Objective On large scales cosmic matter is distributed in a web consistent of clusters, filaments, walls and voids. While the dark-matter skeleton of the cosmic web is closely traced by galaxies and galaxy clusters, the gaseous distribution has never been directly imaged at any wavelength. This situation might change within the next decade, thanks to the new generation of radio instruments that will survey the sky: LOFAR, MWA, ASKAP and the Square Kilometer Array. Non-thermal components, relativistic particles and magnetic fields are thought to have a spatial distribution that is broader than that of thermal baryons. For this reason, the new generation of radio telescopes should might be able to detect the tip of the iceberg from the rarefied intergalactic medium, provided that magnetic fields are sufficiently amplified in these regions. The detectable signal is expected to be weak and complex because of the contribution from radio galaxies and to the presence of diffuse fore- and backgrounds. The developments proposed in this ERC proposal are exactly designed to address this complexity, and turn future radio observations into a unique probe of the growth of magnetic fields and of the acceleration of particles. This will be possible through the theoretical exploration of plasmas in extreme conditions with sophisticated numerical simulations. With these simulations I will be able to predict the specific radio signature for the origin of extragalactic fields. This will enable the community to use radio surveys in a quantitative way and to determine the origin of extragalactic magnetism, a longstanding puzzle connected to many open questions of modern astrophysics. The legacy of this project will be its quantitative representation of non-thermal processes on the largest scales, ultimately going to be fully exploited by the Square Kilometer Array. Fields of science natural sciencesphysical sciencesastronomyextragalactic astronomynatural sciencesphysical sciencesastronomyobservational astronomyradio astronomynatural sciencesphysical sciencesastronomyastrophysics Programme(s) H2020-EU.1.1. - EXCELLENT SCIENCE - European Research Council (ERC) Main Programme Topic(s) ERC-2016-STG - ERC Starting Grant Call for proposal ERC-2016-STG See other projects for this call Funding Scheme ERC-STG - Starting Grant Coordinator ALMA MATER STUDIORUM - UNIVERSITA DI BOLOGNA Net EU contribution € 1 265 943,00 Address Via zamboni 33 40126 Bologna Italy See on map Region Nord-Est Emilia-Romagna Bologna Activity type Higher or Secondary Education Establishments Links Contact the organisation Opens in new window Website Opens in new window Participation in EU R&I programmes Opens in new window HORIZON collaboration network Opens in new window Other funding € 0,00 Beneficiaries (2) Sort alphabetically Sort by Net EU contribution Expand all Collapse all ALMA MATER STUDIORUM - UNIVERSITA DI BOLOGNA Italy Net EU contribution € 1 265 943,00 Address Via zamboni 33 40126 Bologna See on map Region Nord-Est Emilia-Romagna Bologna Activity type Higher or Secondary Education Establishments Links Contact the organisation Opens in new window Website Opens in new window Participation in EU R&I programmes Opens in new window HORIZON collaboration network Opens in new window Other funding € 0,00 UNIVERSITAET HAMBURG Germany Net EU contribution € 200 000,00 Address Mittelweg 177 20148 Hamburg See on map Region Hamburg Hamburg Hamburg Activity type Higher or Secondary Education Establishments Links Contact the organisation Opens in new window Website Opens in new window Participation in EU R&I programmes Opens in new window HORIZON collaboration network Opens in new window Other funding € 0,00
