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We investigate the signal from supernova relic neutrinos in future largescale observatories, such as MEMPHYS (UNO, Hyper-K), LENA and GLACIER, atpresent under study. We discuss that complementary information might be gainedfrom the observation of supernova relic electron anti-neutrinos and neutrinosusing the scattering on protons on one hand, and on nuclei such as oxygen,carbon or argon on the other hand. When determining the relic neutrino fluxeswe also include, for the first time, the coupling of the neutrino magneticmoment to magnetic fields within the core-collapse supernova. We presentnumerical results on both the relic electron neutrino and anti-neutrino fluxesand on the number of events for electron neutrinos on carbon, oxygen and argon,as well as electron anti-neutrinos on protons, for various oscillationscenarios. The observation of supernova relic neutrinos might provide us withunique information on core-collapse supernova explosions, on the star formationhistory and on neutrino properties, that still remain unknown.

Supernova Relic Electron Neutrinos and anti-Neutrinos in future Large-scale Observatories