English

$U(1)_\chi$ and Seesaw Dirac Neutrinos

High Energy Physics - Phenomenology 2019-01-08 v2

Abstract

In the context of SO(10)SU(5)×U(1)χSO(10) \to SU(5) \times U(1)_\chi, it is shown how seesaw Dirac neutrinos may be obtained. In this framework, U(1)U(1) lepton number is conserved, with which self-interaction dark matter with a light scalar dilepton mediator may be implemented. In addition, U(1)U(1) baryon number may be broken to (1)3B(-1)^{3B}, thereby generating a baryon asymmetry of the Universe. The axionic solution to the strong CPCP problem may also be incorporated.

Keywords

Cite

@article{arxiv.1811.09645,
  title  = {$U(1)_\chi$ and Seesaw Dirac Neutrinos},
  author = {Ernest Ma},
  journal= {arXiv preprint arXiv:1811.09645},
  year   = {2019}
}

Comments

10 pages, 1 figure (final version to appear in LHEP)