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 …

Neutron star mergers are the canonical multimessenger events: they have been observed
through photons for half a century, gravitational waves since 2017, and are likely to be …

Recent numerical simulations in general relativistic magnetohydrodynamics (GRMHD)
provide useful constraints for the interpretation of the GW170817 discovery. Combining the …

Model Comparison from LIGO–Virgo Data on GW170817’s Binary Components and
Consequences for the Merger Remnant — Andrews University Research Portal Skip to main …

Since the release of the 2015 Long Range Plan in Nuclear Physics, major events have
occurred that reshaped our understanding of quantum chromodynamics (QCD) and nuclear …

Using hydrodynamical simulations for a large set of high-density matter equations of state
(EOSs), we systematically determine the threshold mass M thres for prompt black-hole …

The electromagnetic (EM) signal of a binary neutron star (BNS) merger depends sensitively
on the total binary mass, M tot, relative to various threshold masses set by the neutron star …

GW170817 and GRB 170817A provided direct evidence that binary neutron star (NSNS)
mergers can produce short gamma-ray bursts (sGRBs). However, questions remain about …

We present the computational relativity (CoRe) collaboration's public database of
gravitational waveforms from binary neutron star mergers. The database currently contains …

This study addresses the collapse behavior of neutron star (NS) mergers expressed through
the binary threshold mass M thres for prompt black-hole (BH) formation, which we determine …