Fermion Triplet Dark Matter and Radiative Neutrino Mass

Abstract

The neutral member of a Majorana fermion triplet (Sigma^+,Sigma^0,Sigma^-) is proposed as a candidate for the dark matter of the Universe. It may also serve as the seesaw anchor for obtaining a radiative neutrino mass.

11 pages

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• Wino-like Minimal Dark Matter and future colliders
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• Anomaly Induced Dark Matter Decay and PAMELA/ATIC Experiments
• Triviality and vacuum stability bounds in the three-loop neutrino mass model
• A Class of Three-Loop Models with Neutrino Mass and Dark Matter
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• Inverse Seesaw Neutrino Mass from Lepton Triplets in the U(1)_Sigma Model
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• Reviewing the prospect of fermion triplets as dark matter and source of baryon asymmetry in non-standard cosmology
• Neutrino masses and mixing from milli-charged dark matter
• Dark matter as the source of neutrino mass: theory overview and experimental prospects
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• Flavor Symmetries in the Yukawa Sector of Non-Supersymmetric SO(10): Numerical Fits Using Renormalization Group Running
• Dark Matter and Lepton Flavour Violation in a Hybrid Neutrino Mass Model
• A common framework for fermion mass hierarchy, leptogenesis and dark matter
• Flavour anomalies and dark matter assisted unification in $SO(10)$ GUT
• Correlating neutrino magnetic moment and scalar triplet dark matter to enlighten XENONnT bounds in a Type-II model
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