arXiv · hep-ph/0405261
Models of maximal atmospheric neutrino mixing and leptogenesis
Abstract
We discuss two extensions of the Standard Model based on the seesaw mechanism and on non-abelian family symmetry groups O(2) and $D_4$, respectively. Both models have a twofold-degenerate neutrino Dirac mass matrix $M_D$, a Majorana mass matrix invariant under a $μ$--$τ$ interchange symmetry and the predictions of maximal atmospheric neutrino mixing and vanishing mixing angle $θ_{13}$. Leptogenesis can naturally be incorporated if $10^{-3} \lesssim m_1 \lesssim 10^{-2}$ eV where $m_1$ the mass of the lightest neutrino and if the relevant heavy neutrinos are in the range $10^{11}$ to $10^{12}$ GeV. The $D_4$ model is more constrained and leptogenesis requires $m_1$ to be in the vicinity of $4 \times 10^{-3}$ eV.
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W. Grimus, L. Lavoura. 2004-05-26. Models of maximal atmospheric neutrino mixing and leptogenesis. https://doi.org/10.1142/9789812701824_0053
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