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Cited by 440

The DOI matches its Crossref record; 144 of the 144 references it cites were found in a registry or an index.

Coalescence of Black Hole-Neutron Star Binaries

Open access
Shibata, Masaru, Taniguchi, Keisuke·2011·Living Reviews in Relativity

Abstract

We review the current status of general relativistic studies for the coalescence of black hole-neutron star (BH-NS) binaries. First, procedures for a solution of BH-NS binaries in quasi-equilibrium circular orbits and the numerical results, such as quasi-equilibrium sequence and mass-shedding limit, of the high-precision computation, are summarized. Then, the current status of numerical-relativity simulations for the merger of BH-NS binaries is described. We summarize our understanding for the merger and/or tidal disruption processes, the criterion for tidal disruption, the properties of the remnant formed after the tidal disruption, gravitational waveform, and gravitational-wave spectrum.

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Metadata

Authors
Shibata, M., & Taniguchi, K.
Venue
Living Reviews in Relativity
Published
2011-08-29
Volume
14
Issue
1
Pages
6-6
ISSN
  • 1433-8351 (ISSN-L)
  • 2367-3613
OpenAlex
W2084772304
Cited by
440
References
144
FWCI
16.77
Type
journal article
Language
en
Open access
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CoChat. (2026). Citation check: Coalescence of Black Hole-Neutron Star Binaries. https://app.cochat.ai/papers/10.12942/lrr-2011-6
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Shibata, M., & Taniguchi, K. (2011). Coalescence of Black Hole-Neutron Star Binaries. Living Reviews in Relativity. https://doi.org/10.12942/lrr-2011-6

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Contains information from the Semantic Scholar Academic Graph Datasets, made available under the ODC Attribution License (ODC-BY 1.0).

Semantic Scholar’s data is described in: Kinney, R., et al. (2023). The Semantic Scholar Open Data Platform. arXiv:2301.10140.