We review the progress in modeling the galaxy population in hydrodynamical simulations of
the ΛCDM cosmogony. State-of-the-art simulations now broadly reproduce the observed …

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

Numerical simulations have become one of the key tools used by theorists in all the fields of
astrophysics and cosmology. The development of modern tools that target the largest …

Subsonic turbulence plays a major role in determining properties of the intracluster medium
(ICM). We introduce a new meshless finite mass (MFM) implementation in OpenGadget3 …

Context. To understand the structures of complex astrophysical objects, 3D numerical
simulations of radiative transfer processes are invaluable. For Monte Carlo radiative transfer …

We address the issue of numerical convergence in cosmological smoothed particle
hydrodynamics simulations using a suite of runs drawn from the eagle project. Our …

We extend the state-of-the-art N-body code pkdgrav3 with the inclusion of mesh-free gas
hydrodynamics for cosmological simulations. Two new hydrodynamic solvers have been …

We implement general relativistic hydrodynamics in the moving-mesh code arepo. We also
couple a solver for the Einstein field equations employing the conformal flatness …

With the observation that the TENO weighting strategy can explicitly distinguish smooth
scales from nonsmooth scales in spectral space, in this paper, a new discontinuity indicator …