Publication Date:
2017-05-12
Description:
Author(s): A. M. Long, T. Adachi, M. Beard, G. P. A. Berg, Z. Buthelezi, J. Carter, M. Couder, R. J. deBoer, R. W. Fearick, S. V. Förtsch, J. Görres, J. P. Mira, S. H. T. Murray, R. Neveling, P. Papka, F. D. Smit, E. Sideras-Haddad, J. A. Swartz, R. Talwar, I. T. Usman, M. Wiescher, J. J. Van Zyl, and A. Volya The Ar 34 ( α , p ) K 37 reaction is believed to be one of the last in a sequence of ( α , p ) and ( p , γ ) reactions within the T z = − 1 , s d -shell nuclei, known as the α p -process. This process is expected to influence the shape and rise times of luminosity curves coming from type I x-ray bursts (XRBs). With very lit… [Phys. Rev. C 95, 055803] Published Wed May 10, 2017
Keywords:
Nuclear Astrophysics
Print ISSN:
0556-2813
Electronic ISSN:
1089-490X
Topics:
Physics
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