Radiative neutrino mass in an alternative $\operatorname{U}(1)_{B-L}$ gauge symmetry

DOI10.1016/J.NUCLPHYSB.2019.02.025zbMath1415.81127arXiv1705.08309OpenAlexW2964093329MaRDI QIDQ2421495

Hiroshi Okada, Takaaki Nomura

Publication date: 17 June 2019

Published in: Nuclear Physics. B (Search for Journal in Brave)

Full work available at URL: https://arxiv.org/abs/1705.08309

Mathematics Subject Classification ID

Unified quantum theories (81V22) Relativistic cosmology (83F05) Anomalies in quantum field theory (81T50) Symmetry breaking in quantum theory (81R40) Weak interaction in quantum theory (81V15)

Related Items (1)

Connecting low scale seesaw for neutrino mass to inelastic sub-GeV dark matter with abelian gauge symmetry

Cites Work

• A radiative model with a naturally mild neutrino mass hierarchy
• A critical analysis of one-loop neutrino mass models with minimal dark matter
• Electron/muon specific two Higgs doublet model
• Radiative neutrino mass with scotogenic scalar triplet
• Classically conformal radiative neutrino model with gauged \(B-L\) symmetry
• Scotogenic inverse seesaw model of neutrino mass
• CalcHEP 3.4~for collider physics within and beyond the standard model

This page was built for publication: Radiative neutrino mass in an alternative $\operatorname{U}(1)_{B-L}$ gauge symmetry