Energy equipartition is a powerful theoretical tool for understanding astrophysical plasmas. It
is invoked, for example, to measure magnetic fields in the interstellar medium (ISM), as …

Primordial magnetic fields (PMFs) are possible candidates for explaining the observed
magnetic fields in galaxy clusters. Two competing scenarios of primordial magnetogenesis …

Small-scale fluctuating magnetic fields of order n G are observed in supernova shocks and
galaxy clusters, where its amplification is likely caused by the Biermann battery mechanism …

We introduce A strophysical H ybrid-K inetic simulations with the flash code ()–a new Hybrid
particle-in-cell (PIC) code developed within the framework of the multiphysics code flash …

Several different methods are regularly used to infer the properties of the neutral interstellar
medium (ISM) using atomic hydrogen (H i) 21cm absorption and emission spectra. In this …

Recent numerical studies suggest that magnetic fields play an important role in primordial
star formation in the early Universe. However, the detailed evolution of the magnetic field in …

Small-scale dynamos play important roles in modern astrophysics, especially on galactic
and extragalactic scales. Owing to dynamo action, purely hydrodynamic Kolmogorov …

Supernova explosions, active galactic nuclei jets, galaxy–galaxy interactions, and cluster
mergers can drive turbulence in the circumgalactic medium (CGM) and the intracluster …

The turbulent small-scale dynamo (SSD) is likely to be responsible for the magnetization of
the interstellar medium (ISM) that we observe in the Universe today. The SSD efficiently …

Magnetic fields are an energetically important component of star formation galaxies, but it is
often difficult to measure their properties from observations. One of the complexities stems …