English

Generalized Tri-bimaximal Neutrino Mixing and Its Sensitivity to Radiative Corrections

High Energy Physics - Phenomenology 2009-11-11 v3

Abstract

We argue that the tri-bimaximal neutrino mixing pattern V0V_0 or its generalized form V0V'_0, which includes two arbitrary Majorana phases of CP violation, may result from an underlying flavor symmetry at a superhigh energy scale close to the seesaw scale (1014\sim 10^{14} GeV). Taking the working assumption that three neutrino masses are nearly degenerate, we calculate radiative corrections to V0V_0 and V0V'_0 in their evolution down to the electroweak scale (102\sim 10^2 GeV). Three mixing angles of V0V_0 or V0V'_0 are essentially stable against radiative corrections in the standard model (SM). In the minimal supersymmetric standard model (MSSM), however, V0V_0 is in general disfavored and V0V'_0 can be compatible with current neutrino oscillation data if its two Majorana phases α1\alpha^{}_1 and α2\alpha^{}_2 are properly fine-tuned. We also find that it is possible to radiatively generate the CP-violating phase δ\delta from α1\alpha^{}_1 and α2\alpha^{}_2, and \delta may keep on staying at its fixed point in either the SM or the MSSM.

Keywords

Cite

@article{arxiv.hep-ph/0509065,
  title  = {Generalized Tri-bimaximal Neutrino Mixing and Its Sensitivity to Radiative Corrections},
  author = {Shu Luo and Zhi-zhong Xing},
  journal= {arXiv preprint arXiv:hep-ph/0509065},
  year   = {2009}
}

Comments

RevTex 14 pages, 2 figures. Table I corrected. Minor changes made. More discussions added