Theoretical Models for Nuclear Astrophysics

Details Theoretical Models for Nuclear Astrophysics Theoretical Models for Nuclear Astrophysics

Dec 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005omeg.conf..241d&link_type=abstract

ORIGIN OF MATTER AND EVOLUTION OF GALAXIES 2003. Held 17-19 November 2003 in RIKEN, Wako, Saitama, Japan. Edited by M Terasawa,

Astronomy and Astrophysics

Astrophysics

Scientific paper

We review and compare some theoretical models used in nuclear astrophysics: the R-matrix method, the DWBA method, and microscopic cluster models. Applications are presented. The R-matrix theory is illustrated by results of a recent compilation of reactions involved in the Big-Bang nucleosynthesis. The DWBA method is tested with the 13C(α,n)16O reaction, and is shown to be quite sensitive to the conditions of the calculation. Finally, we apply a microscopic model to the 7Be(p,γ)8B reaction, and update previous results obtained within this framework.

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