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Aidnogenesis via Leptogenesis and Dark Sphalerons

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Aidnogenesis via Leptogenesis and Dark Sphalerons

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dc.contributor.author Blennow, Mattias
dc.contributor.author Dasgupta, Basudeb
dc.contributor.author Fernández Martínez, Enrique
dc.contributor.author Rius Dionis, Nuria
dc.date.accessioned 2015-03-03T08:20:43Z
dc.date.available 2015-03-03T08:20:43Z
dc.date.issued 2011
dc.identifier.citation Blennow, Mattias Dasgupta, Basudeb Fernández Martínez, Enrique Rius Dionis, Nuria 2011 Aidnogenesis via Leptogenesis and Dark Sphalerons Journal of High Energy Physics 2011 3 014
dc.identifier.uri http://hdl.handle.net/10550/42571
dc.description.abstract We discuss aidnogenesis,(1) i.e. the generation of a dark matter asymmetry, via new sphaleron processes associated to an extra non-abelian gauge symmetry common to both the visible and the dark sectors. Such a theory can naturally produce an abundance of asymmetric dark matter which is of the same size as the lepton and baryon asymmetries, as suggested by the similar sizes of the observed baryonic and dark matter energy content, and provide a definite prediction for the mass of the dark matter particle. We discuss in detail a minimal realization in which the Standard Model is only extended by dark matter fermions which form 'dark baryons' through an SU(3) interaction, and a (broken) horizontal symmetry that induces the new sphalerons. The dark matter mass is predicted to be similar to 6GeV, close to the region favored by DAMA and CoGeNT. Furthermore, a remnant of the horizontal symmetry should be broken at a lower scale and can also explain the Tevatron dimuon anomaly.
dc.language.iso eng
dc.relation.ispartof Journal of High Energy Physics, 2011, vol. 2011, num. 3, p. 014
dc.subject Física
dc.title Aidnogenesis via Leptogenesis and Dark Sphalerons
dc.type journal article es_ES
dc.date.updated 2015-03-03T08:20:44Z
dc.identifier.doi 10.1007/JHEP03(2011)014
dc.identifier.idgrec 063280
dc.rights.accessRights open access es_ES

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