Leptonic mixing matrix in terms of Cabibbo angle

preprint2013arXivOpen access

Abstract

We phenomenologically build a neutrino mass matrix obeying μ−τμ-τ symmetry with only two parameters, Cabibbo angle (λ)(λ) and a flavour twister parameter (η)(η). For vanishing ηη, the model assumes TBM mixing. When η=λη=λ, the model generates a solar mixing angle and solar mass squared difference that coincide with the experimental best-fits. It motivates us to propose a mixing matrix in the neutrino sector with sinθ12<13 sinθ_{12}<\frac{1}{\sqrt{3}}, θ13=0θ_{13}=0 and θ23=π/4θ_{23}=π/4. The corrections in θ13θ_{13} and θ23θ_{23} are conducted following the breaking of μ−τμ-τ symmetry, by choosing a proper unitary diagonalizing charged lepton matrix, and this ensures that θ23θ_{23} lies within the first octant. The Cabibbo angle (λ=sin⁡θc)(λ=\sinθ_{c}) plays the role of a guiding parameter in both neutrino as well as leptonic sector. The effect of the Dirac CP violating phase δcpδ_{cp} is also studied when it enters either through the charged lepton diagonalizing matrix or through neutrino mixing matrix.

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