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 …

Stellar-mass black holes and neutron stars represent extremes in gravity, density, and
magnetic fields. They therefore serve as key objects in the study of multiple frontiers of …

Mergers of black hole–neutron star (BHNS) binaries have now been observed by
gravitational wave (GW) detectors with the recent announcement of GW200105 and …

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

Mergers of binary neutron stars usually result in the formation of a hypermassive neutron
star (HMNS). Whether and when this remnant collapses to a black hole (BH) depends …

We study the radioactively powered transients produced by accretion disc winds following a
compact object merger. Based on the outflows found in two-dimensional hydrodynamical …

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 …

SciNet, one of seven regional HPC consortia operating under the Compute Canada
umbrella, runs Canada's first and third fastest computers (as of June 2010) in a state-of-the …

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 …

Expulsion of neutron-rich matter following the merger of neutron star binaries is crucial to the
radioactively powered electromagnetic counterparts of these events and to their relevance …