Publication Date:
2012-03-30
Description:
Author(s): A. Palumbo, W. P. Tan, J. Görres, A. Best, M. Couder, R. Crowter, R. J. deBoer, S. Falahat, P. J. LeBlanc, H. Y. Lee, S. O'Brien, E. Strandberg, M. Wiescher, J. P. Greene, Zs. Fülöp, G. G. Kiss, E. Somorjai, N. Özkan, G. Efe, and R. T. Güray Production of proton-rich nuclei beyond iron in stars proceeds via the p process, i.e., a sequence of photodisintegration reactions, ( γ , n ), ( γ , p ), and ( γ , α ) on heavy nuclei at temperatures of 2–3×10 9 K. The involved reaction rates are typically calculated with the statistical Hauser-Feshbach (HF) mo... [Phys. Rev. C 85, 035808] Published Thu Mar 29, 2012
Keywords:
Nuclear Astrophysics
Print ISSN:
0556-2813
Electronic ISSN:
1089-490X
Topics:
Physics
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