Galaxy clusters grow by gas accretion, mostly from mergers of substructures, which release
powerful shock waves into cosmic plasmas and convert a fraction of kinetic energy into …

As one of the prime contributors to the interstellar medium energy budget, magnetic fields
naturally play a part in shaping the evolution of galaxies. Galactic magnetic fields can …

Using a series of cosmological simulations that includes one dark-matter-only (DM-only) run,
one gas cooling–star formation–supernova feedback (CSF) run and one that additionally …

Both simulations and observations have shown that turbulence is a pervasive phenomenon
in cosmic scenarios, yet it is particularly difficult to model numerically due to its intrinsically …

Context. New-generation cosmological simulations are providing huge amounts of data,
whose analysis becomes itself a pressing computational problem. In particular, the …

Cosmological shock waves are ubiquitous to cosmic structure formation and evolution. As a
consequence, they play a major role in the energy distribution and thermalization of the …

About half of the expected total baryon budget in the local Universe is 'missing'.
Hydrodynamical simulations suggest that most of the missing baryons are located in a mildly …

We present semi-analytical models for magnetisation of the void inter-galactic medium (IGM)
by outflows from void galaxies. The number density of dark matter haloes in an under-dense …