Pseudo Dirac neutrinos and the solar-neutrino problem

Details Pseudo Dirac neutrinos and the solar-neutrino problem Pseudo Dirac neutrinos and the solar-neutrino problem

May 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992phrvd..45.3316m&link_type=abstract

Physical Review D (Particles, Fields, Gravitation, and Cosmology), Volume 45, Issue 10, 15 May 1992, pp.R3316-R3320

Physics

9

Scientific paper

Observational consequences of the pseudo Dirac-neutrino hypothesis of Kobayashi, Lim, and Nojiri are examined in the context of the solar-neutrino problem. Detailed calculations are performed to obtain expected rates in the 37Cl, Kamiokande II, and 71Ga detectors. In a region of parameters consistent with the former two experiments the 71Ga rate is predicted to be 50-65 solar-neutrino units.

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