Objectif 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. Champ scientifique sciences naturellessciences physiquesastronomieastronomie extragalactiquesciences naturellessciences physiquesastronomieastronomie d’observationradioastronomiesciences naturellessciences physiquesastronomieastrophysique Mots‑clés MAGCOW Programme(s) H2020-EU.1.1. - EXCELLENT SCIENCE - European Research Council (ERC) Main Programme Thème(s) ERC-2016-STG - ERC Starting Grant Appel à propositions ERC-2016-STG Voir d’autres projets de cet appel Régime de financement ERC-STG - Starting Grant Coordinateur ALMA MATER STUDIORUM - UNIVERSITA DI BOLOGNA Contribution nette de l'UE € 1 265 943,00 Adresse Via zamboni 33 40126 Bologna Italie Voir sur la carte Région Nord-Est Emilia-Romagna Bologna Type d’activité Higher or Secondary Education Establishments Liens Contacter l’organisation Opens in new window Site web Opens in new window Participation aux programmes de R&I de l'UE Opens in new window Réseau de collaboration HORIZON Opens in new window Autres sources de financement € 0,00 Bénéficiaires (2) Trier par ordre alphabétique Trier par contribution nette de l'UE Tout développer Tout réduire ALMA MATER STUDIORUM - UNIVERSITA DI BOLOGNA Italie Contribution nette de l'UE € 1 265 943,00 Adresse Via zamboni 33 40126 Bologna Voir sur la carte Région Nord-Est Emilia-Romagna Bologna Type d’activité Higher or Secondary Education Establishments Liens Contacter l’organisation Opens in new window Site web Opens in new window Participation aux programmes de R&I de l'UE Opens in new window Réseau de collaboration HORIZON Opens in new window Autres sources de financement € 0,00 UNIVERSITAET HAMBURG Allemagne Contribution nette de l'UE € 200 000,00 Adresse Mittelweg 177 20148 Hamburg Voir sur la carte Région Hamburg Hamburg Hamburg Type d’activité Higher or Secondary Education Establishments Liens Contacter l’organisation Opens in new window Site web Opens in new window Participation aux programmes de R&I de l'UE Opens in new window Réseau de collaboration HORIZON Opens in new window Autres sources de financement € 0,00
