Nuclear physics in core-collapse supernovae

被引：6

作者：

Liebendoerfer, M. ^{[1
]}

Fischer, T. ^{[1
]}

Froehlich, C. ^{[2
]}

Hix, W. R. ^{[4
]}

Langanke, K. ^{[3
]}

Martinez-Pinedo, G. ^{[3
]}

Mezzacappa, A. ^{[4
]}

Scheidegger, S. ^{[1
]}

Thielemann, F. -K. ^{[1
]}

Whitehouse, S. C. ^{[1
]}

机构：

[1] Univ Basel, Dept Phys, CH-4056 Basel, Switzerland

[2] Univ Chicago, Enrico Fermi Inst, Chicago, IL 60637 USA

[3] Gesell Schwerionenforsch mbH, D-64291 Darmstadt, GE, Germany

[4] Oak Ridge Natl Lab, Div Phys, Oak Ridge, TN 37830 USA

来源：

NEW ASTRONOMY REVIEWS | 2008年 / 52卷 / 7-10期

关键词：

Supernova; Neutron star; Neutrino transport; Gravitational wave;

D O I：

10.1016/j.newar.2008.05.006

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

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. (C) 2008 Elsevier B.V. All rights reserved.

引用

页码：373 / 376

页数：4

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