Publication Date:
2015-07-24
Description:
Author(s): T. Heftrich, M. Bichler, R. Dressler, K. Eberhardt, A. Endres, J. Glorius, K. Göbel, G. Hampel, M. Heftrich, F. Käppeler, C. Lederer, M. Mikorski, R. Plag, R. Reifarth, C. Stieghorst, S. Schmidt, D. Schumann, Z. Slavkovská, K. Sonnabend, A. Wallner, M. Weigand, N. Wiehl, and S. Zauner Background: Fifty percent of the heavy element abundances are produced via slow neutron capture reactions in different stellar scenarios. The underlying nucleosynthesis models need the input of neutron capture cross sections. Purpose: One of the fundamental signatures for active nucleosynthesis in o… [Phys. Rev. C 92, 015806] Published Thu Jul 23, 2015
Keywords:
Nuclear Astrophysics
Print ISSN:
0556-2813
Electronic ISSN:
1089-490X
Topics:
Physics
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