Generalizations of reaction rate integrals with applications to nuclear synthesis in astrophysics and some corrections to published literature

Details Generalizations of reaction rate integrals with applications to nuclear synthesis in astrophysics and some corrections to published literature Generalizations of reaction rate integrals with applications to nuclear synthesis in astrophysics and some corrections to published literature

May 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993ap%26ss.203...43a&link_type=abstract

Astrophysics and Space Science (ISSN 0004-640X), vol. 203, no. 1, p. 43-52.

Astronomy and Astrophysics

Astrophysics

Integral Equations, Nuclear Chemistry, Reaction Kinetics, Space Plasmas, Stellar Models, Maxwell Equation, Mellin Transforms, Stellar Evolution, Synthesis (Chemistry)

Scientific paper

Under the Maxwell-Boltzmann approach, the study of nuclear reactions in dense astrophysical plasmas under various cases (such as resonant, non-resonant, modified non-resonant, non-resonant under electron screening, and so on) leads to a class of complicated reaction rate integrals. It is shown that this general class of integrals can be identified with an integral involving the product of two H-functions. This latter integral is evaluated in this article, and following Buschman (1979), several similar results in the published literature are shown to be incorrect.

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