Physical mechanism of core-collapse supernovae that neutrinos drive.

Autor:	Yamada S; Department of Physics, Faculty of Science and Engineering, Waseda University.; Research Institute for Science and Engineering, Waseda University., Nagakura H; National Astronomical Observatory of Japan., Akaho R; Department of Physics, Faculty of Science and Engineering, Waseda University., Harada A; Interdisciplinary Theoretical and Mathematical Sciences Program (iTHEMS), RIKEN., Furusawa S; College of Science and Engineering, Kanto Gakuin University., Iwakami W; Department of Physics, Faculty of Science and Engineering, Waseda University., Okawa H; Waseda Institute for Advanced Study, Waseda University., Matsufuru H; High Energy Accelerator Research Organization (KEK)., Sumiyoshi K; National Institute of Technology, Numazu College.
Jazyk:	angličtina
Zdroj:	Proceedings of the Japan Academy. Series B, Physical and biological sciences [Proc Jpn Acad Ser B Phys Biol Sci] 2024; Vol. 100 (3), pp. 190-233.
DOI:	10.2183/pjab.100.015
Abstrakt:	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.
Databáze:	MEDLINE
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