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      Effects of Leptonic Nonunitarity on Lepton Flavor Violation, Neutrino Oscillation, Leptogenesis, and Lightest Neutrino Mass

      1 , 1
      Advances in High Energy Physics
      Hindawi Limited

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          Abstract

          Neutrino physics is a mature branch of science with all the three neutrino mixing angles and two mass squared differences determined with high precision. In spite of several experimental verifications of neutrino oscillations and precise measurements of two mass squared differences and the three mixing angles, the unitarity of the leptonic mixing matrix is not yet established, leaving room for the presence of small nonunitarity effects. Deriving the bounds on these nonunitarity parameters from existing experimental constraints, on cLFV decays such as μ e γ , μ τ γ , and τ e γ , we study their effects on the generation of baryon asymmetry through leptogenesis and neutrino oscillation probabilities. We consider a model where see-saw is extended by an additional singlet S which is very light but can give rise to nonunitarity effects without affecting the form on see-saw formula. We do a parameter scan of a minimal see-saw model in a type I see-saw framework satisfying the Planck data on baryon to photon ratio of the Universe, which lies in the interval 5.8 × 1 0 - 10 < Y B < 6.6 × 1 0 - 10 ( B B N ) . We predict values of lightest neutrino mass and Dirac and Majorana CP-violating phases δ C P , α , and β , for normal hierarchy and inverted hierarchy for one-flavor leptogenesis. It is worth mentioning that all these four quantities are unknown yet, and future experiments will be measuring them.

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          Oscillating neutrinos and mu --> e, gamma

          If neutrino masses and mixings are suitable to explain the atmospheric and solar neutrino fluxes, this amounts to contributions to FCNC processes, in particular mu --> e, gamma. If the theory is supersymmetric and the origin of the masses is a see-saw mechanism, we show that the prediction for BR(mu --> e, gamma) is in general larger than the experimental upper bound, especially if the largest Yukawa coupling is O(1) and the solar data are explained by a large angle MSW effect, which recent analyses suggest as the preferred scenario. Our analysis is bottom-up and completely general, i.e. it is based just on observable low-energy data. The work generalizes previous results of the literature, identifying the dominant contributions. Application of the results to scenarios with approximate top-neutrino unification, like SO(10) models, rules out most of them unless the leptonic Yukawa matrices satisfy very precise requirements. Other possible ways-out, like gauge mediated SUSY breaking, are also discussed.
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            Search for the lepton flavour violating decay \(\mu ^+ \rightarrow \mathrm {e}^+ \gamma \) μ + → e + γ with the full dataset of the MEG experiment

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              Leptogenesis

              Leptogenesis is a class of scenarios where the baryon asymmetry of the Universe is produced from a lepton asymmetry generated in the decays of a heavy sterile neutrino. We explain the motivation for leptogenesis. We review the basic mechanism, and describe subclasses of models. We then focus on recent developments in the understanding of leptogenesis: finite temperature effects, spectator processes, and in particular the significance of flavor physics.
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                Author and article information

                Journal
                Advances in High Energy Physics
                Advances in High Energy Physics
                Hindawi Limited
                1687-7357
                1687-7365
                June 25 2018
                June 25 2018
                : 2018
                : 1-10
                Affiliations
                [1 ]Department Of Physics, Gauhati University, Guwahati, Assam 781014, India
                Article
                10.1155/2018/5093251
                b6296109-6c08-4587-ba7f-2535e3f9c3bd
                © 2018

                http://creativecommons.org/licenses/by/4.0/

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