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arXiv · astro-ph/0402668

Cross section predictions for hydrostatic and explosive burning

P. Descouvemont·T. Rauscher
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Abstract

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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P. Descouvemont, T. Rauscher. 2004-02-27. Cross section predictions for hydrostatic and explosive burning. https://doi.org/10.1016/j.nuclphysa.2004.10.024

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