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Neutrino masses and mixings

Conference ·
OSTI ID:10186103
Theoretical prejudices, cosmology, and neutrino oscillation experiments all suggest neutrino mass are far below present direct experimental limits. Four interesting scenarios and their implications are discussed: (1) a 17 keV {nu}{sub {tau}}, (2) a 30 ev {nu}{sub {tau}} making up the dark matter, (3) a 10{sup {minus}3} ev {nu}{sub {mu}} to solve the solar neutrino problem, and (4) a three-neutrino MSW solution.
Research Organization:
Carnegie-Mellon Univ., Pittsburgh, PA (United States). Dept. of Physics
Sponsoring Organization:
USDOE, Washington, DC (United States)
DOE Contract Number:
FG02-91ER40682
OSTI ID:
10186103
Report Number(s):
CONF-910836--7; CMU-HEP--91-15; ON: DE93018867
Country of Publication:
United States
Language:
English

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