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Most phonon-assisted spectral transfer rates across an inhomogeneously broadened line are proportional to the inverse square of the energy change. The time-dependent optical emission profile is calculated exactly for a rectangular line shape for these processes. Numerical solutions are required for other line shapes (e.g., a Gaussian as found in ruby). They are exhibited as a function of time for a variety of initial excitation energies at different positions across the optical line.
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Holstein et al. (1977) studied this question.
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