Publication Date:
2011-04-28
Description:
Author(s): A. Arcones and G. Martínez-Pinedo We use results from long-time core-collapse supernovae simulations to investigate the impact of the late time evolution of the ejecta and of the nuclear physics input on the calculated r-process abundances. Based on the latest hydrodynamical simulations, heavy r-process elements cannot be synthesize... [Phys. Rev. C 83, 045809] Published Wed Apr 27, 2011
Keywords:
Nuclear Astrophysics
Print ISSN:
0556-2813
Electronic ISSN:
1089-490X
Topics:
Physics