Physical mechanism of core-collapse supernovae that neutrinos drive

Shoichi Yamada*, Hiroki Nagakura, Ryuichiro Akaho, Akira Harada, Shun Furusawa, Wakana Iwakami, Hirotada Okawa, Hideo Matsufuru, Kohsuke Sumiyoshi

*この研究の対応する著者

研究成果: Review article査読

2 被引用数 (Scopus)

抄録

The current understanding of the mechanism of core-collapse supernovae (CCSNe), one of the most energetic events in the universe associated with the death of massive stars and the main formation channel of compact objects such as neutron stars and black holes, is reviewed for broad readers from different disciplines of science who may not be familiar with the object. Therefore, we emphasize the physical aspects than the results of individual model simulations, although large-scale high-fidelity simulations have played the most important roles in the progress we have witnessed in the past few decades. It is now believed that neutrinos are the most important agent in producing the commonest type of CCSNe. The so-called neutrino-heating mechanism will be the focus of this review and its crucial ingredients in micro- and macrophysics and in numerics will be explained one by one. We will also try to elucidate the remaining issues.

本文言語English
ページ(範囲)190-233
ページ数44
ジャーナルProceedings of the Japan Academy Series B: Physical and Biological Sciences
100
3
DOI
出版ステータスPublished - 2024

ASJC Scopus subject areas

  • 医学一般

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