At present, we have almost as many theories to explain Fast Radio Bursts as we have Fast
Radio Bursts observed. This landscape will be changing rapidly with CHIME/FRB, recently …

In a single process, the merger of binary neutron star systems combines extreme gravity, the
copious emission of gravitational waves, complex microphysics and electromagnetic …

Abstract The Event Horizon Telescope (EHT) has mapped the central compact radio source
of the elliptical galaxy M87 at 1.3 mm with unprecedented angular resolution. Here we …

The detection of five new fast radio bursts (FRBs) found in the 1.4-GHz High Time
Resolution Universe high-latitude survey at Parkes, is presented. The rate implied is 7 (95 …

Context. Several fast radio bursts have been discovered recently, showing a bright, highly
dispersed millisecond radio pulse. The pulses do not repeat and are not associated with a …

We present the black hole accretion code (BHAC), a new multidimensional general-
relativistic magnetohydrodynamics module for the MPI-AMRVAC framework. BHAC has …

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 …

We review the current status of general relativistic studies for coalescences of black hole–
neutron star binaries. First, high-precision computations of black hole–neutron star binaries …

We present an improved version of the ECHO-QGP numerical code, which self-consistently
includes for the first time the effects of electromagnetic fields within the framework of …