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 |
| Publication status | Published - 1996 Aug 26 |
| Externally published | Yes |
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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 journal › Article
}
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 -