Supersymmetric Inflation, Baryogenesis and ν_μ - ν_τ Oscillations

Details Supersymmetric Inflation, Baryogenesis and ν_μ - ν_τ Oscillations Supersymmetric Inflation, Baryogenesis and ν_μ - ν_τ Oscillations

1997-06-17

arxiv.org/abs/hep-ph/9706385v1

Phys.Lett.B427:53-58,1998

Physics

High Energy Physics

High Energy Physics - Phenomenology

10 pages RevTeX 3 eps figures. email: vlachos@physics.auth.gr

Scientific paper

10.1016/S0370-2693(98)00306-2

In a supersymmetric left-right symmetric model, inflation, baryogenesis (via leptogenesis) and neutrino oscillations can become closely linked. A familiar ansatz for the neutrino Dirac masses and mixing of the two heaviest families, together with the MSW resolution of the solar neutrino puzzle, imply that 1 eV <_\sim m_{\nu _{\tau }<_\sim 9 eV. The predicted range for the mixing angle \theta _\mu \tau will be partially tested by the Chorus/Nomad experiment. The CP violating phase \delta _{\mu \tau } is also discussed.

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