A Flavour-Symmetric Perspective on Neutrino Mixing

Details A Flavour-Symmetric Perspective on Neutrino Mixing A Flavour-Symmetric Perspective on Neutrino Mixing

2009-06-15

arxiv.org/abs/0906.2732v4

Physics

High Energy Physics

High Energy Physics - Phenomenology

16 pages latex. Written version of a talk presented by W. G. Scott at "Neutrino Telescopes", Venice, Italy, 10-13 March 2009 (

Scientific paper

A review and consolidation of some of our more recent publications, many with our various collaborators. While we cannot resist mentioning Tribimaximal mixing, our main theme is Flavour Symmetry, in particular Flavour-Symmetric Observables, scalar (or pseudo-scalar) under $S3_l \times S3_{\nu}$. Our "best guess" for the smallest neutrino mixing angle remains: $\sin \theta_{13}=\sqrt{2 \Delta m^2_{sol}/(3 \Delta m^2_{atm})} \simeq 0.13$.

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