Logotipo do repositório
 

Publicação:
Linking natural supersymmetry to flavour physics

dc.contributor.authorDudas, Emilian
dc.contributor.authorVon Gersdorff, Gero [UNESP]
dc.contributor.authorPokorski, Stefan
dc.contributor.authorZiegler, Robert
dc.contributor.institutionCNRS
dc.contributor.institutionUniversidade Estadual Paulista (UNESP)
dc.contributor.institutionUniversity of Warsaw
dc.contributor.institutionTechnische Universität München
dc.date.accessioned2022-04-29T07:13:53Z
dc.date.available2022-04-29T07:13:53Z
dc.date.issued2014-01-01
dc.description.abstractWith the aim of linking natural supersymmetry to flavour physics, a model is proposed based on a family symmetry G × U(1), where G is a discrete nonabelian subgroup of SU(2), with both F-term and (abelian) D-term supersymmetry breaking. A good fit to the fermion masses and mixing is obtained with the same U(1) charges for the left- and right- handed quarks of the first two families and the right-handed bottom quark, and with zero charge for the left-handed top-bottom doublet and the the right handed top. The model shows an interesting indirect correlation between the correct prediction for the V ub/Vcb ratio and large right-handed rotations in the (s, b) sector, required to diagonalise the Yukawa matrix. For the squarks, one obtains almost degenerate first two generations. The main source of the FCNC and CP violation effects is the splitting between the first two families and the right-handed sbottom determined by the relative size of F-term and D-term supersymmetry breaking. The presence of the large right-handed rotation implies that the bounds on the masses of the first two families of squarks and the right handed sbottom are in a few to a few tens TeV range. The picture that emerges is light stops and left handed sbottom and much heavier other squarks. © 2014 The Author(s).en
dc.description.affiliationCentre de Physique Théorique École Polytechnique CNRS, Palaiseau
dc.description.affiliationICTP South American Institute for Fundamental Research Instituto de Fisica Teorica Sao Paulo State University, Sao Paulo
dc.description.affiliationInstitute of Theoretical Physics Faculty of Physics University of Warsaw, Warsaw
dc.description.affiliationTUM-IAS and Physik Department Technische Universität München, Munich
dc.description.affiliationUnespICTP South American Institute for Fundamental Research Instituto de Fisica Teorica Sao Paulo State University, Sao Paulo
dc.identifierhttp://dx.doi.org/10.1007/JHEP01(2014)117
dc.identifier.citationJournal of High Energy Physics, v. 2014, n. 1, 2014.
dc.identifier.doi10.1007/JHEP01(2014)117
dc.identifier.issn1126-6708
dc.identifier.issn1029-8479
dc.identifier.scopus2-s2.0-84893858369
dc.identifier.urihttp://hdl.handle.net/11449/227555
dc.language.isoeng
dc.relation.ispartofJournal of High Energy Physics
dc.sourceScopus
dc.subjectQuark Masses and SM Parameters
dc.subjectSupersymmetric Standard Model
dc.subjectSupersymmetry Breaking
dc.titleLinking natural supersymmetry to flavour physicsen
dc.typeArtigo
dspace.entity.typePublication
unesp.campusUniversidade Estadual Paulista (UNESP), Instituto de Física Teórica (IFT), São Paulopt

Arquivos