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Obtaining a nonzero  13 in lepton models based on SO(3)  A 4

Obtaining a nonzero  13 in lepton models based on SO(3)  A 4. Yuval Grossman and Wee Hao Ng , Cornell University. arXiv:1404.1413 [ hep -ph]. Phenomenology 2014. Outline. Tri- bimaximal mixing found and lost; how do A 4 models cope? Basics of SO(3)  A 4 model

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Obtaining a nonzero  13 in lepton models based on SO(3)  A 4

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  1. Obtaining a nonzero 13 in lepton models based on SO(3)  A4 Yuval Grossman and Wee Hao Ng, Cornell University arXiv:1404.1413 [hep-ph] Phenomenology 2014

  2. Outline • Tri-bimaximal mixing found and lost; how do A4 models cope? • Basics of SO(3)  A4 model • Nonzero 13 in SO(3)  A4 model • Summary

  3. Tri-bimaximal mixing and A4 models • For long time, PMNS matrix thought to be consistent with TBM • Highly specific pattern… discrete lepton flavor symmetries?

  4. Tri-bimaximal mixing and A4 models • Simplest A4 lepton models • Components • SM Higgs and leptons • Right handed neutrinos • Scalar flavons, ’ • Features • Additional Z2 symmetry so flavonssectorized • Flavons gain VEV  = (v, v, v), ’ = (v’, 0, 0) Representations of A4  TBM!

  5. Tri-bimaximal mixing… lost • Recently, 13 found to be much larger! • Daya Bay (2012): • RENO (2012): • TBM ruled out!

  6. How do A4 models cope? • Actually many A4 models already allow this! • Approaches: • Higher dimension operators, e.g. [Altarelli and Meloni (2009)] • More flavons, e.g. [Chen et al (2013)] • Perturb flavon alignments, e.g. [King (2011)] • Radiative corrections, e.g. [Antusch et al (2003)]

  7. Continuous symmetry  A4 • Class of models based on continuous symmetry  A4. • Originally motivated to explain origin of A4. • Specific example: SO(3)  A4 [Berger and Grossman (2009)] • Turns out 13 already nonzero at tree level! • Even better: 13 related to

  8. Basics of SO(3)  A4 model Left-handed leptons Right-handed leptons Scalars

  9. Basics of SO(3)  A4 model • Most general Lagrangian for leptons • Flavons gain VEV 3D coordinate basis vectors  6  6 mass matrices

  10. Obtaining UPMNS • UPMNS characterize charged-current interactions between light eigenstates. • 6  6 mass matrices: • Block-diagonalise6  6 mass matrices. • Then diagonalise 3  3 mass matrices. • Neutrinos:

  11. Obtaining UPMNS • Charged leptons:

  12. Nonzero 13 • Block diagonalize • Useful to define • Then • Expanding in small parameter • LO: • NLO: 13 still 0! Suggests 13 ~ !

  13. Nonzero 13 • Actual contribution to 13 from deviation turns out to be ~ (m/m)  ~ 10 • Random simulation results In agreement with predictions!

  14. Summary and further work • TBM ruled out, but many A4 models allow for this scenario • In particular, SO(3)  A4 model allow nonzero tree-level 13 of size • % level separation of A4 and SO(3) breaking scales

  15. Thank you!

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