output
19922025
most citedEscaping free-energy minima

5.7k citations

researchers with a paper here

Counting papers with at most 25 authors, so collaboration author lists do not stand in for the people here.

collaborating institutions
Showing astro-ph.COShow all

11 papers · 1 filter

astro-ph.CO2022★ 159 cited

The MillenniumTNG Project: The hydrodynamical full physics simulation and a first look at its galaxy clusters

Ruediger Pakmor, Volker Springel, Jonathan P. Coles +12

Cosmological simulations are an important theoretical pillar for understanding nonlinear structure formation in our Universe and for relating it to observations on large scales. In…

astro-ph.CO2018★ 37 cited

Probing the origin of extragalactic magnetic fields with Fast Radio Bursts

F. Vazza, M. Brüggen, P. M. Hinz +3

The joint analysis of the Dispersion and Faraday Rotation Measure from distant, polarised Fast Radio Bursts may be used to put constraints on the origin and distribution of extraga…

astro-ph.CO2018★ 51 cited

Observations of a nearby filament of galaxy clusters with the Sardinia Radio Telescope

V. Vacca, M. Murgia, F. Govoni +29

We report the detection of diffuse radio emission which might be connected to a large-scale filament of the cosmic web covering a 8deg x 8deg area in the sky, likely associated wit…

astro-ph.CO2016★ 124 cited

Turbulence and Vorticity in Galaxy Clusters Generated by Structure Formation

F. Vazza, T. W. Jones, M. Brüggen +4

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 result…

astro-ph.CO2016★ 5 cited

Detecting the cosmic web with radio surveys

F. Vazza, M. Brueggen, C. Gheller +2

We study the challenges to detect the cosmic web at radio wavelengths with state-of-the-art cosmological simulations of extragalactic magnetic fields. The incoming generation of ra…

astro-ph.CO2015★ 43 cited

Properties of Cosmological Filaments extracted from Eulerian Simulations

Claudio Gheller, Franco Vazza, Jean Favre +1

Using a new parallel algorithm implemented within the VisIt framework, we analysed large cosmological grid simulations to study the properties of baryons in filaments. The procedur…

astro-ph.CO2015★ 71 cited

Forecasts for the detection of the magnetised cosmic web from cosmological simulations

F. Vazza, C. Ferrari, M. Brüggen +3

The cosmic web contains a large fraction of the total gas mass in the universe but is difficult to detect at most wavelengths. Synchrotron emission from shock-accelerated electrons…

astro-ph.CO2015

Filaments of the radio cosmic web: opportunities and challenges for SKA

Franco Vazza, Chiara Ferrari, Annalisa Bonafede +4

The detection of the diffuse gas component of the cosmic web remains a formidable challenge. In this work we study synchrotron emission from the cosmic web with simulated SKA1 obse…

astro-ph.CO2014★ 25 cited

Simulations of cosmic rays in large-scale structures: numerical and physical effects

Franco Vazza, Claudio Gheller, Marcus Brüggen

Non-thermal (relativistic) particles are injected into the cosmos by structure formation shock waves, active galactic nuclei and stellar explosions. We present a suite of unigrid c…

astro-ph.CO2012★ 43 cited

Thermal and non-thermal traces of AGN feedback: results from cosmological AMR simulations

F. Vazza, M. Brueggen, C. Gheller

We investigate the observable effects of feedback from Active Galactic Nuclei (AGN) on non-thermal components of the intracluster medium (ICM). We have modelled feedback from AGN i…

astro-ph.CO2012★ 55 cited

Modelling injection and feedback of Cosmic Rays in grid-based cosmological simulations: effects on cluster outskirts

F. Vazza, M. Bruggen, C. Gheller +1

We present a numerical scheme, implemented in the cosmological adaptive mesh refinement code ENZO, to model the injection of Cosmic Ray (CR) particles at shocks, their advection an…