
5
6
7
          6
f (n-2)   7
                          © 1998 by Harcourt Brace & Company
III. Atomic Electron Configurations
   C. Box Diagrams - Orbitals are represented by boxes and
                     electrons are represented by arrows.
          Element         Orbitals
                     1s   2s       2p
             Li
             Be
             B                             Hund’s Rule – The
             C                             most stable arrangement
                                           of electrons is that with
             N                             the maximum number of
                                           unpaired electrons, all
             O
                                           with the same spin
             F                             direction.
             Ne
III. Atomic Electron Configurations
          Element        Orbitals
                    4s              3d
            Ca
            Sc
            Ti
            V
            Cr
            Mn
            Fe
            Co
            Ni
            Cu
            Zn
III. Atomic Electron Configurations
                                                  Number of electrons in orbital
   D. spdf Notation -              1s1
                  electron shell (n)     Orbital type (l)
          Element               Orbitals                    spdf notation
                        1s      2s       2p
             Li                                               1s2 2s1
             Be                                               1s2 2s2
             B                                                1s2 2s2 2p1
             C                                                1s2 2s2 2p2
             N                                                1s2 2s2 2p3
             O                                                1s2 2s2 2p4
             F                                                1s2 2s2 2p6
             Ne                                               1s2 2s2 2p6
III. Atomic Electron Configurations
                                                  Number of electrons in orbital
   D. spdf Notation -              1s1
                  electron shell (n)     Orbital type (l)
          Element             Orbitals                      spdf notation
                           3s     3p
             Na                                               [Ne] 1s2 2s1
             Mg                                               [Ne] 1s2 2s2
             Al                                               [Ne] 1s2 2s2 2p1
             Si                                               [Ne] 1s2 2s2 2p2
             P                                                [Ne] 1s2 2s2 2p3
             S                                                [Ne] 1s2 2s2 2p4
             Cl                                               [Ne] 1s2 2s2 2p6
             Ar                                               [Ne] 1s2 2s2 2p6
       Electron Configuration
              Examples
Write ground state electron configurations
(using noble gas notation) for the following:
 a) potassium, K
                     (Z=19) [Ar] 4s1
 b) iodine, I
                     (Z=53) [Kr] 5s2 4d10 5p5
 c) bismuth, Bi
                    (Z=83) [Xe] 6s2 4f14 5d10 6p3
Some Electron Configuration Exceptions
   Chromium, Cr (Z=24)
        expected: [Ar]4s2 3d4
        actual: [Ar] 4s1 3d5
   Copper, Cu (Z=29)
        expected: [Ar] 4s2 3d9
        actual: [Ar] 4s1 3d10
               Why Exceptions?
   Recall: energy levels get closer in energy as
    n increases.
   Also, special stability of filled or half-filled
    subshells.
                     Stability
• Electron Configuration Exceptions
   Copper
     EXPECT:               [Ar] 4s2 3d9
     ACTUALLY:      [Ar] 4s1 3d10
   Copper gains stability with a full
   d-sublevel.
                     Stability
• Electron Configuration Exceptions
   Chromium
     EXPECT:               [Ar] 4s2 3d4
     ACTUALLY:   [Ar] 4s1 3d5
   Chromium gains   stability with a half-full d-
   sublevel.
Electrons in Subshells - a Closer Look
         N (Z=7): 1s2 2s2 2p3
          1s    2s       2p
        Paramagnetic vs Diamagnetic
   Paramagnetic - at least one unpaired electron.
   Diamagnetic - all electrons are paired.
   Paramagnetic species are attracted to a magnetic
    field.
   Diamagnetic species are repelled by a magnetic
    field.
     Electron Configurations for Ions
   Metals lose e- and nonmetals gain e-.
   Write configuration for parent atom, then
    add or remove electrons in outermost shell.
   ex: Fe3+
         Fe (Z=26)     [Ar]4s2 3d6
         Fe3+          [Ar] 3d5
  Core Electrons vs Valence Electrons
    core electrons - electrons in inner shells
    valence electrons - electrons in outer shell
             Cl (Z=17): [Ne] 3s2 3p5
                               valence electrons
           core electrons
Most chemical reactions only involve valence electrons!