Neutrino masses from galactic supernovae and large water Čerenkov detectors

Details Neutrino masses from galactic supernovae and large water Čerenkov detectors Neutrino masses from galactic supernovae and large water Čerenkov detectors

Nov 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991nuphb.366..233s&link_type=abstract

Nuclear Physics B, Volume 366, Issue 1, p. 233-251.

Physics

Nuclear Physics

11

Scientific paper

The range of μ and τ neutrino masses accessible to large water Čerenkov detectors via the observation of neutrinos from galactic supernovae is discussed. We show that the available neutrino mass window from detecting late (t > 10 s) arrivals is ~ 75 eV-200 keV. A shortage of early (t < 0.1 s) events may signal a mass as small as 30 eV, but it seems unlikely that any technique using galactic supernovae may be used for masses as low as 10 eV.

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