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Title: Class of models leading to depletions of solar. nu. sub e and atmospheric. nu. sub. mu. fluxes

Journal Article · · Physical Review, D (Particles Fields); (United States)
 [1]
  1. Department of Physics, Northern Illinois University, DeKalb, Illinois 60115 (United States) Fermi National Accelerator Laboratory, P. O. Box 500, Batavia, Illinois 60510 (United States)

A model incorporating three left-handed SU(2){sub {ital L}}{times}U(1){sub {ital Y}}-doublet neutrinos and three right-handed singlet neutrinos, with leptonic Dirac mass submatrices similar to empirical forms which work well for quarks, is required to yield both the nonadiabatic Mikheyev-Smirnov-Wolfenstein solar neutrino effect and the depleted flux of atmospheric muon neutrinos observed by Kamiokande. We find a small segment of the {delta}{ital m}{sub 23}{sup 2} vs sin{sup 2}2{theta}{sub 23} plane exists where such solutions can be achieved and identify the class or right-handed Majorana submatrices required.

OSTI ID:
7235303
Journal Information:
Physical Review, D (Particles Fields); (United States), Vol. 45:3; ISSN 0556-2821
Country of Publication:
United States
Language:
English

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