Astrophysical thermonuclear functions for Boltzmann-Gibbs statistics and Tsallis statistics

被引：15

作者：

Saxena, RK

Mathai, AM

Haubold, HJ

机构：

[1] UN, Off Outer Space Affairs, A-1400 Vienna, Austria

[2] Jai Narain Vyas Univ, Dept Math & Stat, Jodhpur 342001, Rajasthan, India

[3] McGill Univ, Dept Math & Stat, Montreal, PQ H3A 2K6, Canada

来源：

PHYSICA A-STATISTICAL MECHANICS AND ITS APPLICATIONS | 2004年 / 344卷 / 3-4期

关键词：

kinetic theory; solar neutrinos; nuclear reactions; special functions;

D O I：

10.1016/j.physa.2004.06.047

中图分类号：

O4 [物理学];

学科分类号：

0702 ;

摘要：

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. (C) 2004 Elsevier B.V. All rights reserved.

引用

页码：649 / 656

页数：8

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