Study of Diffuse Supernova Neutrino Background with Modern and Future Detectors

Basic properties of the diffuse supernova neutrino background (DSNB) are reviewed. Current DSNB studies and the limits already set on the DSNB flow by the operating detectors Super-Kamiokande, SNO, and KamLAND are discussed. Prospects of DSNB studies with future high-mass neutrino detectors, such as JUNO and Hyper-Kamiokande, are considered.