Gravitational collapse of rotating stellar cores and supernovae

被引：0
作者：
Sato, K
Shimizu, TM
Yamada, S
机构：
[1] Department of Physics, School of Science, University of Tokyo, Tokyo 113, Bunkyo-ku
来源：
NUCLEAR PHYSICS A | 1996年 / 606卷 / 1-2期
关键词：
D O I：
10.1016/0375-9474(96)00236-9
中图分类号：
O57 [原子核物理学、高能物理学];
学科分类号：
070202 ;
摘要：
As is well known, massive stars, which would be the progenitor of type II supernovae, are rapid rotators. It is obviously necessary to investigate the effects of rotation on gravitational collapse of stellar cores and supernova explosions. We review (i) rotational core collapse, (ii) jet-like explosion induced by rotation and asymmetric neutrino emission from proto-neutron-stars, and (iii) explosive nucleosynthesis when an asymmetric jet-like explosion occurs, based on our recent work.
引用
收藏
页码：118 / 136
页数：19
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