Hierarchical Neutrinos and Supersymmetric Inflation
arXiv:hep-ph/9903511 · doi:10.1016/S0370-2693(99)00697-8
Abstract
A moderate extension of MSSM based on a left-right symmetric gauge group, within which hybrid inflation is `naturally' realized, is discussed. The mu problem is solved via a Peccei-Quinn symmetry. Light neutrinos acquire hierarchical masses by the seesaw mechanism. They are taken from the small angle MSW resolution of the solar neutrino puzzle and the SuperKamiokande data. The range of parameters consistent with maximal nu_mu-nu_tau mixing and the gravitino constraint is determined. The baryon asymmetry of the universe is generated through a primordial leptogenesis. The subrange of parameters, where the baryogenesis constraint is also met, is specified. The required values of parameters are more or less `natural'.
13 pages (including 2 figures), Revtex, minor corrections
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- New shifted hybrid inflation
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- S_3 Flavor Symmetry and Leptogenesis
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- Shift Symmetry and Higgs Inflation in Supergravity with Observable Gravitational Waves
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- Standard-smooth hybrid inflation
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- Type II Seesaw Origin of Non-zero and Leptogenesis
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- Particle Physics Approach to Dark Matter
- Leptogenesis
- Corrections to Scaling Neutrino Mixing: Non-zero and Baryon Asymmetry
- Density perturbations from both the inflaton and the curvaton
- -term as the origin of baryon and lepton number asymmetry
- Inverted neutrino mass hierarchies from U(1) symmetries
- Leptogenesis with Majorana neutrinos
- -Scale Resonant Leptogenesis with New Scaling Ansatz on Neutrino Dirac Mass Matrix from Flavor Symmetry