Phenomenological neutrino mass matrix for neutrino oscillations and dark matter

Details Phenomenological neutrino mass matrix for neutrino oscillations and dark matter Phenomenological neutrino mass matrix for neutrino oscillations and dark matter

1997-11-15

arxiv.org/abs/hep-ph/9711340v2

Prog.Theor.Phys.99:483-488,1998

Physics

High Energy Physics

High Energy Physics - Phenomenology

8 pages, latex, minor changes and a new reference added, to be published in Prog. Theor. Phys

Scientific paper

10.1143/PTP.99.483

A phenomenological neutrino mass matrix is proposed to explain the solar and atmospheric neutrino deficits and to present the neutrino as a candidate of hot dark matter in the $3\nu_L+3\nu_R$ framework. The realization of mixing angles which can explain the solar and atmospheric neutrino problems is taken as the first criterion in this construction. The differences among neutrino mass eigenvalues are introduced as a perturbation. In this scheme the structure of a charged lepton mass matrix is not severely constrained by the solar and atmospheric neutrino data.

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