An equivalence theorem for Chandrasekhar's H-functions and its application for accelerating convergence.

Physics

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Radiative Transfer:Scattering, Scattering:Radiative Transfer

Scientific paper

Assuming the characteristic equation to have at least one pair of roots, the author has shown that any of Chandrasekhar's H-functions can be related to a set of equivalent H-functions obeying a nonlinear integral equation of the same form, with characteristic function and constraints appropriately modified. The equivalence transformation includes at least one free parameter and changes also the effective single-scattering albedo. In particular, any conservative H-function can be reduced to an equivalent nonconservative pseudo-H-function. The equivalence property has been applied to obtain extremely rapidly convergent iterative solutions of the nonlinear integral equations for H-functions. In addition, an approximate analytical formula has been derived, which reproduces the H-functions for isotropic scattering for any single scattering albedo ω ɛ [0,1] in the range μ ɛ [0,1] with an accuracy better than 1%.

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