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dc.contributor.authorÁguila Giménez, Francisco Del 
dc.contributor.authorAparici, Alberto
dc.contributor.authorBhattacharya, S.
dc.contributor.authorSantamaria, Arcadi
dc.contributor.authorWudka, Jose
dc.date.accessioned2014-03-06T13:06:48Z
dc.date.available2014-03-06T13:06:48Z
dc.date.issued2012
dc.identifier.citationÁguila, F.; et al. A realistic model of neutrino masses with a large neutrinoless double beta decay rate. Journal of High Energy Physics, 2012: 133 (2012). [http://hdl.handle.net/10481/30718]es_ES
dc.identifier.issn1029-8479
dc.identifier.otherdoi: 10.1007/JHEP05(2012)133
dc.identifier.otherarXiv:1111.6960v3
dc.identifier.urihttp://hdl.handle.net/10481/30718
dc.description.abstractThe minimal Standard Model extension with the Weinberg operator does accommodate the observed neutrino masses and mixing, but predicts a neutrinoless double beta (0νββ) decay rate proportional to the effective electron neutrino mass, which can be then arbitrarily small within present experimental limits. However, in general 0νββ decay can have an independent origin and be near its present experimental bound; whereas neutrino masses are generated radiatively, contributing negligibly to 0νββ decay. We provide a realization of this scenario in a simple, well defined and testable model, with potential LHC effects and calculable neutrino masses, whose two-loop expression we derive exactly. We also discuss the connection of this model to others that have appeared in the literature, and remark on the significant differences that result from various choices of quantum number assignments and symmetry assumptions. In this type of models lepton flavor violating rates are also preferred to be relatively large, at the reach of foreseen experiments. Interestingly enough, in our model this stands for a large third mixing angle, sin2θ13>∼0.008 , when μ→eee is required to lie below its present experimental limit.es_ES
dc.description.sponsorshipThis work has been supported in part by the Ministry of Science and Innovation (MICINN) Spain, under the grant numbers FPA2006-05294, FPA2008-03373, FPA2010- 17915 and FPA2011-23897, by the Junta de Andalucía grants FQM 101, FQM 03048 and FQM 6552, by the “Generalitat Valenciana” grant PROMETEO/2009/128 and by the U.S. Department of Energy grant No. DE-FG03-94ER40837. A.A. is supported by the MICINN under the FPU program.es_ES
dc.language.isoenges_ES
dc.publisherScuola Internazionale Superiore di Studi Avanzati (SISSA)es_ES
dc.rightsCreative Commons Attribution-NonCommercial-NoDerivs 3.0 Licensees_ES
dc.rights.urihttp://creativecommons.org/licenses/by-nc-nd/3.0/es_ES
dc.subjectNeutrino physicses_ES
dc.subjectHiggs Physicses_ES
dc.subjectBeyond Standard Modeles_ES
dc.titleA realistic model of neutrino masses with a large neutrinoless double beta decay ratees_ES
dc.typeinfo:eu-repo/semantics/articlees_ES
dc.rights.accessRightsinfo:eu-repo/semantics/openAccesses_ES


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