English

Radiative Neutrino Masses in a SUSY GUT Model

High Energy Physics - Phenomenology 2015-06-25 v4

Abstract

Radiatively-induced neutrino mass matrix is investigated within the framework of an SU(5) SUSY GUT model. The model has matter fields of three families \bar{5}_{L(+)i}+5_{L(+)i} in addition to the ordinary matter fields \bar{5}_{L(-)i}+10_{L(+)i} and Higgs fields H_{(+)}+\bar{H}_{(0)}, where (+,0,-) denote the transformation properties (\omega^{+1},\omega^0,\omega^{-1}) (\omega^3=+1) under a discrete symmetry Z_3. R-parity violating terms are given by \bar{5}_{L(+)} \bar{5}_{L(+)} 10_{L(+)}, while the Yukawa interactions are given by \bar{H}_{(0)} \bar{5}_{L(-)} 10_{L(+)}, i.e. the \bar{5}-fields in both are different from each other. The Z_3 symmetry is only broken by the terms \bar{5}_{L(+)i}5_{L(+)i} softly, so that the \bar{5}_{L(+)i}\leftrightarrow \bar{5}_{L(-)i} mixings appear at \mu < M_X. Of the R-parity violating terms \bar{5}_{L(+)} \bar{5}_{L(+)} 10_{L(+)}, only the terms (e_L\nu_-\nu_Le_)e_R^c sizably appear at \mu < M_X.

Keywords

Cite

@article{arxiv.hep-ph/0308097,
  title  = {Radiative Neutrino Masses in a SUSY GUT Model},
  author = {Yoshio Koide},
  journal= {arXiv preprint arXiv:hep-ph/0308097},
  year   = {2015}
}

Comments

10 pages, Latex, a typo was corrected