Generating from sterile neutrinos in symmetric models
arXiv:1507.07030 · doi:10.1103/PhysRevD.92.073009
Abstract
The smallness of the mixing angle as observed in neutrino oscillation experiments can be understood through an approximated exchange symmetry in the neutrino mass matrix. Using recent oscillation neutrino data, but assuming no \textit{CP} violation, we study breaking parameter space to establish the conditions under which such a breaking could have a perturbative origin. According to the so-obtained conditions, we suggest that a sterile neutrino, matching LSND/MiniBooNE neutrino oscillation results, could provide the necessary ingredients to properly fix atmospheric and mixing angles to observable values, without exceeding the sterile neutrino fraction bound in solar oscillations. In such a scenario, we analyze the general effect of a fourth neutrino on the prediction for the effective majorana mass parameter.
Version accepted for publication in PRD, 19 pages, 5 figures, references added
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Cited by in corpus (20)
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- The - reflection symmetry of Majorana neutrinos
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- Compatibility of Flavour Symmetric Minimal Extended Seesaw with Neutrino Data
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- Texture zeros of low-energy Majorana neutrino mass matrix in 3+1 scheme
- model with symmetry for activesterile neutrino mixing
- Deviations in Tribimaximal Mixing From Sterile Neutrino Sector
- Deviations to symmetry in a cobimaximal scenario
- Leptonic CP phases near the symmetric limit
- New mixing schemes for (3+1) neutrinos
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- Further study on the textures of neutrino mass matrix for maximal atmospherical mixing angle and Dirac CP phase
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- Dirac neutrino mixings from hidden symmetry
- Dirac CP phases in a 3+1 neutrino scenario with symmetry