Dirac Neutrino Mass Matrix and its Link to Freeze-in Dark Matter

Abstract

Using a mechanism which allows naturally small Dirac neutrino masses and its linkage to a dark gauge $U(1{)}_D$ symmetry, a realistic Dirac neutrino mass matrix is derived from $S_3$. The dark sector naturally contains a fermion singlet having a small seesaw mass. It is thus a good candidate for freeze-in dark matter from the decay of the $U(1{)}_D$ Higgs boson.

9 pages, no figure

References in corpus (2)

• Gauging U(1) symmetries and the number of right-handed neutrinos
• Linkage of Dirac Neutrinos to Dark U(1) Gauge Symmetry

Cited by in corpus (8)

• Seesaw determination of the dark matter relic density
• Gauged Lepton Number, Dirac Neutrinos, Dark Matter, and Muon $g-2$
• Revisiting the Dirac Nature of Neutrinos in the Light of $\Delta (27)$ and Cyclic Symmetries
• Cobimaximal Mixing with Dirac Neutrinos
• Naturally Light Dirac Neutrinos from SU(6)
• Naturally Light Dirac Neutrinos from $SO(10)\times U(1{)}_{\psi }$
• Neutrino mass matrices from localization in M-theory on $G_2$ orbifold
• Dirac Neutrinos and Dark Matter within a Minimal Discrete Symmetry Model