Ameliorating the popular lepton mixings with A4 symmetry: A see-saw model for realistic neutrino masses and mixing
Abstract
A model for neutrino masses and mixing is devised appointing the see-saw mechanism. The proffered model is fabricated with a combination of Type -I and Type-II see-saw contributions of which the latter dominates. The scalars and the leptons in the model are assigned A4 charges conducive to obtain the mass matrices viable for the scheme. The Type -II see-saw mass matrix accommodates atmospheric mass splitting and maximal mixing in the atmospheric sector (θ23=π/4). It is characterized by vanishing solar mass splitting and θ13 whereas the third neutrino mixing angle is free to acquire any value of θ120. Particular alternatives of θ120 corresponding to the popular lepton mixings viz. θ120=35.3 (tribimaximal), 45.0 (bimaximal), 31.7 (golden ratio) are accounted for. Another choice of θ120=0 (no solar mixing) is reckoned. The subdominant Type-I see-saw constituent of the model propels all the neutrino oscillation parameters into the ranges allowed by the data which in its turn get interrelated owing to their common origin. This makes the model testable in the light of future experimental data. As an example, θ23 emerges in the first (second) octant for normal (inverted) ordering. CP-violation is governed by phases present in the right-handed Majorana neutrino mass matrix, M R. Only normal ordering is allowed if these phases are absent. If M R is complex the Dirac CP-violating phase δ, is capable of being large, i.e., π/2, and inverted ordering of neutrino masses is also permitted. T2K and NOVA preliminary data favouring normal ordering and δ -π/2 predicts lightest neutrino mass to be 0.05 eV or more within the framework of this model.
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