Neutrino mass explanations of solar and atmospheric neutrino deficits and hot dark matter

David O. Caldwell and Rabindra N. Mohapatra
Phys. Rev. D 48, 3259 – Published 1 October 1993
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Abstract

If the solar and atmospheric neutrino deficits and the apparent need for a hot dark matter component all result from neutrino mass, one of three neutrino mass patterns is required. Of these, two appear quite unlikely, leading to a unique solution which points to further experimental tests. We briefly outline possible theoretical models which could generate these three neutrino mass matrices without adjustment of parameters.

  • Received 17 March 1993

DOI:https://doi.org/10.1103/PhysRevD.48.3259

©1993 American Physical Society

Authors & Affiliations

David O. Caldwell

  • Department of Physics, University of California, Santa Barbara, California 93106-9530

Rabindra N. Mohapatra

  • Department of Physics, University of Maryland, College Park, Maryland 20742

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Issue

Vol. 48, Iss. 7 — 1 October 1993

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