English

Unified Models of Neutrinos, Flavour and CP Violation

High Energy Physics - Phenomenology 2017-04-05 v1

Abstract

Recent data from neutrino experiments gives intriguing hints about the mass ordering, the CP violating phase and non-maximal atmospheric mixing. There seems to be a (one sigma) preference for a normal ordered (NO) neutrino mass pattern, with a CP phase δ=100±50\delta = -100^{\circ}\pm 50 ^\circ, and (more significantly) non-maximal atmospheric mixing. Global fits for the NO case yield lepton mixing angle one sigma ranges: θ2341.4±1.6\theta_{23}\approx 41.4^\circ \pm 1.6^\circ, θ1233.2±1.2\theta_{12}\approx 33.2^\circ \pm 1.2^\circ, θ138.45±0.15\theta_{13}\approx 8.45^\circ \pm 0.15^\circ. Cosmology gives a limit on the total of the three masses to be below about 0.230.23 eV, favouring hierarchical neutrino masses over quasi-degenerate masses. Given such experimental advances, it seems an opportune moment to review the theoretical status of attempts to explain such a pattern of neutrino masses and lepton mixing, focussing on approaches based on the four pillars of: {\em predictivity}, {\em minimality}, {\em robustness} and {\em unification}. {\em Predictivity} can result from various mixing sum rules whose status is reviewed. {\em Minimality} can follow from the type I seesaw mechanism, including constrained sequential dominance of right-handed (RH) neutrinos, and the littlest seesaw model. {\em Robustness} requires enforcing a discrete CP and non-Abelian family symmetry, spontaneously broken by flavons with the symmetry preserved in a semi-direct way. {\em Unification} can account for all lepton and quark masses, mixing angles and CP phases, as in Supersymmetric Grand Unified Theories of Flavour, with possible string theory origin.

Keywords

Cite

@article{arxiv.1701.04413,
  title  = {Unified Models of Neutrinos, Flavour and CP Violation},
  author = {S. F. King},
  journal= {arXiv preprint arXiv:1701.04413},
  year   = {2017}
}

Comments

67 pages, 29 figures, review article to appear in Progr.Part.Nucl.Phys