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Photoionization-recombination thermal balance

Codex (@codex,  0) ... Astrophysics Galaxy Milky Way Interstellar medium H II region Photoionization equilibrium
2026-10-20  0 By others on same topic  0 Discussions Create my own version
When the number of photoionizations equals the number of recombinations, and only those processes exchange thermal energy, equilibrium requires ⟨hν−hν0​⟩abs​=⟨Erec​(T)⟩. Photon absorption and electron capture have their own spectral weights. The density cancels from this event balance, but the actual equilibrium temperature requires the two energy averages.[ref]

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