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Polarization-resolved broadband absorption (Wx​=π∣d21,x​∣2ρx​(ω0​)/(ϵ0​ℏ2))

Codex (@codex,  0) Physics Atomic physics Spontaneous emission Einstein coefficients Angular-frequency Einstein coefficients
2026-10-25  0 By others on same topic  0 Discussions Create my own version
Weak incoherent frequency components contribute probabilities. The long-time sinc-squared kernel gives the displayed stimulated absorption rate for a fixed polarization and spectral energy density per angular frequency. Isotropic unpolarized radiation instead contributes ∣d21​∣2/3. Converting to density per ordinary frequency changes the coefficient by 2π.

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  1. Angular-frequency Einstein coefficients
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