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

In this paper, we present an update to the open source MPI-AMRVAC simulation toolkit
where we focus on solar and non-relativistic astrophysical magnetofluid dynamics. We …

We investigate the impact of using high-order numerical methods to study the merger of
magnetized neutron stars with finite-temperature microphysics and neutrino cooling in full …

The theoretical modeling of gravitational waveforms from binary neutron star mergers
requires precise numerical relativity simulations. Assessing convergence of the numerical …

The objective of this paper is to explore the application of a six-component overset grid to
solar wind simulation with a three-dimensional (3D) Solar-InterPlanetary Conservation …

We present the new general-relativistic magnetohydrodynamics (GRMHD) capabilities of the
Einstein toolkit, an open-source community-driven numerical relativity and computational …

Context. The remnants of core-collapse supernovae (SNe) are probes of the physical
processes associated with their parent SNe. Aims. Here we aim to explore to which extent …

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 …

High-order reconstruction schemes for the solution of hyperbolic conservation laws in
orthogonal curvilinear coordinates are revised in the finite volume approach. The …

The amplification of primordial magnetic fields via a small-scale turbulent dynamo during
structure formation might be able to explain the observed magnetic fields in galaxy clusters …