collaborators

6 papers

astro-ph.CO2026

Magneto-Thermal Instability in Galaxy Clusters -- III. The Limit of Adiabatic Stratification

Lorenzo Maria Perrone, Henrik Latter

In the hot and dilute intracluster medium of galaxy clusters, large-scale buoyancy instabilities can develop due to the transport of heat along magnetic field lines. In particular,…

astro-ph.GA2026

The PICO-Cluster Project: presenting the galaxy cluster sample and studying magnetic field growth, Faraday rotation and Braginskii heating

Thomas Berlok, Christoph Pfrommer, Ewald Puchwein +9

Galaxy clusters constitute a microcosm of the Universe and offer a unique laboratory for studying plasma astrophysics, encompassing processes such as cosmic-ray acceleration and no…

astro-ph.GA2026

Active galactic nucleus driven jet feedback in cosmologically forming cool-core galaxy clusters I: The effect of hierarchical assembly on intra-cluster medium properties

Rainer Weinberger, Lorenzo Maria Perrone, Christoph Pfrommer +7

The atmospheres of cool-core galaxy clusters are excellent probes of astrophysical plasmas. However, how the interplay between assembly and active galactic nucleus (AGN) feedback l…

astro-ph.GA2026

Characterizing turbulence in galaxy clusters: defining turbulent energies and assessing multi-scale versus fixed-scale filters

Lorenzo Maria Perrone, Thomas Berlok, Ewald Puchwein +1

Disentangling turbulence and bulk motions in the intracluster medium (ICM) of galaxy clusters is inherently ambiguous, as the plasma is continuously stirred by different processes…

astro-ph.CO2025

Does the magneto-thermal instability survive whistler-suppression of thermal conductivity in galaxy clusters?

Lorenzo Maria Perrone, Thomas Berlok, Christoph Pfrommer

The hot and dilute intracluster medium (ICM) plays a central role in many key processes that shape galaxy clusters.Nevertheless, the nature of plasma turbulence and particle transp…

astro-ph.CO2025

Thermal conductivity with bells and whistlers: suppression of the magnetothermal instability in galaxy clusters

Lorenzo Maria Perrone, Thomas Berlok, Christoph Pfrommer

In the hot intracluster medium (ICM) in galaxy clusters, plasma microinstabilities may play an important role in the transport of heat and momentum on the large scales. In this pap…