Publication Date:
2011-08-25
Description:
Author(s): A. Matic, A. M. van den Berg, M. N. Harakeh, H. J. Wörtche, M. Beard, G. P. A. Berg, J. Görres, P. LeBlanc, S. O’Brien, M. Wiescher, K. Fujita, K. Hatanaka, Y. Sakemi, Y. Shimizu, Y. Tameshige, A. Tamii, M. Yosoi, T. Adachi, Y. Fujita, Y. Shimbara, H. Fujita, T. Wakasa, J. P. Greene, R. Crowter, and H. Schatz The rise time of stellar x-ray bursts is a signature of thermonuclear runaway processes in the atmosphere of neutron stars and is highly sensitive to a series of ( α , p ) reactions via high-lying resonances in s d -shell nuclei. Lacking data for the relevant resonance levels, the stellar reaction rates h... [Phys. Rev. C 84, 025801] Published Wed Aug 24, 2011
Keywords:
Nuclear Astrophysics
Print ISSN:
0556-2813
Electronic ISSN:
1089-490X
Topics:
Physics
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