Detectability of supernova neutrinos with an existing proton decay detector

Details Detectability of supernova neutrinos with an existing proton decay detector Detectability of supernova neutrinos with an existing proton decay detector

Apr 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984sci...224...56l&link_type=abstract

Science (ISSN 0036-8075), vol. 224, April 6, 1984, p. 56-58. Research supported by the Research Corp.

Other

6

Extraterrestrial Radiation, Neutrinos, Radiation Detectors, Supernovae, Electromagnetic Noise, Gravitational Collapse, Photomultiplier Tubes

Scientific paper

The 8000-ton water IMB nucleon decay detector has good sensitivity to the neutrino burst associated with the collapse of stars. It is particularly sensitive to the nu-bar(e) charged current interactions with protons but can also record other neutrino interactions through nu(e) scattering. Signal, noise, physics objectives, and detector modifications that would enhance burst detection are discussed. The objectives include astrophysical questions about the pulse structure and power. It also may be possible with a distant source to study neutrino masses and neutrino oscillations.

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