Abstract
We obtain a new representation of Chandrasekhar'sH-functionsH(z) corresponding to the dispersion functionT(z) = |δ rs −f rs (z)|, [f rs (z)] is of rank one.H(z) is obtained in the form
WhereP r x(=ø r (x)/H(x)) is continuous onE r which are subsets of [0, 1].A o ,A 1 are determinable constants andK is the positive root ofT(z),ø r (x) are known functions. From this formH(z) is then obtained in terms of a Fredholm type integral equation. This new form ofH(z) has proved to be very useful in solving coupled integral equations involvingX-,Y-functions of transport problems.P r(x) can be replaced by approximating polynomials whose coefficients can be determined as functions of the moments of known functions; a closed form approximation ofH(z) to a sufficiently high degree of accuracy is then readily available by term integrations.
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References
Chandrasekhar, S.: 1950,Radiative Transfer, Clarendon Press, Oxford.
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Kourganoff, V.: 1952,Basic Methods in Transfer Problems, Clarendon Press, Oxford, art. 29.8.
Muskhelishvili, N. I.: 1946,Singular Integral Equations, English Translation (1953), P. Noordhoff, Ltd., Groningen, Holland, Chapters 1 and 2.
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Das Gupta, S.R. A new representation of theH-functions of radiative transfer. Astrophys Space Sci 50, 187–203 (1977). https://doi.org/10.1007/BF00648531
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DOI: https://doi.org/10.1007/BF00648531