Gravitational collapse of rotating stellar cores and supernovae

K. Sato; T. M. Shimizu; S. Yamada

doi:10.1016/0375-9474(96)00236-9

Gravitational collapse of rotating stellar cores and supernovae

K. Sato, T. M. Shimizu, S. Yamada

Research output: Contribution to journal › Article › peer-review

Abstract

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.

Original language	English
Pages (from-to)	118-136
Number of pages	19
Journal	Nuclear Physics A
Volume	606
Issue number	1-2
DOIs	https://doi.org/10.1016/0375-9474(96)00236-9
Publication status	Published - 1996 Aug 26
Externally published	Yes

ASJC Scopus subject areas

Nuclear and High Energy Physics

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AB - 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.

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Gravitational collapse of rotating stellar cores and supernovae

Abstract

ASJC Scopus subject areas

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