The universe is magnetized on all scales probed so far. On the largest scales, galaxies and
galaxy clusters host magnetic fields at the micro Gauss level coherent on scales up to ten …

Radio observations prove the existence of relativistic particles and magnetic field associated
with the intra-cluster-medium (ICM) through the presence of extended synchrotron emission …

We use the high-resolution TNG50 cosmological magnetohydrodynamical simulation to
explore the properties and origin of cold circumgalactic medium (CGM) gas around massive …

Magnetic reconnection, topological changes in magnetic fields, is a fundamental process in
magnetized plasmas. It is associated with energy release in regions of magnetic field …

Abstract The hot (107 to 108 kelvin), X-ray-emitting intracluster medium (ICM) is the
dominant baryonic constituent of clusters of galaxies. In the cores of many clusters, radiative …

This paper presents a theoretical framework for understanding plasma turbulence in
astrophysical plasmas. It is motivated by observations of electromagnetic and density …

Context. The existence of magnetic fields in the circumgalactic medium (CGM) is largely
unconstrained. Their detection is important as magnetic fields can have a significant impact …

We review the present theoretical and numerical understanding of magnetic field
amplification in cosmic large-scale structure, on length scales of galaxy clusters and beyond …

We present analysis of bulk and random gas motions in the intracluster medium using high-
resolution Eulerian cosmological simulations of 16 simulated clusters, including both very …

Magnetized turbulence and magnetic reconnection are often invoked to explain the
nonthermal emission observed from a wide variety of astrophysical sources. By means of …