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Lecture 8: Laser amplifiers

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Transition rates<br />

<br />

In thermal equilibrium, both the blackbody radiation spectral<br />

density and the atomic population density in each energy<br />

level should reach a steady state<br />

N 2<br />

(W 21<br />

()W sp<br />

()) N 1<br />

W 12<br />

()<br />

<br />

This is the principle of detailed balance in thermal<br />

equilibrium. The steady-state population distribution in<br />

thermal equilibrium:<br />

N 2<br />

N 1<br />

<br />

W 12<br />

()<br />

W 21<br />

()W sp<br />

() <br />

B 12<br />

u()<br />

B 21<br />

u() A 21<br />

27

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