With the first observation of a binary neutron star merger through gravitational waves and
light, GW170817, compact binary mergers have now taken the center stage in nuclear …

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 …

We present a systematic numerical relativity study of the mass ejection and the associated
electromagnetic transients and nucleosynthesis from binary neutron star (NS) mergers. We …

We present results of a systematic study of failing core-collapse supernovae and the
formation of stellar-mass black holes (BHs). Using our open-source general-relativistic 1.5 D …

Merging binaries consisting of two neutron stars (NSs) or an NS and a stellar-mass black
hole typically form a massive accretion torus around the remnant black hole or long-lived …

Binary neutron star mergers observations are a unique way to constrain fundamental
physics and astrophysics at the extreme. The interpretation of gravitational-wave events and …

We investigate the influence of magnetic fields on the evolution of binary neutron star (BNS)
merger remnants via three-dimensional (3D) dynamical-spacetime general-relativistic …

Rotating relativistic stars have been studied extensively in recent years, both theoretically
and observationally, because of the information they might yield about the equation of state …

Fast neutron-rich material ejected dynamically over≲ 10 ms during the merger of a binary
neutron star (BNS) can give rise to distinctive electromagnetic counterparts to the system's …

The recent multimessenger observation of the short gamma-ray burst (SGRB) GRB 170817A
together with the gravitational wave (GW) event GW170817 provides evidence for the long …