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Common Origin of Neutrino Mass, Dark Matter, and Baryogenesis
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Combining one established idea with two recent ones, it is pointed out for the first time that three of the outstanding problems of particle physics and cosmology, i.e. neutrino mass, dark matter, and baryogenesis, may have a common solution, arising from the interactions of a single term, with experimentally verifiable consequences.
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Cited by 4 Pith papers
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Low-scale leptogenesis in the scotogenic model: spectator processes and benchmark points
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Inverse-seesaw U(1)_{B-L} model correlates leptogenesis, Majorana DM relic density, and neutrino masses with collider signatures in dilepton and single-lepton channels.
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Dark Matter and CP Violation in Some Symmetry-Constrained 3HDMs
S3-symmetric three-Higgs-doublet models allow dark matter in a 29-42 GeV window, exclude heavy candidates above 500 GeV, and admit MeV-scale light scalars, while continuous-symmetry variants produce mass-degenerate da...
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Baryogenesis in the paradigm of quintessential inflation
Quintessential inflation can generate the observed baryon asymmetry through a derivative coupling of the inflaton to a non-conserved baryon current, at the price of a carefully chosen cutoff scale.
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