TY - JOUR
T1 - Neutrino mass and detection of neutrino supernova bursts
AU - Piran, Tsvi
PY - 1981/6/18
Y1 - 1981/6/18
N2 - A neutrino mass will cause a dispersion in the arrival time of a neutrino burst from a supernova explosion. Such a dispersion may reduce the sensitivity of neutrino detectors to such bursts. Detection of a dispersed neutrino burst could yield a direct measurement of the neutrino mass if it is in the range mν≳0.1 eV.
AB - A neutrino mass will cause a dispersion in the arrival time of a neutrino burst from a supernova explosion. Such a dispersion may reduce the sensitivity of neutrino detectors to such bursts. Detection of a dispersed neutrino burst could yield a direct measurement of the neutrino mass if it is in the range mν≳0.1 eV.
UR - http://www.scopus.com/inward/record.url?scp=0038537903&partnerID=8YFLogxK
U2 - 10.1016/0370-2693(81)90880-7
DO - 10.1016/0370-2693(81)90880-7
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AN - SCOPUS:0038537903
SN - 0370-2693
VL - 102
SP - 299
EP - 302
JO - Physics Letters, Section B: Nuclear, Elementary Particle and High-Energy Physics
JF - Physics Letters, Section B: Nuclear, Elementary Particle and High-Energy Physics
IS - 4
ER -