Broken $S^{}_{3{\rm L}} \times S^{}_{3{\rm R}}$ Flavor Symmetry and Leptonic CP Violation
Abstract: In the framework of canonical seesaw model, we present a simple but viable scenario to explicitly break an $S{}_{3{\rm L}} \times S{}_{3{\rm R}}$ flavor symmetry in the leptonic sector. It turns out that the leptonic flavor mixing matrix is completely determined by the mass ratios of charged leptons (i.e., $m{}e/m{}\mu$ and $m{}\mu/m{}\tau$) and those of light neutrinos (i.e., $m{}_1/m{}_2$ and $m{}_2/m{}_3$). The latest global-fit results of three neutrino mixing angles ${\theta{}_{12}, \theta{}_{13}, \theta{}_{23}}$ and two neutrino mass-squared differences ${\Delta m2_{21}, \Delta m2_{31}}$ at the $3\sigma$ level are used to constrain the parameter space of ${m{}_1/m{}_2, m{}_2/m{}_3}$. The predictions for the mass spectrum and flavor mixing are highlighted: (1) The neutrino mass spectrum shows a hierarchical pattern and a normal ordering, e.g., $m{}_1 \approx 2.2~{\rm meV}$, $m{}_2 \approx 8.8~{\rm meV}$ and $m{}_3 \approx 52.7~{\rm meV}$; (2) Only the first octant of $\theta{}_{23}$ is allowed, namely, $41.8\circ \lesssim \theta{}_{23} \lesssim 43.3\circ$; (3) The Dirac CP-violating phase $\delta \approx -22\circ$ deviates significantly from the maximal value $-90\circ$. All these predictions are ready to be tested in the ongoing and forthcoming neutrino oscillation experiments. Moreover, we demonstrate that the cosmological matter-antimatter asymmetry can be explained via resonant leptogenesis, including the individual lepton-flavor effects. In our scenario, the leptonic CP violation at low- and high-energy scales are closely connected.
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