Astrophysics (Index)About

Eddington approximation

(approximation of a star's internal EMR's divergence from isotropic)

The Eddington approximation is a well-defined, relatively-easy-to-work-with description of electromagnetic radiation's variation by direction (anisotropy, departure from isotropic), used in modeling stellar structure. Assuming isotropy could make modeling even simpler, but would fail to (realistically?) transfer energy toward the surface where it is emitted as starlight. The Eddington approximation assumes there is a general transfer of energy away from the middle of the star ("up"), and models the intensity of radiation in each direction such as to do that, with tractable complication to equations that would presume isotropy. It is one of the approximations developed to make the modeling of stars practical.

(physics,EMR,stars,radiative transfer)
Further reading:

Referenced by pages:
gray atmosphere
equation of radiative transfer (RTE)
stellar structure
two-stream approximation