English

Radiative generation of neutrino masses in a 3-3-1 type model

High Energy Physics - Phenomenology 2020-05-15 v2

Abstract

A new model for tiny neutrino masses is proposed in the gauge theory of SU(3)CSU(3)LU(1)XSU(3)_C \otimes SU(3)_L \otimes U(1)_X, where neutrino masses are generated via the quantum effect of new particles. In this model, the fermion content is taken to be minimal to realize the gauge anomaly cancellation, while the scalar sector is extended from the minimal 3-3-1 model to have an additional SU(3)LSU(3)_L triplet field. After SU(3)LU(1)XSU(3)_L\otimes U(1)_X is broken into SU(2)LU(1)YSU(2)_L\otimes U(1)_Y, the "Zee model" like diagrams are naturally induced, which contain sufficient lepton flavor violating interactions to reproduce current neutrino oscillation data. Furthermore, the remnant Z2Z_2 symmetry appears after the electroweak symmetry breaking, which guarantees the stability of dark matter. It is confirmed that this model can satisfy current dark matter data. As an important prediction to test this model, productions and decays of doubly-charged scalar bosons at collider experiments are discussed in successful benchmark scenarios.

Keywords

Cite

@article{arxiv.2003.05857,
  title  = {Radiative generation of neutrino masses in a 3-3-1 type model},
  author = {Arindam Das and Kazuki Enomoto and Shinya Kanemura and Kei Yagyu},
  journal= {arXiv preprint arXiv:2003.05857},
  year   = {2020}
}

Comments

35 pages, 8 figures, 4 tables; Version published in Phys. Rev. D