Review of Mathematical Techniques Applicable in Astrophysical Reaction Rate Theory

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dc.creatorMathai, A. M.
dc.creatorHaubold, H. J.
dc.date2002-06-23
dc.date.accessioned2026-07-07T11:36:27Z
dc.date.available2026-07-07T11:36:27Z
dc.descriptionAn overview is presented on statistical techniques for the analytic evaluation of integrals for non-resonant, non-resonant depleted, non-resonant cut-off, non-resonant sccreened, and resonant thermonuclear reaction rates. The techniques are based on statistical distribution theory and the theory of Meijer's G-function and Fox's H-function. The implementation of Meijer's G-function in Mathematica constituts an additional utility for analytic manipulations and numerical computation of thermonuclear reaction rate integrals. Recent results in the astrophysical literature related to the use of analytic thermonuclear reaction rates are incorporated.
dc.description24 pages, LaTeX
dc.identifierhttps://arxiv.org/abs/math/0206239
dc.identifierhttp://arxiv.org/abs/math/0206239
dc.identifierAstrophys.SpaceSci.282:265-280,2002
dc.identifierdoi:10.1023/A:1021123124894
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/198923
dc.subjectClassical Analysis and ODEs
dc.subjectMathematical Physics
dc.titleReview of Mathematical Techniques Applicable in Astrophysical Reaction Rate Theory
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