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 …

This paper describes the open-source code Enzo, which uses block-structured adaptive
mesh refinement to provide high spatial and temporal resolution for modeling astrophysical …

Although galaxies, groups, and clusters contain∼ 10% of the baryons, many more reside in
the photoionized and shocked-heated intergalactic medium (IGM) and in the circumgalactic …

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 …

We discuss new methods to integrate the cosmic ray (CR) evolution equations coupled to
magnetohydrodynamics on an unstructured moving mesh, as realized in the massively …

The utility of large Sunyaev–Zel'dovich (SZ) surveys for determining cosmological
parameters from cluster abundances is limited by the theoretical uncertainties in the …

In large-scale cosmological hydrodynamic simulations simplified sub-grid models for gas
accretion on to black holes and AGN feedback are commonly used. Such models typically …

Current theories predict relativistic hadronic particle populations in clusters of galaxies in
addition to the already observed relativistic leptons. In these scenarios hadronic interactions …

We present a comparison between weak-lensing and x-ray mass estimates of a sample of
numerically simulated clusters. The sample consists of the 20 most massive objects at …

Turbulence is a key ingredient for the evolution of the intracluster medium, whose properties
can be predicted with high-resolution numerical simulations. We present initial results on the …