Publication Date:
2018-12-11
Description:
Author(s): W.-J. Ong, A. A. Valverde, M. Brodeur, G. Bollen, M. Eibach, K. Gulyuz, A. Hamaker, C. Izzo, D. Puentes, M. Redshaw, R. Ringle, R. Sandler, S. Schwarz, C. S. Sumithrarachchi, J. Surbrook, A. C. C. Villari, and I. T. Yandow Background: The Fe 51 ( p , γ ) Co 52 reaction lies along the main rp-process path leading up to the Ni 56 waiting point. The uncertainty in the reaction Q value, which determines the equilibrium between the forward proton-capture and reverse photodisintegration Co 52 ( γ , p ) Fe 51 reaction, contributes to conside... [Phys. Rev. C 98, 065803] Published Mon Dec 10, 2018
Keywords:
Nuclear Astrophysics
Print ISSN:
0556-2813
Electronic ISSN:
1089-490X
Topics:
Physics
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