A neutrino mass model with S3 symmetry and see-saw interplay
Soumita Pramanick, Amitava Raychaudhuri (University of Calcutta)

TL;DR
This paper proposes a neutrino mass model based on S3 x Z3 symmetry that combines Type-I and Type-II see-saw mechanisms, predicting specific mixing angles and CP-violation effects consistent with current experimental hints.
Contribution
It introduces a novel S3 x Z3 symmetric see-saw model that links neutrino mixing angles, mass ordering, and CP phases, making testable predictions and exploring the interplay of different see-saw contributions.
Findings
Type-II see-saw sets atmospheric splitting and heta_{23} = rac{ ext{ extpi}}{4}
Type-I see-saw adjusts mixing angles to fit data
Model favors normal ordering with large CP-violation phases
Abstract
We develop a see-saw model for neutrino masses and mixing with an S3\times Z3 symmetry. It involves an interplay of Type-I and Type-II see-saw contributions of which the former is subdominant. The S3 \times Z3 quantum numbers of the fermion and scalar fields are chosen such that the Type-II see-saw generates a mass matrix which incorporates the atmospheric mass splitting and sets \theta_{23} = \pi/4. The solar splitting and \theta_{13} are absent, while the third mixing angle can achieve any value, \theta_{12}^0. Specific choices of \theta_{12}^0 are of interest, e.g., 35.3^\circ (tribimaximal), 45.0^\circ (bimaximal), 31.7^\circ (golden ratio), and 0^\circ (no solar mixing). The role of the Type-I see-saw is to nudge all the above into the range indicated by the data. The model results in novel interrelationships between these quantities due to their common origin, making it readily…
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