Gravitational collapse of rotating stellar cores and supernovae

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

Research output: Contribution to journalArticle

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 languageEnglish
Pages (from-to)118-136
Number of pages19
JournalNuclear Physics A
Volume606
Issue number1-2
Publication statusPublished - 1996 Aug 26
Externally publishedYes

Fingerprint

stellar cores
gravitational collapse
supernovae
explosions
massive stars
nuclear fusion
neutron stars
neutrinos

ASJC Scopus subject areas

  • Nuclear and High Energy Physics

Cite this

Gravitational collapse of rotating stellar cores and supernovae. / Sato, K.; Shimizu, T. M.; Yamada, Shoichi.

In: Nuclear Physics A, Vol. 606, No. 1-2, 26.08.1996, p. 118-136.

Research output: Contribution to journalArticle

Sato, K, Shimizu, TM & Yamada, S 1996, 'Gravitational collapse of rotating stellar cores and supernovae', Nuclear Physics A, vol. 606, no. 1-2, pp. 118-136.
Sato, K. ; Shimizu, T. M. ; Yamada, Shoichi. / Gravitational collapse of rotating stellar cores and supernovae. In: Nuclear Physics A. 1996 ; Vol. 606, No. 1-2. pp. 118-136.
@article{c2ed2c4d49d345c5b3186701f3b86024,
title = "Gravitational collapse of rotating stellar cores and supernovae",
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.",
author = "K. Sato and Shimizu, {T. M.} and Shoichi Yamada",
year = "1996",
month = "8",
day = "26",
language = "English",
volume = "606",
pages = "118--136",
journal = "Nuclear Physics A",
issn = "0375-9474",
publisher = "Elsevier",
number = "1-2",

}

TY - JOUR

T1 - Gravitational collapse of rotating stellar cores and supernovae

AU - Sato, K.

AU - Shimizu, T. M.

AU - Yamada, Shoichi

PY - 1996/8/26

Y1 - 1996/8/26

N2 - 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.

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.

UR - http://www.scopus.com/inward/record.url?scp=0030602965&partnerID=8YFLogxK

UR - http://www.scopus.com/inward/citedby.url?scp=0030602965&partnerID=8YFLogxK

M3 - Article

VL - 606

SP - 118

EP - 136

JO - Nuclear Physics A

JF - Nuclear Physics A

SN - 0375-9474

IS - 1-2

ER -