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PHOTONS IN

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Title: Slide 1 Author: UCSB Last modified by: devries Created Date: 4/10/2006 9:04:38 PM Document presentation format: On-screen Show (4:3) Company – PowerPoint PPT presentation

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Title: PHOTONS IN


1
PHOTONS IN CHEMISTRY OUT
WHY BOTHER?
2
E h ?
3
E h ?
4
?? c 3 108 m/s
5
Visible light from the sun
450-750 nm
Take 500 nm
electronic state
6
Boltzman
T oK n2/n1
300 3 x 10-42
400 7 x 10-32
1000 3.4 x 10-13
2,000 6 x 10-7
5,000 3 x 10-3
6,400 1
10,000 5.7
20,000 24
50,000 56
7
Grotthuss-Draper law Only the light absorbed in
a molecule can produce photochemical Change in
the molecule (1871 and 1841)
Stark - Einstein If a species absorbs
radiation, then one particle is excited for each
quantum of radiation absorbed
8
Stark - Einstein If a species absorbs
radiation, then one particle is excited for each
quantum of radiation absorbed
9
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10
Photochemical kinetics
11
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12
Transmittance
Absorbance
Beers Law
13
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14
NB 1 Beer fails when
photochemistry happens
NB 2 The photophysics
Is hidden in s
(So we havent done much yet)
15
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16
Absorption of a mixture
17
Photochemical kinetics
STEADY STATE HYPOTESIS
18
NB 2 The photophysics
Is hidden in s
(So we havent done much yet)
19
EINSTEIN COEFFICIENT
of transitions / second
Radiation density of photons/unit freq.
of molecules
degeneracy
20
Stimulated emission
Spontaneous emission
21
Stimulated emission
Spontaneous emission
22
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24
Boltzman
Planck
25
Oscillator strength
26
Lifetimes
Einstein coefficients are rate constants
27
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28
Heisenberg may have been here
29
Contributions to excited state lifetime
  • Natural lifetime
  • Pressure broadening
  • Saturaiton broadening
  • Doppler broadening

NB f(v) in a gas is Gaussian ?Doppler line
shape is Gausian
30
electrons
Nuclei
(depends on coordinates of electrons and
nuclei And on time)
31
NB Resonant frequency
NB 1 I f ? e0 and µ becomes permanent
dipole NB 2 ?if as beat frequency NB
3 compare to nuclear vibrations
32
Compare 1015 s-1 to IR
Nuclear motion is 2 orders of Magnitude slower
than Electronic motion
Born-Oppenheimer approximation
33
Orthogonal (no overlap)
34
Mx is odd
35
One more parameter.
a ß up down ? ? ½ -½
SPIN
36
If we can separate space and spin (no spin-orbit
coupling)
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44
Conical Intersections
E
R2
R1
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