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dc.contributor.authorMira Martínez, Jesús María-
dc.contributor.authorNardi, Enrico-
dc.contributor.authorRestrepo Quintero, Diego Alejandro-
dc.contributor.authorValle, José W. F.-
dc.date.accessioned2017-09-28T16:35:16Z-
dc.date.available2017-09-28T16:35:16Z-
dc.date.issued2000-
dc.identifier.citationMira, J. M., Nardi, E., Restrepo Quintero, D. A., & Valle, J. W. F. (2000). Bilinear R-parity violation and small neutrino masses: a self-consistent framework. Physics Letters B. 492, 81-90.spa
dc.identifier.issn0370-2693-
dc.identifier.urihttp://hdl.handle.net/10495/8393-
dc.description.abstractABSTRACT: We study extensions of supersymmetric models without R-parity which include an anomalous U.1/H horizontal symmetry. Bilinear R-parity violating terms induce a neutrino mass at tree level mvtree ~~ (tetha2)& eV where tetha ~_ 0.22 is the U(1)H breaking parameter and & is an integer number that depends on the horizontal charges of the leptons. For &=1 a unique self-consistent model arises in which (i) all the superpotential trilinear R-parity violating couplings are forbidden by holomorphy; (ii) mvtree falls in the range suggested by the atmospheric neutrino problem; (iii) radiative contributions to neutrino masses are strongly suppressed resulting in m2 solar ~~ fe 10^8 eV2 which only allows for the LOW (or quasi-vacuum) solution to the solar neutrino problem; (iv) the neutrino mixing angles are not suppressed by powers of tetha and can naturally be large.spa
dc.format.mimetypeapplication/pdfspa
dc.language.isoengspa
dc.publisherElsevierspa
dc.type.hasversioninfo:eu-repo/semantics/publishedVersionspa
dc.rightsAtribución-CompartirIgual 2.5 Colombia (CC BY-SA 2.5 CO)*
dc.rightsinfo:eu-repo/semantics/openAccessspa
dc.rights.urihttp://creativecommons.org/licenses/by-sa/2.5/co/*
dc.titleBilinear R-parity violation and small neutrino masses : a self-consistent frameworkspa
dc.typeinfo:eu-repo/semantics/articlespa
dc.publisher.groupGrupo de Fenomenologia de Interacciones Fundamentalesspa
oaire.versionhttp://purl.org/coar/version/c_970fb48d4fbd8a85spa
dc.rights.accessrightshttp://purl.org/coar/access_right/c_abf2spa
dc.identifier.eissn1873-2445-
oaire.citationtitleSemiconductor Science and Technology Particle Physics, Nuclear Physics and Cosmologyspa
oaire.citationstartpage81spa
oaire.citationendpage90spa
oaire.citationvolume492spa
dc.rights.creativecommonshttps://creativecommons.org/licenses/by-sa/4.0/spa
dc.type.coarhttp://purl.org/coar/resource_type/c_2df8fbb1spa
dc.type.redcolhttps://purl.org/redcol/resource_type/ARTspa
dc.type.localArtículo de investigaciónspa
dc.subject.lembNeutrinos-
dc.subject.lembNeutrines-
dc.subject.lembSimetría-
dc.subject.lembSymmetry-
dc.subject.lembCargas-
dc.subject.lembFreight-
dc.subject.lembDominios de holomorfía-
dc.subject.lembDomains of holomorphy-
dc.subject.lembNeutrinos solares-
dc.subject.lembSolar neutrinos-
dc.subject.agrovocAtmósfera-
dc.subject.agrovocAtmosphere-
dc.subject.proposalMasas de neutrinosspa
dc.subject.proposalCargas de leptonesspa
dc.subject.agrovocurihttp://aims.fao.org/aos/agrovoc/c_8994-
dc.description.researchgroupidCOL0008423spa
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