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SUMMARY:Sub-GeV atmospheric neutrinos background in organic liquid scintil
 lator mediums
DTSTART;VALUE=DATE-TIME:20161013T104500Z
DTEND;VALUE=DATE-TIME:20161013T110000Z
DTSTAMP;VALUE=DATE-TIME:20260720T215135Z
UID:indico-contribution-723@cern.ch
DESCRIPTION:Speakers: Viktor Atroshchenko (NRC Kurchatov Institute)\nAtmos
 pheric neutrinos are produced in interactions of cosmic rays with atomic n
 uclei in the Earth’s atmosphere. In low energy neutrino experiments they
  mainly considered as a background for studied processes. For atmospheric 
 neutrinos in energy range below 1 GeV we present semi-analytical expected 
 yield for four neutrino detection reactions: νp-ES\, νe-ES\, inverse β-
 decay and 12C(ν\, ν′)12C*(15.1 MeV)\, as well as results of Monte-Carl
 o simulation for other ν12C interaction channels. Calculations are made f
 or several neutrino experiments and include neutrino oscillation averaged 
 over neutrino arrival directions.\n\nhttps://indico.particle.mephi.ru/even
 t/4/contributions/723/
LOCATION:Milan Hotel Verdi
URL:https://indico.particle.mephi.ru/event/4/contributions/723/
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