Astrophysical Thermonuclear Functions for Boltzmann-Gibbs Statistics and Tsallis Statistics
arXiv:math-ph/0406049 · doi:10.1016/j.physa.2004.06.047
Abstract
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.
10 pages, LaTeX