# Numerical simulations of neutron star-black hole binaries in the near-equal-mass regime

@article{Foucart2019NumericalSO,
title={Numerical simulations of neutron star-black hole binaries in the near-equal-mass regime},
author={F. Foucart and M. Duez and L. Kidder and S. Nissanke and H. Pfeiffer and M. Scheel},
journal={Physical Review D},
year={2019},
volume={99},
pages={103025}
}
• F. Foucart, +3 authors M. Scheel
• Published 2019
• Physics
• Physical Review D
• Simulations of neutron star-black hole (NSBH) binaries generally consider black holes with masses in the range $(5-10)M_\odot$, where we expect to find most stellar mass black holes. The existence of lower mass black holes, however, cannot be theoretically ruled out. Low-mass black holes in binary systems with a neutron star companion could mimic neutron star-neutron (NSNS) binaries, as they power similar gravitational wave (GW) and electromagnetic (EM) signals. To understand the differences… CONTINUE READING

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