Supersymmetric Inflation, Baryogenesis and ν_μ - ν_τ Oscillations

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dc.creatorLazarides, G.
dc.creatorShafi, Q.
dc.creatorVlachos, N. D.
dc.date1997-06-17
dc.date.accessioned2026-07-07T11:35:23Z
dc.date.available2026-07-07T11:35:23Z
dc.descriptionIn 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_{ν_{τ}<_\sim 9 eV. The predicted range for the mixing angle θ_μτwill be partially tested by the Chorus/Nomad experiment. The CP violating phase δ_{μτ} is also discussed.
dc.description10 pages RevTeX 3 eps figures. email: vlachos@physics.auth.gr
dc.identifierhttps://arxiv.org/abs/hep-ph/9706385
dc.identifierhttp://arxiv.org/abs/hep-ph/9706385
dc.identifierPhys.Lett.B427:53-58,1998
dc.identifierdoi:10.1016/S0370-2693(98)00306-2
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/198573
dc.subjectHigh Energy Physics - Phenomenology
dc.subjectAstrophysics
dc.titleSupersymmetric Inflation, Baryogenesis and ν_μ - ν_τ Oscillations
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