Cross section predictions for hydrostatic and explosive burning

Details Cross section predictions for hydrostatic and explosive burning Cross section predictions for hydrostatic and explosive burning

2004-02-27

arxiv.org/abs/astro-ph/0402668v1

Nucl.Phys. A777 (2006) 137-156

Astronomy and Astrophysics

Astrophysics

25 pages, 3 figures, invited article to appear in Nucl. Phys. A

Scientific paper

10.1016/j.nuclphysa.2004.10.024

We review different models used for reactions involved in nuclear astrophysics. The reaction rate is defined for resonant as well as for non-resonant processes. For low-density nuclei, we describe the DWBA method, the potential model, the R-matrix method, and microscopic cluster models. The statistical model is developed for high-level densities. Details of calculations in the low- and high-density regimes are illustrated with new results concerning transfer reactions and level densities.

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