Testing constrained sequential dominance models of neutrinos

preprint2015arXivOpen access

Abstract

Constrained sequential dominance (CSD) is a natural framework for implementing the see-saw mechanism of neutrino masses which allows the mixing angles and phases to be accurately predicted in terms of relatively few input parameters. We analyze a class of CSD(nn) models where, in the flavour basis, two right-handed neutrinos are dominantly responsible for the "atmospheric" and "solar" neutrino masses with Yukawa couplings to (νe,νμ,ντ)(ν_e, ν_μ, ν_τ) proportional to (0,1,1)(0,1,1) and (1,n,n−2)(1,n,n-2), respectively, where nn is a positive integer. These coupling patterns may arise in indirect family symmetry models based on A4A_4. With two right-handed neutrinos, using a χ2χ^2 test, we find a good agreement with data for CSD(3) and CSD(4) where the entire PMNS mixing matrix is controlled by a single phase ηη, which takes simple values, leading to accurate predictions for mixing angles and the magnitude of the oscillation phase ∣δCP∣|δ_{CP}|. We carefully study the perturbing effect of a third "decoupled" right-handed neutrino, leading to a bound on the lightest physical neutrino mass m1≲1m_1 \lesssim 1 meV for the viable cases, corresponding to a normal neutrino mass hierarchy. We also discuss a direct link between the oscillation phase δCPδ_{CP} and leptogenesis in CSD(nn) due to the same see-saw phase ηη appearing in both the neutrino mass matrix and leptogenesis.

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