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タイトル: Coalescence of black hole–neutron star binaries
著者: Kyutoku, Koutarou
Shibata, Masaru  kyouindb  KAKEN_id  orcid https://orcid.org/0000-0002-4979-5671 (unconfirmed)
Taniguchi, Keisuke
著者名の別形: 久德, 浩太郎
柴田, 大
キーワード: Numerical relativity
Black holes
Neutron stars
Gravitational waves
Gamma-ray burst
Nucleosynthesis
発行日: Dec-2021
出版者: Springer Nature
誌名: Living Reviews in Relativity
巻: 24
号: 1
論文番号: 5
抄録: We review the current status of general relativistic studies for coalescences of black hole–neutron star binaries. First, high-precision computations of black hole–neutron star binaries in quasiequilibrium circular orbits are summarized, focusing on the quasiequilibrium sequences and the mass-shedding limit. Next, the current status of numerical-relativity simulations for the merger of black hole–neutron star binaries is described. We summarize our understanding for the merger process, tidal disruption and its criterion, properties of the merger remnant and ejected material, gravitational waveforms, and gravitational-wave spectra. We also discuss expected electromagnetic counterparts to black hole–neutron star coalescences.
著作権等: © The Author(s) 2021
This article is licensed under a Creative Commons Attribution 4.0 International License, which permits use, sharing, adaptation, distribution and reproduction in any medium or format, as long as you give appropriate credit to the original author(s) and the source, provide a link to the Creative Commons licence, and indicate if changes were made. The images or other third party material in this article are included in the article's Creative Commons licence, unless indicated otherwise in a credit line to the material. If material is not included in the article's Creative Commons licence and your intended use is not permitted by statutory regulation or exceeds the permitted use, you will need to obtain permission directly from the copyright holder.
URI: http://hdl.handle.net/2433/276920
DOI(出版社版): 10.1007/s41114-021-00033-4
出現コレクション:学術雑誌掲載論文等

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