scholarly journals Prospects for Gravitational-Wave Observations of Neutron-Star Tidal Disruption in Neutron-Star–Black-Hole Binaries

2000 ◽  
Vol 84 (16) ◽  
pp. 3519-3522 ◽  
Author(s):  
Michele Vallisneri
Keyword(s):  
Black Hole ◽  
Neutron Star ◽  
Gravitational Wave ◽  
Tidal Disruption ◽  
Black Hole Binaries

scholarly journals Coalescence of black hole–neutron star binaries

2021 ◽  
Vol 24 (1) ◽  
Author(s):  
Koutarou Kyutoku ◽  
Masaru Shibata ◽  
Keisuke Taniguchi
Keyword(s):  
Black Hole ◽  
Neutron Star ◽  
Gravitational Wave ◽  
High Precision ◽  
Numerical Relativity ◽  
Current Status ◽  
Wave Spectra ◽  
Tidal Disruption ◽  
Merger Process ◽  
General Relativistic

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.

Gravitational waves from neutron star binaries

2017 ◽  
Vol 26 (01n02) ◽  
pp. 1740015 ◽  
Author(s):  
Chang-Hwan Lee
Keyword(s):  
Black Hole ◽  
Neutron Star ◽  
Neutron Stars ◽  
Gravitational Wave ◽  
Gravitational Waves ◽  
Future Prospect ◽  
Black Hole Binaries ◽  
Wave Detection ◽  
Low Mass ◽  
Merger Rate

With H. A. Bethe, G. E. Brown worked on the merger rate of neutron star binaries for the gravitational wave detection. Their prediction has to be modified significantly due to the observations of [Formula: see text] neutron stars and the detection of gravitational waves. There still, however, remains a possibility that neutron star-low mass black hole binaries are significant sources of gravitational waves for the ground-based detectors. In this paper, I review the evolution of neutron star binaries with super-Eddington accretion and discuss the future prospect.

scholarly journals Neutron-Star–Black-Hole Binaries Produced by Binary-Driven Hypernovae

2015 ◽  
Vol 115 (23) ◽  
Author(s):  
Chris L. Fryer ◽  
F. G. Oliveira ◽  
J. A. Rueda ◽  
R. Ruffini
Keyword(s):  
Black Hole ◽  
Neutron Star ◽  
Black Hole Binaries
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