activity
20112026
most citedInfluence of adaptive mesh refinement and the hydro solver on shear-induced mass stripping in a minor-merger scenario

8 citations · 9 across the 5 of their papers we have counts for

collaborators

6 papers

astro-ph.CO2026

Cosmological simulation of a radio synchrotron bridge between pre-merging galaxy clusters

Kosuke Nishiwaki, Gianfranco Brunetti, Franco Vazza +1

Radio bridges are diffuse synchrotron emission observed between merging galaxy clusters. Recent radio observations have reported both detections and non-detections of radio bridges…

astro-ph.GA2026

Cold gas formation triggered by active galactic nuclei jet feedback in galaxy cluster cores

Stefano Sotira, Martin A. Bourne, Debora Sijacki +2

Extended warm and cold gas nebulae, with complex morphologies and kinematics, have been observed in the centres of cool-core galaxy clusters. Their origin within the hot intraclust…

physics.pop-ph2025★ 1 cited

Astrophysical constraints on the simulation hypothesis for this Universe: why it is (nearly) impossible that we live in a simulation

F. Vazza

We assess how physically realistic the ''simulation hypothesis'' for this Universe is, based on physical constraints arising from the link between information and energy, and on kn…

astro-ph.CO2016

The quest for extragalactic magnetic fields

Franco Vazza

We review the observational and theoretical constraints on extragalactic magnetic fields across cosmic environment. In the next decade, the combination of sophisticated numerical s…

astro-ph.CO2014★ 8 cited

Influence of adaptive mesh refinement and the hydro solver on shear-induced mass stripping in a minor-merger scenario

W. Schmidt, J. Schulz, L. Iapichino +2

We compare two different codes for simulations of cosmological structure formation to investigate the sensitivity of hydrodynamical instabilities to numerics, in particular, the hy…

astro-ph.CO2011

Merger and non-merger galaxy clusters in cosmological AMR simulations

Franco Vazza

Aims: We discuss the dependence of shocks, cosmic rays acceleration and turbulence on the dynamical state of the host clusters. Method: We perform cosmological simulations with the…