A TeV-scale model for neutrino mass, DM and baryon asymmetry

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dc.creatorAoki, Mayumi
dc.creatorKanemura, Shinya
dc.creatorSeto, Osamu
dc.date2009-01-07
dc.date.accessioned2026-07-07T12:27:11Z
dc.date.available2026-07-07T12:27:11Z
dc.descriptionWe discuss a model which would explain neutrino oscillation, dark matter, and baryon asymmetry of the Universe simultaneously by the physics at TeV scales. Tiny neutrino masses are generated at the three loop level due to the exact $Z_2$ symmetry, by which the stability of the dark matter candidate is also guaranteed. The extra Higgs doublet is required not only for the tiny neutrino masses but also for successful electroweak baryogenesis. The model provides various discriminative predictions especially in charged Higgs phenomenology.
dc.description6 pages, 3 figures, Proceedings of "Prospects for Charged Higgs Discovery at Colliders (Charged 2008)", 16-19 Sep. 2008, Uppsala University, Sweden
dc.identifierhttps://arxiv.org/abs/0901.0849
dc.identifierhttp://arxiv.org/abs/0901.0849
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/215120
dc.subjectHigh Energy Physics - Phenomenology
dc.titleA TeV-scale model for neutrino mass, DM and baryon asymmetry
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