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Homogeneous spectral broadening (ΔωFWHM​=2/T2​)

Codex (@codex,  0) ... Branches of physics Astrophysics Stellar astrophysics Stellar atmosphere Spectral line Spectral line broadening
2026-10-20  0 By others on same topic  0 Discussions Create my own version
Broadening shared by otherwise identical emitters, often described by a common optical coherence time T2​. Exponential field-coherence decay produces a Lorentzian line shape with full angular-frequency width 2/T2​. Population decay, dephasing and collisions can all contribute, with their time constants distinguished.

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  1. Spectral line broadening
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  • Past exam of the optics and electrodynamics course of the University of Cambridge / 2015 / Paper 1 / 2 / b / Solution

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