Publication Date:
2012-04-12
Description:
Author(s): T. Fischer, G. Martínez-Pinedo, M. Hempel, and M. Liebendörfer The neutrino-driven wind, which occurs after the onset of a core-collapse supernova explosion, has long been considered as the possible site for the synthesis of heavy r -process elements in the Universe. Only recently, it has been possible to simulate supernova explosions up to ∼10 seconds , based o... [Phys. Rev. D 85, 083003] Published Wed Apr 11, 2012
Keywords:
Astrophysics & Cosmology
Print ISSN:
0556-2821
Electronic ISSN:
1089-4918
Topics:
Physics
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