▪ Abstract Cosmic structure has formed as a result of gravitational amplification of primordial
density fluctuations together with the action of other physical processes (adiabatic gas …

We demonstrate with a new three-dimensional adaptive mesh refinement code that
perturbations arising from discretization of the equations of self-gravitational hydrodynamics …

We present results of N-body/gasdynamical simulations designed to investigate the
evolution of X-ray clusters in a flat, low-density, Λ-dominated cold dark matter (CDM) …

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 …

We present the results of a set of high-resolution chemo-dynamical simulations of dwarf
galaxies in a ΛCDM cosmology. Out of an original cosmological box, a sample of 27 systems …

Numerical simulations of dwarf galaxies have so far failed to reproduce the observed
metallicity-luminosity relation, down to the regime of ultra-faint dwarfs (UFDs). We address …

In the framework of Tsallis statistics, we study the effect of medium nonextensivity on the
Jeans gravitational instability criterion for a self-gravitating protoplanetary cloud, the …

In this work, the dynamics of self-gravitating systems composed by dark and baryonic matter
is analyzed. Searching for a description of this dynamics, a system of collisionless …

The question we address in this paper is the determination of the correlation properties of
the dark matter halos appearing in cosmic density fields once they underwent a strongly …

The effects of sampling are investigated on measurements of counts-in-cells in three-
dimensional magnitude-limited galaxy surveys, with emphasis on moments of the underlying …