Search for Supernova Neutrino Bursts at Super-Kamiokande

Understand

The result of a search for neutrino bursts from supernova explosions using the Super-Kamiokande detector is reported.

• Super-Kamiokande is sensitive to core-collapse supernova explosions via observation of their neutrino emissions.
• The expected number of events comprising such a burst is ~10^4 and the average energy of the neutrinos is in few tens of MeV range in the case of a core-collapse supernova explosion at the typical distance in our galaxy (10 kiloparsecs); this large signal means that the detection efficiency anywhere within our galaxy and well past the Magellanic Clouds is 100%.
• We examined a data set which was taken from May, 1996 to July, 2001 and from December, 2002 to October, 2005 corresponding to 2589.2 live days.