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SUMMARY:Supernova Registration in Water Cherenkov Veto of DarkSide-20k Dar
 k Matter Detector
DTSTART;VALUE=DATE-TIME:20161012T123000Z
DTEND;VALUE=DATE-TIME:20161012T130000Z
DTSTAMP;VALUE=DATE-TIME:20260712T092929Z
UID:indico-contribution-632@cern.ch
DESCRIPTION:Speakers: Dmitry Pugachev (NRC KI)\, Igor Machulin (NRC "Kurch
 atov Institute")\nRegistration of supernova neutrinos is one of the main g
 oals of large underground neutrino\ndetectors. We consider the possibility
  of using the large 2 kT water veto tank of DarkSide-20k dark matter detec
 tor as the additional facility for future Supernova detection. Simulations
  were performed for registration of cherenkov light in water tank from hig
 h energy positrons created by supernova electron antineutrinos via inverse
  beta decay reaction. The expected number of events and their energies for
  standard galactic Supernova is compatible with the information extracted 
 from the neutrinos from Supernova 1987a. Comparison between characteristic
 s of different supernova neutrino detectors are presented.\n\nhttps://indi
 co.particle.mephi.ru/event/4/contributions/632/
LOCATION:Milan Hotel Hall of the 2nd floor
URL:https://indico.particle.mephi.ru/event/4/contributions/632/
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