3. Of all the transitions that are allowed, how do I figure out intensities?

4. good Franck-Condon overlap:
more likely
poor Franck-Condon overlap:
less likely

5. Spectrum observed is built from all Franck-Condon permitted transitions.
Intensity of each possible transition is proportional to overlap of vibrational wavefunctions squared: Sfi2

6. What might cause these surfaces to have no displacement?
Relative displacement of potential curves involved in electronic transition can change.
What might cause these surfaces to have no displacement?
What might cause these surfaces to be displaced?
Displacement effects the shape of electronic spectrum observed.

8. Notice unit on x-axis and its direction

9. What is Q for the electronic spectrum
of Benzene shown on the last slide?
Some nuclear coordinate that changes substantially between ground and excited state…
How can you tell this looking at spectrum?

10. Set of p-molecular orbitals derived from LCAO of pure p-orbitals on each carbon coming out of plane of ring (Hückel Theory).
Configurations:
Yground: p12 p22 p32
Yexcited:
p12 p22 p31 p41 or
p12 p22 p32 p51 or
p12 p21 p32 p41 or
p12 p21 p32 p51
So again, what could be the origin of displaced potential energy surfaces and what is Q?

11. Surfaces displaced even further
Remember that higher vibrational wavefunctions spend most of their time (higher probability) at the classical turning points.
Have we seen this type of picture?
What kind of surface is this excited state?
Are transitions allowed above the dissociation limit?

13. An interesting case where spectroscopy reveals an unbound state.

14. One important question: where does the transition come from?
What is the role of temperature?
Remember Boltzman statistics based on our vibrational spacing in the ground state will determine what vibrational states are populated and therefore what transitions are allowed and seen.

15. Rates of non-radiative relaxation in the excited-state are frequently higher than the rates of radiative (emissive relaxation).
What does this mean, i.e. where does emission come from?
Emissive transitions, like absorptive ones, are vertical. This leads to Stokes shift.

17. Observation of the Stokes shift.
Emission
Absorption

18. Origin of Fluorescence versus Phosphorescence
S0 = ground state singlet
S1 = first singlet excited state
S2 = second singlet excited state
T1 = first triplet excited state