Abstract
The detection of the neutrino burst from supernova explosion by Kamiokande, IBM, and BAKSAN on the 23rd of February, 1987 opened the door to the new era of neutrino astrophysics. Nowadays, many neutrino detectors are running to detect neutrinos from supernova explosions. On the other hand, the diffuse flux of neutrinos from all past supernovae, supernova relic neutrinos (SRN), exists in space. Since large target mass and high background reduction are necessary, SRN has not been observed. For observation of SRN, GADZOOKS! project has been proposed and R&D project is ongoing.
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