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Non-Abelian family symmetries in Pati-Salam unification · Around

2011

Non-Abelian family symmetries in Pati-Salam unification

Varzielas, Ivo de Medeiros

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We present a framework of underlying SU(3) x SU(3) family symmetries consistent with Pati-Salam unification and discuss advantages that can justify introducing multiple non-Abelian factors.

Advantages include improved vacuum alignment and increased predictivity.
We explore in this framework deviations from tri-bi-maximal neutrinos, such as relatively large theta13.

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G. G. Ross, L. Velasco-Sevilla, and O. Vives, Spontaneous CP violation and nonAbelian family symmetry in SUSY
2004
Earlier work this paper cites.
S. King, Predicting neutrino parameters from SO(3) family symmetry and quark-lepton unification
2005
Earlier work this paper cites.
T. Appelquist, Y. Bai, and M. Piai, Quark mass ratios and mixing angles from SU(3) family gauge symmetry
2006
Earlier work this paper cites.
I. de Medeiros Varzielas and G. G. Ross, SU(3) family symmetry and neutrino bi-tri-maximal mixing
2006
Earlier work this paper cites.
I. de Medeiros Varzielas, S. F. King, and G. G. Ross, Neutrino tri-bi-maximal mixing from a non-Abelian discrete family symmetry
2007
Earlier work this paper cites.
C. Luhn, S. Nasri, and P. Ramond, Tri-Bimaximal Neutrino Mixing and the Family Symmetry Z 7 ⋊ Z 3 Z_{7}\rtimes Z_{3}
Original
2007
Earlier work this paper cites.

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T. Schwetz, M. Tortola, and J. W. F. Valle, Where we are on θ 13 \theta_{13} : addendum to ’Global neutrino data and recent reactor fluxes: status of three- flavour oscillation parameters’
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