The coalescence of double neutron star (NS–NS) and black hole (BH)–NS binaries are
prime sources of gravitational waves (GW) for Advanced LIGO/Virgo and future ground …

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 …

We present the first comprehensive study of r-process element nucleosynthesis in the ejecta
of compact binary mergers (CBMs) and their relic black hole (BH)–torus systems. The …

Gravitational-wave (GW) and electromagnetic (EM) signals from the merger of a neutron star
(NS) and a black hole (BH) are a highly anticipated discovery. We present a simple formula …

Numerical-relativity simulations for the merger of binary neutron stars are performed for a
variety of equations of state (EOSs) and for a plausible range of the neutron-star mass …

The exterior gravitational field of a slowly rotating neutron star can be characterized by its
multipole moments, the first few being the neutron star mass, moment of inertia, and …

Abstract We describe the Einstein Toolkit, a community-driven, freely accessible
computational infrastructure intended for use in numerical relativity, relativistic astrophysics …

The final inspiral of double neutron star and neutron-star–black-hole binaries are likely to be
detected by advanced networks of ground-based gravitational wave (GW) interferometers …

Seconds-long numerical-relativity simulations for black hole–neutron star mergers are
performed for the first time to obtain a self-consistent picture of the merger and post-merger …