Coalescence of Black Hole-Neutron Star Binaries

Details Coalescence of Black Hole-Neutron Star Binaries Coalescence of Black Hole-Neutron Star Binaries

Aug 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011lrr....14....6s&link_type=abstract

Living Reviews in Relativity, vol. 14, no. 6

Statistics

Computation

5

Neutron Star, Gravitational Waves, Black Hole, Numerical Relativity

Scientific paper

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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