English

Lepton mixing angle $\theta_{13} = 0$ with a horizontal symmetry $D_4$

High Energy Physics - Phenomenology 2009-11-10 v1

Abstract

We discuss a model for the lepton sector based on the seesaw mechanism and on a D4D_4 family symmetry. The model predicts the mixing angle θ13\theta_{13} to vanish. The solar mixing angle θ12\theta_{12} is free--it will in general be large if one does not invoke finetuning. The model has an enlarged scalar sector with three Higgs doublets, together with two real scalar gauge singlets χi\chi_i (i=1,2 i = 1, 2) which have vacuum expectation values < \chi_i >_0attheseesawscale.Theatmosphericmixingangle at the seesaw scale. The atmospheric mixing angle \theta_{23}isgivenby is given by \tan \theta_{23} = <\chi_2>_0/<χ1>0 /<\chi_1>_0, and it is maximal if the Lagrangian is D4D_4-invariant; but D4D_4 may be broken softly, by a term of dimension two in the scalar potential, and then < \chi_2_0 becomes different from < \chi_1_0. Thus, the strength of the soft D4D_4 breaking controls the deviation of θ23\theta_{23} from π/4\pi / 4. The model predicts a normal neutrino mass spectrum (m3>m2>m1m_3 > m_2 > m_1) and allows successful leptogenesis if m14×103eVm_1 \sim 4 \times 10^{-3} \mathrm{eV}; these properties of the model are independent of the presence and strength of the soft D4D_4 breaking.

Keywords

Cite

@article{arxiv.hep-ph/0407112,
  title  = {Lepton mixing angle $\theta_{13} = 0$ with a horizontal symmetry $D_4$},
  author = {W. Grimus and A. S. Joshipura and S. Kaneko and L. Lavoura and M. Tanimoto},
  journal= {arXiv preprint arXiv:hep-ph/0407112},
  year   = {2009}
}

Comments

13 pages, one figure