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Contribution Details
Type | Journal Article |
Scope | Discipline-based scholarship |
Title | Nuclear physics in core-collapse supernovae |
Organization Unit |
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Authors |
|
Item Subtype | Original Work |
Refereed | Yes |
Status | Published in final form |
Language |
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Journal Title | New Astronomy Reviews |
Geographical Reach | international |
ISSN | 13876473 |
Volume | 52 |
Number | 7-10 |
Page Range | 373 - 376 |
Date | 2008 |
Abstract Text | Core-collapse and the launch of a supernova explosion form a very short episode of few seconds in the evolution of a massive star, during which an enormous gravitational energy of several times 1053 erg is transformed into observable neutrino-, kinetic-, and electromagnetic radiation energy. We emphasize the wide range of matter conditions that prevail in a supernova event and sort the conditions into distinct regimes in the density and entropy phase diagram to briefly discuss their different impact on the neutrino signal, gravitational wave emission, and ejecta. |
Digital Object Identifier | 10.1016/j.newar.2008.05.006 |
Export | BibTeX |