Por favor, use este identificador para citar o enlazar este ítem: https://hdl.handle.net/10495/9338
Registro completo de metadatos
Campo DC Valor Lengua/Idioma
dc.contributor.authorFilippi, Simoneta-
dc.contributor.authorPonce Gutiérrez, William Antonio-
dc.contributor.authorSánchez Duque, Luis Alberto-
dc.date.accessioned2018-04-06T19:15:50Z-
dc.date.available2018-04-06T19:15:50Z-
dc.date.issued2006-
dc.identifier.citationFilippi, S., Ponce Gutiérrez, W. A., & Sánchez, L. A. (2006). Dark matter from the scalar sector of 3-3-1 models without exotic electric charges. Europhysics Letters, 73(1), 142-148. DOI: 10.1209/epl/i2005-10349-xspa
dc.identifier.issn0295-5075-
dc.identifier.urihttp://hdl.handle.net/10495/9338-
dc.description.abstractABSTRACT: It is shown that three SU(2) singlet neutral scalars (two CP-even and one CP-odd) in the spectrum of models based on the gauge symmetry SU(3)c ⊗ SU(3)L ⊗ U(1)X, which do not contain exotic electric charges, are realistic candidates for thermally generated self-interacting dark matter in the Universe, a type of dark matter that has been recently proposed in order to overcome some difficulties of collisionless cold-dark-matter models at the galactic scale. These candidates arise without introducing a new mass scale in the model and/or without the need for a discrete symmetry to stabilize them, but at the expense of tuning several combinations of parameters of the scalar potential.spa
dc.format.mimetypeapplication/pdfspa
dc.language.isoengspa
dc.publisherEuropean Physical Societyspa
dc.type.hasversioninfo:eu-repo/semantics/publishedVersionspa
dc.rightsAtribución-NoComercial-SinDerivadas 2.5 Colombia*
dc.rightsinfo:eu-repo/semantics/openAccessspa
dc.rights.urihttp://creativecommons.org/licenses/by-nc-nd/2.5/co/*
dc.titleDark matter from the scalar sector of 3-3-1 models without exotic electric chargesspa
dc.typeinfo:eu-repo/semantics/articlespa
dc.publisher.groupGrupo de Fenomenologia de Interacciones Fundamentalesspa
dc.identifier.doi10.1209/epl/i2005-10349-x-
oaire.versionhttp://purl.org/coar/version/c_970fb48d4fbd8a85spa
dc.rights.accessrightshttp://purl.org/coar/access_right/c_abf2spa
dc.identifier.eissn0302-072X-
oaire.citationtitleEurophysics Lettersspa
oaire.citationstartpage142spa
oaire.citationendpage148spa
oaire.citationvolume73spa
oaire.citationissue1spa
dc.rights.creativecommonshttps://creativecommons.org/licenses/by-nc-nd/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.unescoUniverso-
dc.subject.unescoUniverse-
dc.subject.unescoGalaxia-
dc.subject.unescoGalaxies-
dc.subject.lembSimetría (Física)-
dc.subject.lembSymmetry (physics)-
dc.subject.lembNúcleos galácticos-
dc.subject.lembGalactic nuclei-
dc.subject.proposalMateria oscura (Astronomía)spa
dc.subject.proposalColisiones galácticasspa
dc.subject.unescourihttp://vocabularies.unesco.org/thesaurus/concept3230-
dc.subject.unescourihttp://vocabularies.unesco.org/thesaurus/concept3226-
dc.relation.ispartofjournalabbrevEurophys. Lett.spa
Aparece en las colecciones: Artículos de Revista en Ciencias Exactas y Naturales

Ficheros en este ítem:
Fichero Descripción Tamaño Formato  
PonceWilliam_2006_DarkMatterScalar.pdfArtículo de investigación143.69 kBAdobe PDFVisualizar/Abrir


Este ítem está sujeto a una licencia Creative Commons Licencia Creative Commons Creative Commons