Dark $SU(2{)}_D$ Gauge Symmetry and Scotogenic Dirac Neutrinos

Abstract

Dark matter is postulated to transform under the non-Abelian $SU(2{)}_D$ gauge symmetry. Its connection to Dirac neutrino masses is explored.

16 pages, 10 figures

References in corpus (9)

• micrOMEGAs4.1: two dark matter candidates
• Status of the Higgs Singlet Extension of the Standard Model after LHC Run 1
• Discovering the Higgs Through Highly-Displaced Vertices
• Multi-Component Dark Matter
• Delta r and the W-boson mass in the Singlet Extension of the Standard Model
• Search for dark matter annihilation signals in the H.E.S.S. Inner Galaxy Survey
• Type II Dirac Seesaw with Observable $\Delta N_{\mathrm{eff}}$ in the light of W-mass Anomaly
• Leptonic Source of Dark Matter and Radiative Majorana or Dirac Neutrino Mass
• Linkage of Dirac Neutrinos to Dark U(1) Gauge Symmetry

Cited by in corpus (4)

• Pseudo-Nambu-Goldstone Dark Matter from Non-Abelian Gauge Symmetry
• Dark $SU(2)\to Z_3\times Z_2$ Gauge Symmetry
• Study on the global minimum and $H\to \gamma \gamma$ in the Dirac scotogenic model
• Flavor Imprints on Novel Low Mass Dark Matter