Normal and Special Models of Neutrino Masses and Mixings

Abstract

One can make a distinction between "normal" and "special" models. For normal models ${\theta }_{23}$ is not too close to maximal and ${\theta }_{13}$ is not too small, typically a small power of the self-suggesting order parameter $\sqrt{r}$, with $r=\Delta m_{sol}^2/\Delta m_{atm}^2\sim 1/35$. Special models are those where some symmetry or dynamical feature assures in a natural way the near vanishing of ${\theta }_{13}$ and/or of ${\theta }_{23}-\pi /4$. Normal models are conceptually more economical and much simpler to construct. Here we focus on special models, in particular a recent one based on A4 discrete symmetry and extra dimensions that leads in a natural way to a Harrison-Perkins-Scott mixing matrix.

To be published in the Proceedings of Rencontres de Physique de la Vallée d'Aoste, La Thuile, Italy

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