Coalescence of black hole–neutron star binaries-Reference-Cited by-同舟云学术

Coalescence of black hole–neutron star binaries

Published:2021-12 Issue:1 Volume:24 Page:
ISSN:2367-3613
Container-title:Living Reviews in Relativity
language:en
Short-container-title:Living Rev Relativ

Author:

Kyutoku Koutarou,Shibata Masaru,Taniguchi Keisuke

Abstract

AbstractWe 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.

Publisher

Springer Science and Business Media LLC

Subject

Physics and Astronomy (miscellaneous)

Link

https://link.springer.com/content/pdf/10.1007/s41114-021-00033-4.pdf

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