Scalar contributions to oblique parameters in the 331RHN model yield an upper limit ω ≲ 10 TeV dominated by the T parameter.
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A dark matter fermion is shown to simultaneously explain the relic density, satisfy direct detection and collider bounds, and produce observable rates for muon-to-electron transitions in a viable parameter region.
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Scalar contributions from $331RHN$ minimal model to oblique parameters
Scalar contributions to oblique parameters in the 331RHN model yield an upper limit ω ≲ 10 TeV dominated by the T parameter.
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Dark Matter as a Source for Lepton Flavor Violation
A dark matter fermion is shown to simultaneously explain the relic density, satisfy direct detection and collider bounds, and produce observable rates for muon-to-electron transitions in a viable parameter region.