Nuclear physics in core-collapse supernovae

Détails

ID Serval
serval:BIB_583CEA430C30
Type
Article: article d'un périodique ou d'un magazine.
Collection
Publications
Titre
Nuclear physics in core-collapse supernovae
Périodique
New Astronomy Reviews
Auteur(s)
Liebendörfer M., Fischer T., Fröhlich C., Hix W.R., Langanke K., Martinez-Pinedo G., Mezzacappa A., Scheidegger S., Thielemann F.-K., Whitehouse S.C.
ISSN
1387-6473
Statut éditorial
Publié
Date de publication
10/2008
Peer-reviewed
Oui
Volume
52
Numéro
7-10
Pages
373-376
Langue
anglais
Résumé
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 10^53 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.
Mots-clé
Supernova, Neutron star, Neutrino transport, Gravitational wave
Web of science
Création de la notice
06/11/2018 10:07
Dernière modification de la notice
20/08/2019 15:12
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