Astrophysical thermonuclear functions

W. J. Anderson; H. J. Haubold; A. M. Mathai

doi:10.1007/bf00982324

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arXiv · astro-ph/9402020

Astrophysical thermonuclear functions

W. J. Anderson·H. J. Haubold·A. M. Mathai

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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.

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W. J. Anderson, H. J. Haubold, A. M. Mathai. 1994-02-08. Astrophysical thermonuclear functions. https://doi.org/10.1007/bf00982324

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