Neutrino mass, Dark Matter and Baryon Asymmetry via TeV-Scale Physics without Fine-Tuning

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dc.creatorAoki, Mayumi
dc.creatorKanemura, Shinya
dc.creatorSeto, Osamu
dc.date2008-07-02
dc.date2009-01-07
dc.date.accessioned2026-07-07T12:46:55Z
dc.date.available2026-07-07T12:46:55Z
dc.descriptionWe propose an extended version of the standard model, in which neutrino oscillation, dark matter, and baryon asymmetry of the Universe can be simultaneously explained by the TeV-scale physics without assuming unnatural hierarchy among the mass scales. Tiny neutrino masses are generated at the three loop level due to the exact $Z_2$ symmetry, by which stability of the dark matter candidate is guaranteed. The extra Higgs doublet is required not only for the tiny neutrino masses but also for successful electroweak baryogenesis. The model provides discriminative predictions especially in Higgs phenomenology, so that it is testable at current and future collider experiments.
dc.description4 pages including 3 figures; version with revised figures
dc.identifierhttps://arxiv.org/abs/0807.0361
dc.identifierhttp://arxiv.org/abs/0807.0361
dc.identifierPhys.Rev.Lett.102:051805,2009
dc.identifierdoi:10.1103/PhysRevLett.102.051805
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/221544
dc.subjectHigh Energy Physics - Phenomenology
dc.titleNeutrino mass, Dark Matter and Baryon Asymmetry via TeV-Scale Physics without Fine-Tuning
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