Two neutron stars merge somewhere in the Universe approximately every 10 to 100 s,
creating violent explosions potentially observable in gravitational waves and across the …

With the computational power and algorithmic improvements available today, the ongoing
STAR/RHIC and HADES/GSI experiments, the future FAIR and NICA facilities becoming …

We present a new moment-based energy-integrated neutrino transport code for neutron star
merger simulations in general relativity. In the merger context, ours is the first code to include …

We present a systematic numerical relativity study of the dynamical ejecta, winds, and
nucleosynthesis in neutron star (NS) merger remnants. Binaries with the chirp mass …

We present realistic expectations for the number and properties of neutron star binary
mergers to be detected as multi-messenger sources during the upcoming fourth observing …

For the first∼ 3 yrs after the binary neutron star merger event GW 170817, the radio and X-
ray radiation has been dominated by emission from a structured relativistic off-axis jet …

We investigate the quark deconfinement phase transition in the context of binary neutron
star (BNS) mergers. We treat hadronic matter using a Brueckner-Hartree-Fock quantum …

We present a systematic numerical relativity study of the impact of different physics input and
grid resolution in binary neutron star mergers. We compare simulations employing a …

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 …

The joint detection of the gravitational wave GW170817, of the short γ-ray burst
GRB170817A and of the kilonova AT2017gfo, generated by the the binary neutron star (NS) …