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Title: Signal for supernova {bold {nu}}{sub {bold {mu}}} and {bold {nu}}{sub {bold {tau}}} neutrinos in water {hacek C}erenkov detectors

Abstract

We suggest that photons with energies between 5 and 10 MeV, generated by the ({nu},{nu}{prime}{ital p}{gamma}) and ({nu},{nu}{prime}{ital n}{gamma}) reactions on {sup 16}O, constitute a signal which allows a unique identification of supernova {nu}{sub {mu}} and {nu}{sub {tau}} neutrinos in water {hacek C}erenkov detectors. We calculate the yield of such {gamma} events and estimate that a few hundred of them would be detected in Superkamiokande for a supernova at 10kpc distance. {copyright} {ital 1996 The American Physical Society.}

Authors:
; ;  [1]
  1. W. K. Kellogg Radiation Laboratory, 106-38, California Institute of Technology, Pasadena, California 91125 (United States)
Publication Date:
Research Org.:
California Institute of Technology (CalTech), Pasadena, CA (United States)
OSTI Identifier:
285406
DOE Contract Number:  
FG03-88ER40397
Resource Type:
Journal Article
Journal Name:
Physical Review Letters
Additional Journal Information:
Journal Volume: 76; Journal Issue: 15; Other Information: PBD: Apr 1996
Country of Publication:
United States
Language:
English
Subject:
66 PHYSICS; SUPERNOVAE; MUON NEUTRINOS; TAU NEUTRINOS; SIGNALS; CHERENKOV COUNTERS; PHOTONS; MEV RANGE 01-10; OXYGEN 16; NEUTRINO REACTIONS; LIQUID SCINTILLATION DETECTORS; WATER

Citation Formats

Langanke, K, Vogel, P, Kolbe, E, Physics Department, California Institute of Technology, Pasadena, California 91125, and Institut fuer Physik, Universitaet Basel, Basel. Signal for supernova {bold {nu}}{sub {bold {mu}}} and {bold {nu}}{sub {bold {tau}}} neutrinos in water {hacek C}erenkov detectors. United States: N. p., 1996. Web. doi:10.1103/PhysRevLett.76.2629.
Langanke, K, Vogel, P, Kolbe, E, Physics Department, California Institute of Technology, Pasadena, California 91125, & Institut fuer Physik, Universitaet Basel, Basel. Signal for supernova {bold {nu}}{sub {bold {mu}}} and {bold {nu}}{sub {bold {tau}}} neutrinos in water {hacek C}erenkov detectors. United States. https://doi.org/10.1103/PhysRevLett.76.2629
Langanke, K, Vogel, P, Kolbe, E, Physics Department, California Institute of Technology, Pasadena, California 91125, and Institut fuer Physik, Universitaet Basel, Basel. 1996. "Signal for supernova {bold {nu}}{sub {bold {mu}}} and {bold {nu}}{sub {bold {tau}}} neutrinos in water {hacek C}erenkov detectors". United States. https://doi.org/10.1103/PhysRevLett.76.2629.
@article{osti_285406,
title = {Signal for supernova {bold {nu}}{sub {bold {mu}}} and {bold {nu}}{sub {bold {tau}}} neutrinos in water {hacek C}erenkov detectors},
author = {Langanke, K and Vogel, P and Kolbe, E and Physics Department, California Institute of Technology, Pasadena, California 91125 and Institut fuer Physik, Universitaet Basel, Basel},
abstractNote = {We suggest that photons with energies between 5 and 10 MeV, generated by the ({nu},{nu}{prime}{ital p}{gamma}) and ({nu},{nu}{prime}{ital n}{gamma}) reactions on {sup 16}O, constitute a signal which allows a unique identification of supernova {nu}{sub {mu}} and {nu}{sub {tau}} neutrinos in water {hacek C}erenkov detectors. We calculate the yield of such {gamma} events and estimate that a few hundred of them would be detected in Superkamiokande for a supernova at 10kpc distance. {copyright} {ital 1996 The American Physical Society.}},
doi = {10.1103/PhysRevLett.76.2629},
url = {https://www.osti.gov/biblio/285406}, journal = {Physical Review Letters},
number = 15,
volume = 76,
place = {United States},
year = {Mon Apr 01 00:00:00 EST 1996},
month = {Mon Apr 01 00:00:00 EST 1996}
}