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

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 …

This book introduces the modern field of 3+ 1 numerical relativity. The book has been written
in a way as to be as self-contained as possible, and only assumes a basic knowledge of …

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 …

This article presents a comprehensive overview of numerical hydrodynamics and magneto-
hydrodynamics (MHD) in general relativity. Some significant additions have been …

Three-dimensional simulations for the merger of binary neutron stars are performed in the
framework of full general relativity. We pay particular attention to the black hole formation …

We present numerical results of three-dimensional simulations for the merger of binary
neutron stars in full general relativity. Hybrid equations of state are adopted to mimic realistic …

We present a new three-dimensional fully general-relativistic hydrodynamics code using
high-resolution shock-capturing techniques and a conformal traceless formulation of the …

We review the current status of general relativistic studies for the coalescence of black hole-
neutron star (BH-NS) binaries. First, procedures for a solution of BH-NS binaries in quasi …