In a growing number of galaxy clusters diffuse extended radio sources have been found.
These sources are not directly associated with individual cluster galaxies. The radio …

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 introduce the IllustrisTNG project, a new suite of cosmological magnetohydrodynamical
simulations performed with the moving-mesh code arepo employing an updated Illustris …

The Square Kilometre Array (SKA) is a planned large radio interferometer designed to
operate over a wide range of frequencies, and with an order of magnitude greater sensitivity …

We present and study a large suite of high-resolution cosmological zoom-in simulations,
using the FIRE-2 treatment of mechanical and radiative feedback from massive stars …

The Cherenkov Telescope Array (CTA), the new-generation ground-based observatory for γ-
ray astronomy, provides unique capabilities to address significant open questions in …

The magnetic fields observed in the Milky Way and nearby galaxies appear to be in
equipartition with the turbulent, thermal and cosmic ray energy densities, and hence are …

We take advantage of the wealth of rotation measures data contained in the NRAO VLA Sky
Survey catalog to derive new, statistically robust, upper limits on the strength of extragalactic …

The origin of extragalactic magnetic fields is still poorly understood. Based on a dedicated
suite of cosmological magneto-hydrodynamical simulations with the ENZO code we have …

Faraday rotation and synchrotron emission from extragalactic radio sources give evidence
for the presence of magnetic fields extending over∼ Mpc scales. However, the origin of …