collaborators

7 papers

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.HE2026

Identifying heating processes in simulations with an entropy-based scheme: A single jet episode in a galaxy cluster

Moun Meenakshi, Rainer Weinberger, Christoph Pfrommer +1

Understanding heating processes in galaxy clusters is essential for predicting the regulation of radiative cooling and star formation, and for clarifying the mechanisms underlying…

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.GA2025

Anisotropic Velocity Fluctuations in Galaxy Mergers: A Probe of the Magnetic Field

Yue Hu, Joseph Whittingham, A. Lazarian +3

Magnetic fields and turbulence are fundamental to the evolution of galaxies, yet their precise measurement and analysis present significant challenges. The recently developed Veloc…

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…