Abstract
Radiationless transitions of a solute molecule embedded in a crystalline solvent are treated in close analogy to radiative transitions. A semiclassical interaction Hamiltonian employing empirically determined coupling constants connects solute particles to a force field amplitude set up by the phonons of the solvent. By relating this amplitude to phonon energy density an Einstein B coefficient is derived. Debye's formula for the phonon energy density combined with thermodynamic arguments yield Einstein A coefficients. It is shown that the theory (1) explains the fast rates of radiationless transitions, (2) provides for temperature dependence, (3) has a cutoff frequency for radiationless transition, (4) provides for the Franck—Condon principle, and (5) explains the lack of selection rules. A value is derived for the empirical coupling constants.
References
10
Referenced
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Dates
Type | When |
---|---|
Created | 20 years, 7 months ago (Jan. 5, 2005, 10:19 p.m.) |
Deposited | 1 year, 6 months ago (Feb. 8, 2024, 3:44 p.m.) |
Indexed | 1 week ago (Aug. 26, 2025, 2:26 a.m.) |
Issued | 63 years, 3 months ago (June 1, 1962) |
Published | 63 years, 3 months ago (June 1, 1962) |
Published Print | 63 years, 3 months ago (June 1, 1962) |
@article{Gouterman_1962, title={Radiationless Transitions: A Semiclassical Model}, volume={36}, ISSN={1089-7690}, url={http://dx.doi.org/10.1063/1.1732389}, DOI={10.1063/1.1732389}, number={11}, journal={The Journal of Chemical Physics}, publisher={AIP Publishing}, author={Gouterman, Martin}, year={1962}, month=jun, pages={2846–2853} }