Coalescence of black hole–neutron star binaries

@article{Kyutoku2021CoalescenceOB,
  title={Coalescence of black hole–neutron star binaries},
  author={Koutarou Kyutoku and Masaru Shibata and Keisuke Taniguchi},
  journal={Living Reviews in Relativity},
  year={2021},
  volume={24},
  pages={1-182}
}
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… 

References

SHOWING 1-10 OF 290 REFERENCES
Simulations of Binary Coalescence of a Neutron Star and a Black Hole
We present the results of Newtonian hydrodynamic simulations of the coalescence of a binary consisting of a black hole with a neutron star. The calculations show that for a wide range of initial
Coalescence of Black Hole-Neutron Star Binaries
TLDR
The current status of general relativistic studies for the coalescence of black hole-neutron star (BH-NS) binaries is reviewed and understanding for the merger and/or tidal disruption processes, the criterion for tidal disruption, and the properties of the remnant formed after the tidal disruption are summarized.
Merger and Mass Ejection of Neutron Star Binaries
Mergers of binary neutron stars and black hole–neutron star binaries are among the most promising sources for ground-based gravitational-wave (GW) detectors and are also high-energy astrophysical
Accretion dynamics in neutron star black hole binaries
We perform three-dimensional, Newtonian hydrodynamic simulations with a nuclear equation of state to investigate the accretion dynamics in neutron star black hole systems. We find as a general result
A semi-relativistic model for tidal interactions in BH–NS coalescing binaries
We study the tidal effects of a Kerr black hole on a neutron star in black hole–neutron star (BH–NS) binary systems by using a semi-analytical approach which describes the neutron star as a
Initial data for black hole–neutron star binaries, with rotating stars
The coalescence of a neutron star with a black hole is a primary science target of ground-based gravitational wave detectors. Constraining or measuring the neutron star spin directly from
Massive disc formation in the tidal disruption of a neutron star by a nearly extremal black hole
Black hole–neutron star (BHNS) binaries are important sources of gravitational waves for second-generation interferometers, and BHNS mergers are also a proposed engine for short, hard gamma-ray
Black Hole-Neutron Star Mergers as Central Engines of Gamma-Ray Bursts.
TLDR
Hydrodynamic simulations of the merger of stellar mass black hole-neutron star binaries are compared with mergers of binary neutron stars and the use of a physical nuclear equation of state allows us to include the effects of neutrino emission.
Mergers of Neutron Star-Black Hole Binaries with Small Mass Ratios: Nucleosynthesis, Gamma-Ray Bursts, and Electromagnetic Transients
We discuss simulations of the coalescence of black hole-neutron star binary systems with black hole masses between 14 and 20 M☉. The calculations use a three-dimensional smoothed particle
Neutron Star and Black Hole Binaries in the Galaxy
We present a statistical analysis of the number and birthrate of double neutron star (NS-NS) binaries. We estimate that there are ∼10 4.5 z 0 such systems in the Galaxy, with a birthrate ∼10 −5 z 0
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