Gravitational-wave detectors have transformed the way we observe the Universe. Together
with ground and space electromagnetic observatories, they have provided key insights into …

Numerical simulations of neutron star–neutron star and neutron star–black hole binaries
play an important role in our ability to model gravitational-wave and electromagnetic signals …

Neutrino flavor instabilities have the potential to shuffle neutrinos between electron, mu, and
tau flavor states, possibly modifying the core-collapse supernova mechanism and the heavy …

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 …

We present the second data release of gravitational waveforms from binary neutron star
(BNS) merger simulations performed by the Computational Relativity (CoRe) collaboration …

ABSTRACT GW190425 was the second gravitational wave (GW) signal compatible with a
binary neutron star (BNS) merger detected by the Advanced LIGO and Advanced Virgo …

The multi-messenger detection of the gravitational-wave signal GW170817, the
corresponding kilonova AT2017gfo and the short gamma-ray burst GRB170817A, as well as …

We investigate the properties of postmerger remnants of binary neutron star mergers in the
framework of Damour–Esposito-Farese-type scalar-tensor theory of gravity with a massive …

We examine the long-term evolution of accretion tori around black hole (BH) remnants of
compact object mergers involving at least one neutron star, to better understand their …

Recent gravitational wave observations of neutron-star-neutron-star and neutron-star-black-
hole binaries appear to indicate that massive neutron stars may not be too uncommon in …