Over recent decades, cosmological simulations of galaxy formation have been instrumental
in advancing our understanding of structure and galaxy formation in the Universe. These …

We present two new Lagrangian methods for hydrodynamics, in a systematic comparison
with moving-mesh, smoothed particle hydrodynamics (SPH), and stationary (non-moving) …

Hydrodynamic cosmological simulations at present usually employ either the Lagrangian
smoothed particle hydrodynamics (SPH) technique or Eulerian hydrodynamics on a …

We introduce the public version of the cosmological magnetohydrodynamical moving-mesh
simulation code A repo. This version contains a finite-volume magnetohydrodynamics …

We present a new numerical code, PLUTO, for the solution of hypersonic flows in 1, 2, and 3
spatial dimensions and different systems of coordinates. The code provides a multiphysics …

We present the simulation framework CRPropa version 3 designed for efficient development
of astrophysical predictions for ultra-high energy particles. Users can assemble modules of …

The formation of protostars and their disks has been understood as the result of the
gravitational collapse phase of an accumulation of dense gas that determines the mass …

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

The presence of a dark matter core in the central kiloparsec of many dwarf galaxies has
been a long-standing problem in galaxy formation theories based on the standard cold dark …

A new code for astrophysical magnetohydrodynamics (MHD) is described. The code has
been designed to be easily extensible for use with static and adaptive mesh refinement. It …