p-process nucleosynthesis: Activation ex
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J. Glorius; M. KnΓΆrzer; S. MΓΌller; N. Pietralla; A. Sauerwein; K. Sonnabend; C.
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Article
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2011
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Elsevier Science
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English
β 342 KB
For the astrophysical p process a complex reaction network has to be solved. In the order of 10,000 theoretically predicted reaction rates are needed for simulations of this network. For reactions involving Ξ± particles or protons, the predictions in the framework of the Hauser-Feshbach (HF) model w