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 …

Observations show that at least some gamma-ray bursts (GRBs) happen simultaneously
with core-collapse supernovae (SNe), thus linking by a common thread nature's two …

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

We present the first generalization of Navier-Stokes theory to relativity that satisfies all of the
following properties:(a) the system coupled to Einstein's equations is causal and strongly …

A new approach is described to help improve the foundations of relativistic viscous fluid
dynamics and its coupling to general relativity. Focusing on neutral conformal fluids …

We present results for the elliptic and triangular flow coefficients v 2 and v 3 in Au+ Au
collisions at s= 200 A GeV using event-by-event D= 3+ 1 viscous hydrodynamic simulations …

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 …

Massive (hypermassive and supramassive) neutron stars are likely to be often formed after
the merger of binary neutron stars. We explore the evolution process of the remnant massive …

Inferring the properties of dense matter is one of the most exciting prospects from the
measurement of gravitational waves from neutron star mergers. However, it requires reliable …

We study the lifetimes of the remnant produced by the merger of two neutron stars and revisit
the determination of the threshold mass to prompt collapse, M th. Using a fully general …