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Please use this identifier to cite or link to this item: http://acervodigital.unesp.br/handle/11449/67389
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dc.contributor.authorMagro, Mauricio Bernardino-
dc.contributor.authorDe Campos, Fernando-
dc.contributor.authorÉboli, Oscar J. P.-
dc.contributor.authorPorod, Werner-
dc.contributor.authorRestrepo, Diego-
dc.contributor.authorValle, José W. F.-
dc.date.accessioned2014-05-27T11:20:53Z-
dc.date.accessioned2016-10-25T18:18:50Z-
dc.date.available2014-05-27T11:20:53Z-
dc.date.available2016-10-25T18:18:50Z-
dc.date.issued2003-09-01-
dc.identifierhttp://dx.doi.org/10.1088/1126-6708/2003/09/071-
dc.identifier.citationJournal of High Energy Physics, v. 7, n. 9, p. 1687-1705, 2003.-
dc.identifier.issn1029-8479-
dc.identifier.urihttp://hdl.handle.net/11449/67389-
dc.identifier.urihttp://acervodigital.unesp.br/handle/11449/67389-
dc.description.abstractWe analyse the production of multileptons in the simplest supergravity model with bilinear violation of R parity at the Fermilab Tevatron. Despite the small .R-parity violating couplings needed to generate the neutrino masses indicated by current atmospheric neutrino data, the lightest supersymmetric particle is unstable and can decay inside the detector. This leads to a phenomenology quite distinct from that of the R-parity conserving scenario. We quantify by how much the supersymmetric multilepton signals differ from the R-parity conserving expectations, displaying our results in the m0 ⊙ m1/2 plane. We show that the presence of bilinear R-parity violating interactions enhances the supersymmetric multilepton signals over most of the parameter space, specially at moderate and large m0. © SISSA/ISAS 2003.en
dc.format.extent1687-1705-
dc.language.isoeng-
dc.sourceScopus-
dc.subjectBeyond Standard Model-
dc.subjectSolar and Atmospheric Neutrinos-
dc.subjectSupersymmetry Phenomenology-
dc.titleProbing neutrino mass with multilepton production at the Tevatron in the simplest R-parity violation modelen
dc.typeoutro-
dc.contributor.institutionUniversidade de São Paulo (USP)-
dc.contributor.institutionUniversidade Estadual Paulista (UNESP)-
dc.contributor.institutionUniversität Zürich-
dc.contributor.institutionUniversidad de Antioquia-
dc.contributor.institutionEdificio Institutos de Paterna-
dc.description.affiliationInstituto de Física Universidade de São Paulo, São Paulo, SP-
dc.description.affiliationDepartamento de Física e Química Universidade Estadual Paulista-
dc.description.affiliationInstitut für Theoretische Physik Universität Zürich, Zürich-
dc.description.affiliationInstituto de Física Universidad de Antioquia-
dc.description.affiliationInstituto de Física Corpuscular C.S.I.C. Edificio Institutos de Paterna, Apt 22085, E-46071 València-
dc.description.affiliationUnespDepartamento de Física e Química Universidade Estadual Paulista-
dc.identifier.doi10.1088/1126-6708/2003/09/071-
dc.identifier.wosWOS:000186766200071-
dc.rights.accessRightsAcesso restrito-
dc.relation.ispartofJournal of High Energy Physics-
dc.identifier.scopus2-s2.0-23144447257-
Appears in Collections:Artigos, TCCs, Teses e Dissertações da Unesp

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