Thermal equilibration: radiative and nonradiative contributions. A collection of two-level atoms in a crystal is coupled both to the electromagnetic surroundings with radiative decay rate Yrad and to the crystal-lattice surroundings with decay rate Yar. Suppose the electromagnetic surroundings are somehow held at a fixed temperature Trad which is different from the fixed temperature Tür of the crystal lattice. Derive a formula for the steady-state equilibrium value of the Boltzmann temperature Ta for the level populations of the two-level atoms in this case, as a function of the two surrounding temperatures Trad and Thr, the normalized energy gap ħw/k, and the ratio Yrad/Ynr.

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1. Thermal equilibration: radiative and nonradiative contributions. A collection of
two-level atoms in a crystal is coupled both to the electromagnetic surroundings
with radiative decay rate Yrad and to the crystal-lattice surroundings with decay
rate Ynr. Suppose the electromagnetic surroundings are somehow held at a fixed
temperature Trad which is different from the fixed temperature Tür of the crystal
lattice. Derive a formula for the steady-state equilibrium value of the Boltzmann
temperature Ta for the level populations of the two-level atoms in this case, as
a function of the two surrounding temperatures Trad and Thr, the normalized
energy gap ħw/k, and the ratio Yrad/Ynr.
Transcribed Image Text:1. Thermal equilibration: radiative and nonradiative contributions. A collection of two-level atoms in a crystal is coupled both to the electromagnetic surroundings with radiative decay rate Yrad and to the crystal-lattice surroundings with decay rate Ynr. Suppose the electromagnetic surroundings are somehow held at a fixed temperature Trad which is different from the fixed temperature Tür of the crystal lattice. Derive a formula for the steady-state equilibrium value of the Boltzmann temperature Ta for the level populations of the two-level atoms in this case, as a function of the two surrounding temperatures Trad and Thr, the normalized energy gap ħw/k, and the ratio Yrad/Ynr.
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