Db. Cline et al., PROSPECTS FOR DETECTION OF A COSMOLOGICALLY SIGNIFICANT NEUTRINO MASSFROM A GALACTIC SUPERNOVA NEUTRINO BURST USING A NEUTRAL-CURRENT-BASED DETECTOR, Physical review. D. Particles and fields, 50(2), 1994, pp. 720-729
We discuss how proposed supernova neutrino detectors could measure mas
ses for nu(mu) or nu(tau) neutrinos in the range of 15 to 50 eV. The r
ange for measurable masses might be extended down to 5 eV, depending o
n our confidence in some of the predicted features of the supernova-ne
utrino-burst signal. We discuss the expected characteristics of supern
ova neutrino signals in proposed neutral-current-based detectors.