An overview of grid-based numerical methods used in relativistic hydrodynamics (RHD) and
magnetohydrodynamics (RMHD) is presented. Special emphasis is put on a comprehensive …

The design and implementation of a new framework for adaptive mesh refinement
calculations are described. It is intended primarily for applications in astrophysical fluid …

We perform a general-relativistic neutrino-radiation magnetohydrodynamic simulation of a
one second-long binary neutron star merger on the Japanese supercomputer Fugaku using …

The merger of two neutron stars launches a relativistic jet, which must be driven by a strong
large-scale magnetic field. However, the magnetohydrodynamical mechanism required to …

Particle acceleration in collisionless plasma systems is a central question in astroplasma
and astroparticle physics. The structure of the acceleration regions, electron–ion energy …

We present a description of the adaptive mesh refinement (AMR) implementation of the
PLUTO code for solving the equations of classical and special relativistic …

Relativistic hydro and magnetohydrodynamics provide continuum fluid descriptions for gas
and plasma dynamics throughout the visible universe. We present an overview of state-of …

We have performed magnetohydrodynamic (MHD) simulations of relativistic jets from
supermassive blackholes over a few tens of kpc for a range of jet parameters. One of the …

The interaction of gamma-ray burst (GRB) jets with the dense media into which they are
launched promote the growth of local hydrodynamic instabilities along the jet boundary. In a …

We present THC: a new high-order flux-vector-splitting code for Newtonian and special-
relativistic hydrodynamics designed for direct numerical simulations of turbulent flows. Our …