Coalescence of black hole–neutron star binaries
Bibliographic Information
- Other Title
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- Solar Flares: Magnetohydrodynamic Processes
Abstract
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.
Journal
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- Living Reviews in Relativity
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Living Reviews in Relativity 24 (1), 6-, 2021-12
Springer Nature
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Keywords
Details 詳細情報について
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- CRID
- 1050856893077653760
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- ISSN
- 14338351
- 23673613
- http://id.crossref.org/issn/14338351
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- HANDLE
- 2433/276920
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- Web Site
- https://link.springer.com/content/pdf/10.12942/lrr-2011-6.pdf
- https://link.springer.com/article/10.12942/lrr-2011-6/fulltext.html
- http://link.springer.com/content/pdf/10.12942/lrr-2011-6
- https://link.springer.com/content/pdf/10.1007/s41114-021-00033-4.pdf
- https://link.springer.com/article/10.1007/s41114-021-00033-4/fulltext.html
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- Text Lang
- en
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- Article Type
- journal article
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- Data Source
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- IRDB
- Crossref
- KAKEN