Radiative neutrino mass with scotogenic scalar triplet

DOI10.1016/J.PHYSLETB.2013.11.045zbMath1377.81248arXiv1310.3183OpenAlexW1984897319MaRDI QIDQ1690728

Ivica Picek, Branimir Radovčić, Vedran Brdar

Publication date: 12 January 2018

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

Full work available at URL: https://arxiv.org/abs/1310.3183

zbMATH Keywords

dark matterneutrino mass

Mathematics Subject Classification ID

Unified quantum theories (81V22) Symmetry breaking in quantum theory (81R40)

Related Items (4)

One-loop type II seesaw neutrino model with stable dark matter candidates ⋮ Scotogenic R\(\nu\)MDM at three-loop level ⋮ Radiative neutrino mass in an alternative $\operatorname{U}(1)_{B-L}$ gauge symmetry ⋮ A critical analysis of one-loop neutrino mass models with minimal dark matter

Cites Work

• Enhancement of \(h \to \gamma \gamma\) by seesaw-motivated exotic scalars
• The simplest models of radiative neutrino mass

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