TY - JOUR
T1 - Consequences of a 17-keV neutrino
AU - Caldwell, David O.
AU - Langacker, Paul
N1 - Copyright:
Copyright 2015 Elsevier B.V., All rights reserved.
PY - 1991
Y1 - 1991
N2 - If the controversial 17-keV neutrino exists, laboratory, astrophysical and cosmological bounds, unless significantly weakened, require that (1) it be a Majorana neutrino and mainly ; (2) it not be the dark matter of the universe, although its existence would rule out dominant hot dark matter; (3) the be a heavy Majorana neutrino of mass 17 keV or in the range 170270 keV; and (4) the Mikheyev-Smirnov-Wolfenstein solution to the solar-neutrino problem involve e conversion to a light sterile [SU(2)-singlet] neutrino.
AB - If the controversial 17-keV neutrino exists, laboratory, astrophysical and cosmological bounds, unless significantly weakened, require that (1) it be a Majorana neutrino and mainly ; (2) it not be the dark matter of the universe, although its existence would rule out dominant hot dark matter; (3) the be a heavy Majorana neutrino of mass 17 keV or in the range 170270 keV; and (4) the Mikheyev-Smirnov-Wolfenstein solution to the solar-neutrino problem involve e conversion to a light sterile [SU(2)-singlet] neutrino.
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U2 - 10.1103/PhysRevD.44.823
DO - 10.1103/PhysRevD.44.823
M3 - Article
AN - SCOPUS:24544481628
SN - 1550-7998
VL - 44
SP - 823
EP - 828
JO - Physical review D: Particles and fields
JF - Physical review D: Particles and fields
IS - 3
ER -