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

Names: CTA Consortium (Organization) Title: Science with the Cherenkov Telescope
Array/by The CTA Consortium. Description: New Jersey: World Scientific, 2018.| Includes …

Diffuse cluster radio sources, in the form of radio halos and relics, reveal the presence of
cosmic rays and magnetic fields in the intracluster medium (ICM). These cosmic rays are …

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 …

Context. Radio relics in galaxy clusters are giant diffuse synchrotron sources powered in
cluster outskirts by merger shocks. Although the relic–shock connection has been …

This book summarizes the science to be carried out by the upcoming Cherenkov Telescope
Array, a major ground-based gamma-ray observatory that will be constructed over the next …

Non-thermal emission from relativistic cosmic ray (CR) electrons gives insight into the
strength and morphology of intra-cluster magnetic fields, as well as providing powerful …

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 …

We investigate the evolution of magnetic fields in galaxy clusters starting from constant
primordial fields using highly resolved () cosmological (magnetohydrodynamic) MHD …