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Electronic Structure of Atoms

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Title: Electronic Structure of Atoms


1
Electronic Structure of Atoms
  • Chapter 6 in Brown LeMay

2
The Physics of Light
  • Until 1900s light was considered a wave
  • During the 1900s, light is considered a particle
    also

3
Electromagnetic Wave
4
General Wave Characteristics
  • Amplitude height from origin to peak
  • This is intensity for light and loudness for sound

5
Wavelength
  • Distance from one point to the next identical
    point (could be peak to peak for example)
  • Units are meters/cycle
  • Symbol ?
  • Called lambda

6
Frequency
  • Speed of oscillation
  • Example how many water waves pass your eye per
    second
  • Unit is cycles/second, also called hertz
  • 1 hertz 1 cycle per second 1/seconds
  • Symbol f or nu

7
Speed (v)
  • Speed of a wave is the rate that it travels
    through space
  • Speed of all EM waves c
  • C 3.00 X 108 m/s
  • V wavelength X frequency ?f
  • Units meters X cycles
  • --------------------- m/s
  • cycles X second

8
Animation
  • http//www.surendranath.org/Applets/Waves/Twave01/
    Twave01Applet.html

9
EM Spectrum
  • If speed is constant, than all EM waves must have
    varying wavelengths and frequencies
  • As wavelength goes up, frequency must go down.

10
Visible Light
11
Why does white light show colors in a prism?
  • Different wavelengths are affected differently
  • Red is spread the least largest wavelength
  • Purple is spread the most smallest wavelength

12
Light Through a Prism
13
Continuous Spectrum
  • The kind of spectrum shown when light passes
    through a prism is called a continuous spectrum
  • All wavelengths of visible light are represented
  • Rainbows are continuous

14
Exceptions
  • There were some phenomena of light that could not
    be explained by waves
  • Black-body radiation heated object glowed
    several different colors ( orange to blue to
    white)

15
Max Planck
  • First associated color with a certain frequency,
    and therefore amount of energy
  • Energy can be absorbed by atoms in discrete
    chunks called quanta (bundle in Latin
  • E hf
  • h 6.626 X 10-34 J-s
  • Nobel Prize in 1918

16
Einsteins Contribution - 1905
  • Solar cell electrons on a metallic surface are
    removed by light and a current flows
  • A certain frequency (or higher) is needed
  • Higher intensity of a lower frequency does not
    work
  • Connects this to Planck photons are bundles of
    light energy.
  • You need a threshold frequency and everything
    else higher works
  • This is called the photoelectric effect
  • His only Nobel Prize

17
Quanta and the Hydrogen Atom
  • Elements that were heated (flame tests) or
    electrified (discharge tubes) gave line spectra
    (not continuous spectra like rainbows)
  • Balmer and Rydberg did calculations to get
    wavelength (and therefore color) of each line on
    hydrogen line spectrum 9late 1800s)
  • 1/? (on board)
  • Rydbergs constant 1.096776 X 107 1/m
  • They had no clue what this meant!

18
Bohrs Explanation
  • 1. Only orbits of certain radii with definite
    enrgies are allowed
  • 2. Circular motion does not radiate enrgy and
    therefore remains stable
  • 3. Energy permitted to be absorbed or emitted is
    equal to hf.
  • Nobel Prize in 1922

19
Details
  • Energy allowed for each orbit
  • E (-2.18 X 10-18 J)(1/n2)
  • n 1, 2, 3
  • n is called principal quantum number
  • As n increases, orbit gets larger
  • Most negative energy for n 1 (called ground
    state), therefore most stable
  • Derive equation for a jump
  • Try http//www.mhhe.com/physsci/astronomy/applet
    s/Bohr/applet_files/Bohr.html

20
Problems
  • Only works for 1-electron atoms hydrogen!
    Actually, simply a mental exercise.
  • Language remains
  • Ground state
  • Jumping up and down
  • Energy is quantized

21
More Pieces to the Puzzle
  • All matter can behave as a wave or a particle!
  • de Broglie (1897 1987)
  • ? h/mv (mv is momentum)
  • Calaulate wavelength of a person
  • Calculate wavelength of an electron
  • (m 9.11 X 10-28 g, v 5.97 X 106 m/s)

22
Uncertainty Principle
  • It is inherently impossible to know both the
    exact momentum and location of an electron at the
    same time.
  • (?x) x (?mv) or h/4pi
  • If you calculate the location of an electron
    using known m and v, the error is larger than the
    size of the electron.
  • Photon explanation is simpler.
  • Location is best described as probability.

23
Quantum Mechanics
  • Schrödinger (1887 1961) equation which deals
    with both particle and wave behavior of the
    electron
  • Based upon wave functions which describes the
    place in space where electron is most likely to
    be probability density
  • Wave function is called an orbital a specific
    distribution in space

24
Quantum Mechanical Model First quantum number
  • Three numbers are used in the equations to
    describe this n,l,m
  • n is the principle quantum number
  • 1,2,3, etc.
  • Larger the n, further from the nucleus, larger
    the E value will take less to remove the
    electron.

25
Second quantum number
  • Called l
  • Values are 0 to n-1
  • Defines shape
  • This is where we get s,p,d,f
  • S 0 p 1 d 2 f 3
  • For example, how many l values for n 3?
  • What are they?

26
Third Quantum Number
  • Called m
  • This is the magnetic quantum number, which
    describes the orientation in space
  • Values are between L and L, including 0
  • For a p sublevel, what is the L?
  • What are the possible m values?

27
Continued
  • Collection of all orbitals make the electron
    shell
  • Subshell or sublevel same n and l
  • Total number of orbitals in n is n2
  • Orbitals are like nodes in wave
  • S 1
  • P 3
  • D 5
  • F 7

28
Energy within one level
  • Increases with value of L
  • All orbitals within the same L (like all d
    orbitals have equal energy
  • The term is degenerate for this
  • The last quantum number is ms or spin number
  • Pauli Exclusion Principle no two electrons can
    have the same 4 quantum numbers
  • or (½)
  • If orbital has two electrons, they have opposite
    spin.
  • Try a few

29
Electron Configuration
  • This is the distribution of electrons in various
    orbitals
  • Ground state all electrons are in lowest
    possible state
  • Simple configuration does not show orbitals
  • Try carbon

30
Orbital Diagram
  • This shows how degenerate orbitals fill also
  • Follow Hunds Rule for degenerate orbitals, the
    lowest energy is obtained when the number of
    electrons with the same spin is maximized.
  • Show carbon
  • Try iron to show order of filling
  • Read across table

31
Condensed version
  • For convenience, indicate nearest noble gas in
    brackets and continue on with the configuration
  • This clearly shows core and valence (outer)
    electrons
  • Try gold
  • Exceptions are not interesting chemically
  • Lanthanum, chromium, copper
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