Constraints on 17-keV neutrinos

Details Constraints on 17-keV neutrinos Constraints on 17-keV neutrinos

Jan 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992phrvl..68..270c&link_type=abstract

Physical Review Letters (ISSN 0031-9007), vol. 68, Jan. 20, 1992, p. 270-273.

Astronomy and Astrophysics

Astrophysics

13

Neutrinos, Nuclear Astrophysics, Nuclear Fusion, Radiative Lifetime, Radioactive Decay, Supernova 1987A, Weak Interactions (Field Theory)

Scientific paper

Recent experiments indicate that a 17-keV neutrino mixes with nu(e) with
1-percent probability. The constraints from neutrinoless double-beta
decay, cosmology, and astrophysics that any model possessing a 17-keV
neutrino must obey are discussed. Several recently proposed models are
shown to be incompatible with these constraints.

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