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Supersymmetric Inflation, Baryogenesis and $\nu_{\mu} - \nu_{\tau}$ Oscillations
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, impl...
Autores principales: | , , |
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Lenguaje: | eng |
Publicado: |
1997
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Materias: | |
Acceso en línea: | https://dx.doi.org/10.1016/S0370-2693(98)00306-2 http://cds.cern.ch/record/328108 |
Sumario: | 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 CP violating phase \delta _{\mu \tau } is also discussed. |
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