Testing constrained sequential dominance models of neutrinos
arXiv:1412.6996
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() models where, in the flavour basis, two right-handed neutrinos are dominantly responsible for the "atmospheric" and "solar" neutrino masses with Yukawa couplings to proportional to and , respectively, where is a positive integer. These coupling patterns may arise in indirect family symmetry models based on . With two right-handed neutrinos, using a 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 , which takes simple values, leading to accurate predictions for mixing angles and the magnitude of the oscillation phase . We carefully study the perturbing effect of a third "decoupled" right-handed neutrino, leading to a bound on the lightest physical neutrino mass meV for the viable cases, corresponding to a normal neutrino mass hierarchy. We also discuss a direct link between the oscillation phase and leptogenesis in CSD() due to the same see-saw phase appearing in both the neutrino mass matrix and leptogenesis.
34 pages, 15 figures. Version to be published in J.Phys G. Note the change in title. Clarifying comments added. Previous versions: 32 pages, 15 figures. Improved discussion of chi squared analysis, new plots added. // 29 pages, 13 figures. Minor changes and discussion about the origin of the vacuum alignments added to an Appendix
References in corpus (6)
- On the origin of neutrino flavour symmetry
- Lepton Mixing Predictions including Majorana Phases from Flavour Symmetry and Generalised CP
- Decrypting -inspired leptogenesis
- Successful leptogenesis with flavour coupling effects in realistic unified models
- Vacuum misalignment corrections to tri-bimaximal mixing and form dominance
- Quark mixing from Delta(6N^2) family symmetry