Publication Date:
2016-05-11
Description:
Author(s): R. Talwar, T. Adachi, G. P. A. Berg, L. Bin, S. Bisterzo, M. Couder, R. J. deBoer, X. Fang, H. Fujita, Y. Fujita, J. Görres, K. Hatanaka, T. Itoh, T. Kadoya, A. Long, K. Miki, D. Patel, M. Pignatari, Y. Shimbara, A. Tamii, M. Wiescher, T. Yamamoto, and M. Yosoi Background: The Ne 22 ( α , n ) Mg 25 reaction is the dominant neutron source for the slow neutron capture process ( s process) in massive stars, and contributes, together with C 13 ( α , n ) O 16 , to the production of neutrons for the s process in asymptotic giant branch (AGB) stars. However, the reaction is endoth… [Phys. Rev. C 93, 055803] Published Tue May 10, 2016
Keywords:
Nuclear Astrophysics
Print ISSN:
0556-2813
Electronic ISSN:
1089-490X
Topics:
Physics
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