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

This review covers the main aspects of black hole accretion disk theory. We begin with the
view that one of the main goals of the theory is to better understand the nature of black holes …

Abstract We describe the Einstein Toolkit, a community-driven, freely accessible
computational infrastructure intended for use in numerical relativity, relativistic astrophysics …

Fully general relativistic models of astrophysical sources are in high demand, not only since
the discovery of gravitational waves emitted from merging stellar mass black holes (Abbott et …

Using numerical relativity simulations with a subgrid dynamo prescription to generate strong
initial magnetic fields, we investigate the possibility of launching a jet-like outflow from the …

This monograph originates from lectures given at the General Relativity Trimester at the
Institut Henri Poincaré in Paris [1]; at the VII Mexican School on Gravitation and …

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

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 studies of the coalescence of binary neutron star systems.
We begin with a discussion of the formation channels of merging binaries and we discuss …

We present numerical simulations of axisymmetric, magnetically driven relativistic jets. Our
special-relativistic, ideal-magnetohydrodynamics numerical scheme is specifically designed …