Neutrino Masses and Mixing from Supersymmetric Inflation

Details Neutrino Masses and Mixing from Supersymmetric Inflation Neutrino Masses and Mixing from Supersymmetric Inflation

1998-01-19

arxiv.org/abs/hep-ph/9801340v1

Physics

High Energy Physics

High Energy Physics - Phenomenology

6 pages, 2 postscript figures, uses spocl.sty To be published in the proceedings of COSMO-97,International Workshop on Particl

Scientific paper

A supersymmetric model based on a left-right symmetric gauge group is proposed where hybrid inflation, baryogenesis and neutrino oscillations are linked.This scheme, supplemented by a familiar ansatz for the neutrino Dirac masses and mixing of the two heaviest families and with the MSW resolution of the solar neutrino puzzle, implies that $m_{\nu_{\tau}}$ lies between 1 and 9 eV. The mixing angle $\theta_{\mu \tau}$ is predicted to lie in a narrow range which will be partially tested by the Chorus/Nomad experiment.

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