PHOTONS IN - PowerPoint PPT Presentation

1 / 44
About This Presentation
Title:

PHOTONS IN

Description:

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

Number of Views:34
Avg rating:3.0/5.0
Slides: 45
Provided by: UCSB
Category:

less

Transcript and Presenter's Notes

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
(No Transcript)
10
Photochemical kinetics
11
(No Transcript)
12
Transmittance
Absorbance
Beers Law
13
(No Transcript)
14
NB 1 Beer fails when
photochemistry happens
NB 2 The photophysics
Is hidden in s
(So we havent done much yet)
15
(No Transcript)
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
(No Transcript)
23
(No Transcript)
24
Boltzman
Planck
25
Oscillator strength
26
Lifetimes
Einstein coefficients are rate constants
27
(No Transcript)
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)
37
(No Transcript)
38
(No Transcript)
39
(No Transcript)
40
(No Transcript)
41
(No Transcript)
42
(No Transcript)
43
(No Transcript)
44
Conical Intersections
E
R2
R1
Write a Comment
User Comments (0)
About PowerShow.com