Astrophysical thermonuclear functions for Boltzmann–Gibbs statistics and Tsallis statistics

We present an analytic proof of the integrals for astrophysical thermonuclear functions which are derived on the basis of Boltzmann–Gibbs statistical mechanics. Among the four different cases of astrophysical thermonuclear functions, those with a depleted high-energy tail and a cut-off at high energies find a natural interpretation in q-statistics.

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Year of publication:	2004
Authors:	Saxena, R.K. ; Mathai, A.M. ; Haubold, H.J.
Published in:	Physica A: Statistical Mechanics and its Applications. - Elsevier, ISSN 0378-4371. - Vol. 344.2004, 3, p. 649-656
Publisher:	Elsevier
Subject:	Kinetic theory \| Solar neutrinos \| Nuclear reactions \| Special functions

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Type of publication:	Article
Source:	RePEc - Research Papers in Economics

Persistent link: https://www.econbiz.de/10010588702