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Some of this weeks seminars: Dynamical Studies of the Photodissociation of Ozone: From the Near IR to the VUV February 12 | 4-5 p.m. | Pitzer Auditorium,

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Presentation on theme: "Some of this weeks seminars: Dynamical Studies of the Photodissociation of Ozone: From the Near IR to the VUV February 12 | 4-5 p.m. | Pitzer Auditorium,"— Presentation transcript:

1 Some of this weeks seminars: Dynamical Studies of the Photodissociation of Ozone: From the Near IR to the VUV February 12 | 4-5 p.m. | Pitzer Auditorium, 120 Latimer Hall Dr. Reinhard Schinke, Max-Planck-Institut fuer Dynamik und Selbstorganisation, Goettingen, Germany Engineering Organic-to-Semiconductor Heterojunctions February 13 | 4-5 p.m. | Pitzer Auditorium, 120 Latimer Hall Professor Thomas F. Kuech, Dept. of Chemical & Biological Engineering, University of Wisconsin - Madison Using Supported Lipid Bilayers as a Separation Matrix February 15 | 4-5 p.m. | 775A Tan Hall Professor Paul Cremer, Dept. of Chemistry, Texas A & M University Dynamical Studies of the Photodissociation of Ozone: From the Near IR to the VUVPitzer Auditorium, 120 Latimer Hall Dr. Reinhard Schinke Engineering Organic-to-Semiconductor HeterojunctionsPitzer Auditorium, 120 Latimer Hall Professor Thomas F. Kuech Using Supported Lipid Bilayers as a Separation MatrixTan Hall Professor Paul Cremer

2 Absorption/Emission

3 Connections between the rates of stimulated and spontaneous emission: Case a) Thermal equilibrium in a cavity A 21 B 12 W(  )B 21 W(  ) E 2,N 2,g 2 E 1,N 1,g 1 W(  ), the energy density and A,B the Einstein A and B coefficients which are the rate constants (per molecule), excepting the energy density for the transition probability, W if. Also N large so we need not consider statistics. At equilibrium dN 1 /dt = -dN 2 /dt = 0 = N 2 A 21 -N 1 B 12 W(  )+N 2 B 21 W(  )

4 Connect A and B to Golden Rule

5

6 The two expressions are equal at all T only if: Comparing again to Planck’s Law T=300K at =50  m, 6THz, 200 cm -1 Longer wavelengths stimulated exceeds spontaneous rate Shorter stimulated emission is slow compared to spontaneous rate

7 Case b) A light source, Now W is not thermal energy density but the energy density of the light source (assumed to be large enough that we can neglect the thermal field). At the stimulated and spontaneous rates are equal. Consider visible light of frequency 5x10 14 Hz, 3x10 -19 J Intensity obtained by,multiplying by c is 3x10 -6 d  W/m 2 d  for an ordinary spectroscopic light source is ~10 11 Hz The intensity required to equalize spontaneous and stimulated emission rates is ~10 5 W/m 2

8 I (W/m 2 )E(V/m)n/V(m -3 ) Photons/mode Strong Hg Lamp 10 4 10 3 10 14 10 -2 cw laser 10 5 10 4 10 1510 pulsed laser (ns) 10 13 10 8 10 23 10 18 Some light sources Footnote: Derivation of relations between A, B, assumed thermal radiation. The relations hold so long as either the radiation field or the molecules are randomly oriented in space—not necessarily for solids interacting with lasers.

9 A 21 B 12 W(  )B 21 W(  ) E 2,N 2,g 2 E 1,N 1,g 1 dN 1 /dt = -dN 2 /dt = N 2 A 21 + (N 2 -N 1 ) B 12 W(  ) N 2 +N 1 =N absorption negligible

10 Expanding the exponential as 1-(A+2BW)t

11 time N 2 /N Why this behavior?

12 BW/A N 2 /N 1 4 Steady state value What is the limiting ratio?

13 How does this connect to Beer’s Law? Recall I=I 0 e -N  l =I 0 2.30310 -  Cl g( ) a normalized lineshape function n index of refraction

14 The square of the transition dipole can be expressed as an integral (over all frequencies) of the absorption cross- section (or molar absorptivity).

15 What happens when we increase [ ] vs. I? (Discussion)

16 Breakdown of Beer’s Law. BW/A>>1 Intensity falls off linearly with distance in absorber not exponentially and is independent of I 0

17 Oscillator Strength (CH4.4.3) f if =1; 1 electron allowed transition >1 multiple transitions =0.001-0.01; forbidden transitions


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