Natural framework for solar and 17-keV neutrinos

C. P. Burgess, J. M. Cline, and Markus A. Luty
Phys. Rev. D 46, 364 – Published 1 July 1992
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Abstract

Motivated by recent experimental claims for the existence of a 17-keV neutrino and by the solar-neutrino problem, we consider a class of models which contain in their low-energy spectrum a single light sterile neutrino and one or more Nambu-Goldstone bosons. In these models, the required pattern of small neutrino masses and Nambu-Goldstone-boson couplings are understood as the low-energy residue of the pattern of breaking of lepton-number symmetries near the electroweak scale, and all mass hierarchies are technically natural. The models are compatible with all cosmological and astrophysical constraints, and can solve the solar-neutrino problem either via the Mikheyev-Smirnov-Wolfenstein effect or vacuum oscillations. The deficit in atmospheric muon neutrinos seen in the Kamiokande and IMB detectors can also be explained in these models.

  • Received 5 February 1992

DOI:https://doi.org/10.1103/PhysRevD.46.364

©1992 American Physical Society

Authors & Affiliations

C. P. Burgess and J. M. Cline

  • Department of Physics, McGill University, 3600 University Street, Montréal, Québec, Canada H3A 2T8

Markus A. Luty

  • Physics Division, Lawrence Berkeley Laboratory, 1 Cyclotron Road, Berkeley, California 94707

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Issue

Vol. 46, Iss. 1 — 1 July 1992

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