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Predictive discrete dark matter model and neutrino oscillations

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Predictive discrete dark matter model and neutrino oscillations

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dc.contributor.author Boucenna, Mohamed Sofiane
dc.contributor.author Morisi, S.
dc.contributor.author Peinado Rodríguez, Eduardo
dc.contributor.author Furtado Valle, José Wagner
dc.contributor.author Shimizu, Yusuke
dc.date.accessioned 2015-09-28T08:15:39Z
dc.date.available 2015-09-28T08:15:39Z
dc.date.issued 2012
dc.identifier.citation Boucenna, Mohamed Sofiane Morisi, S. Peinado Rodríguez, Eduardo Furtado Valle, José Wagner Shimizu, Yusuke 2012 Predictive discrete dark matter model and neutrino oscillations Physical Review D 86 7 073008
dc.identifier.uri http://hdl.handle.net/10550/47315
dc.description.abstract Dark Matter stability can be achieved through a partial breaking of a flavor symmetry. In this framework we propose a type-II seesaw model where left-handed matter transforms nontrivially under the flavor group Delta(54), providing correlations between neutrino oscillation parameters, consistent with the recent Daya-Bay and RENO reactor angle measurements, as well as lower bounds for neutrinoless double beta decay. The dark matter phenomenology is provided by a Higgs-portal.
dc.language.iso eng
dc.relation.ispartof Physical Review D, 2012, vol. 86, num. 7, p. 073008
dc.subject Física
dc.title Predictive discrete dark matter model and neutrino oscillations
dc.type journal article es_ES
dc.date.updated 2015-09-28T08:15:39Z
dc.identifier.doi 10.1103/PhysRevD.86.073008
dc.identifier.idgrec 084323
dc.rights.accessRights open access es_ES

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