Astrophysical thermonuclear functions
Astrophysics
2009-10-22 v1
Abstract
As theoretical knowledge and experimental verification of nuclear cross sections increases it becomes possible to refine analytic representations for nuclear reaction rates. In this paper mathematical/statistical techniques for deriving closed-form representations of thermonuclear functions are summarized and numerical results for them are given.The purpose of the paper is also to compare numerical results for approximate and closed-form representations of thermonuclear functions.
Cite
@article{arxiv.astro-ph/9402020,
title = {Astrophysical thermonuclear functions},
author = {W. J. Anderson and H. J. Haubold and A. M. Mathai},
journal= {arXiv preprint arXiv:astro-ph/9402020},
year = {2009}
}
Comments
17 pages in LaTeX, 8 figures available on request from [email protected]