Publikationsdatum:
2018-03-17
Beschreibung:
Author(s): M. Weigand, T. Heftrich, Ch. E. Düllmann, K. Eberhardt, S. Fiebiger, J. Glorius, K. Göbel, R. Haas, C. Langer, S. Lohse, R. Reifarth, D. Renisch, and C. Wolf Background: About 50% of the heavy elements are produced in stars during the slow neutron capture process. The analysis of branching points allows to set constraints on the temperature and the neutron density in the interior of stars. The temperature dependence of the branch point Tm 171 is weak. Hen... [Phys. Rev. C 97, 035803] Published Fri Mar 16, 2018
Schlagwort(e):
Nuclear Astrophysics
Print ISSN:
0556-2813
Digitale ISSN:
1089-490X
Thema:
Physik
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