Joshipura, Anjan S. ; Kodrani, Bhavik P. ; Patel, Ketan M. (2009) Fermion masses and mixings in a μ-τ symmetric SO(10) Physical Review D - Particles, Fields, Gravitation and Cosmology, 79 (11). p. 115017. ISSN 1550-7998
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Official URL: http://prd.aps.org/abstract/PRD/v79/i11/e115017
Related URL: http://dx.doi.org/10.1103/PhysRevD.79.115017
Abstract
The μ-T symmetry imposed on the neutrino mass matrix in the flavor basis is known to be quite predictive. We integrate this very specific neutrino symmetry into a more general framework based on the supersymmetric SO(10) grand unified theory. As in several other models, the fermion mass spectrum is determined by Hermitian mass matrices resulting from the renormalizable Yukawa couplings of the 16-plet of fermions with the Higgs fields transforming as 10, 126̅, and 120 representations of the SO(10) group. The μ-τ symmetry is spontaneously broken through the 120-plet. Consequences of this scheme are considered for fermion masses using both a type-I and a type-II seesaw mechanism. This scenario is shown to lead to a generalized CP invariance of the mass matrices and vanishing CP violating phases if the Yukawa couplings are invariant under the μ-τ symmetry. Small explicit breaking of the μ-τ symmetry is then shown to provide a very good understanding of all of the fermion masses and mixing. Detailed fits to the fermion spectrum are presented in several scenarios. One obtains a very good fit to all observables in the context of the type-I seesaw mechanism, but the type-II seesaw model also provides a good description except for the overall scale of the neutrino masses. Three major predictions on the leptonic mixing parameters in the type-I seesaw case are (i) the atmospheric mixing angle θ23l close to maximal, (ii) θ13l close to the present upper bound, and (iii) a negative but very small Dirac CP violating phase in the neutrino oscillations.
Item Type: | Article |
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Source: | Copyright of this article belongs to The American Physical Society. |
ID Code: | 67612 |
Deposited On: | 31 Oct 2011 05:28 |
Last Modified: | 31 Oct 2011 05:28 |
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