Neutrino-nucleus reactions in core-collapse supernovae

被引：5
作者：
Langanke, K. [1 ]
机构：
[1] GSI Darmstadt, Darmstadt, Germany
[2] Tech Univ Darmstadt, Darmstadt, Germany
来源：
INTERNATIONAL WORKSHOP ON NUCLEAR PHYSICS 27TH COURSE: NEUTRINOS IN COSMOLOGY, IN ASTRO, PARTICLE AND NUCLEAR PHYSICS | 2006年 / 57卷 / 01期
关键词：
D O I：
10.1016/j.ppnp.2005.11.027
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
Nuclear physics plays an essential role in the dynamics of a type II supernova (a collapsing star). Recent advances in nuclear many-body theory allow us now to calculate the stellar weak-interaction processes involving nuclei. The most important process is the electron capture on finite nuclei with mass numbers A > 55. This process is the source of neutrinos during the collapse phase. Neutrino-nucleus reactions occur during the collapse. They also play an interesting role during the supernova nucleosynthesis. (c) 2005 Elsevier B.V. All rights reserved.
引用
收藏
页码：324 / 333
页数：10
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