Eddington approximation

E1989397 UNEXPLORED

The Eddington approximation is a simplifying method in radiative transfer theory that relates radiation pressure to energy density to make the equations of stellar atmospheres and interiors more tractable.

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Label	Occurrences
Eddington approximation canonical	2

Referenced by (2)

Full triples — surface form annotated when it differs from this entity's canonical label.

Milne–Eddington approximation → basedOn → Eddington approximation ⓘ

Schuster–Schwarzschild theorem → relatedTo → Eddington approximation ⓘ