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Prospects for detection of a cosmologically significant neutrino mass from a galactic supernova neutrino burst using a neutral-current-based detector.

Author(s): Cline, DB; Fuller, GM; Hong, WP; Meyer, B; Wilson, J | Abstract: We discuss how proposed supernova neutrino detectors could measure masses for or neutrinos in the range of 15 to 50 eV. The range for measurable masses might be extended down to 5 eV, depending on our confidence in some of the predicted features of the supernova-neutrino-burst signal. We discuss the expected characteristics of supernova neutrino signals in proposed neutral-current-based detectors. © 1994 The American Physical Society.