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Please use this identifier to cite or link to this item: http://acervodigital.unesp.br/handle/11449/128946
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dc.contributor.authorBertuzzo, Enrico-
dc.contributor.authorFrugiuele, Claudia-
dc.contributor.authorGregoire, Thomas-
dc.contributor.authorPonton, Eduardo-
dc.date.accessioned2015-10-21T17:03:34Z-
dc.date.accessioned2016-10-25T21:07:19Z-
dc.date.available2015-10-21T17:03:34Z-
dc.date.available2016-10-25T21:07:19Z-
dc.date.issued2015-04-20-
dc.identifierhttp://link.springer.com/article/10.1007%2FJHEP04%282015%29089-
dc.identifier.citationJournal Of High Energy Physics. New York: Springer, n. 4, p. 1-22, 2015.-
dc.identifier.issn1029-8479-
dc.identifier.urihttp://hdl.handle.net/11449/128946-
dc.identifier.urihttp://acervodigital.unesp.br/handle/11449/128946-
dc.description.abstractWe study a supersymmetric scenario with a quasi exact R-symmetry in light of the discovery of a Higgs resonance with a mass of 125 GeV. In such a framework, the additional adjoint superfields, needed to give Dirac masses to the gauginos, contribute both to the Higgs mass and to electroweak precision observables. We analyze the interplay between the two aspects, finding regions in parameter space in which the contributions to the precision observables are under control and a 125 GeV Higgs boson can be accommodated. We estimate the fine-tuning of the model finding regions of the parameter space still unexplored by the LHC with a fine-tuning considerably improved with respect to the minimal supersymmetric scenario. In particular, sizable non-holomorphic (non-supersoft) adjoints masses are required to reduce the fine-tuning.en
dc.description.sponsorshipAgence National de la Recherche-
dc.description.sponsorshipSpanish Ministry MICINN-
dc.description.sponsorshipNatural Sciences and Engineering Research Council of Canada (NSERC)-
dc.description.sponsorshipFundação de Amparo à Pesquisa do Estado de São Paulo (FAPESP)-
dc.description.sponsorshipFermi Research Alliance, LLC-
dc.description.sponsorshipUnited States Department of Energy-
dc.format.extent1-22-
dc.language.isoeng-
dc.publisherSpringer-
dc.sourceWeb of Science-
dc.subjectHiggs Physicsen
dc.subjectBeyond Standard Modelen
dc.subjectSupersymmetric Standard Modelen
dc.titleDirac gaugions, R symmetry and the 125 GeV Higgsen
dc.typeoutro-
dc.contributor.institutionCEA Saclay-
dc.contributor.institutionUniv Autonoma Barcelona-
dc.contributor.institutionFermilab Natl Accelerator Lab-
dc.contributor.institutionCarleton Univ-
dc.contributor.institutionUniversidade Estadual Paulista (UNESP)-
dc.description.affiliationCEA Saclay, Inst Phys Theor, F-91191 Gif Sur Yvette, France-
dc.description.affiliationUniv Autonoma Barcelona, IFAE, E-08193 Barcelona, Spain-
dc.description.affiliationFermilab Natl Accelerator Lab, Batavia, IL 60510 USA-
dc.description.affiliationCarleton Univ, Ottawa Carleton Inst Phys, Dept Phys, Ottawa, ON K1S 5B6, Canada-
dc.description.affiliationUniv Estadual Paulista UNESP, ICTP, South Amer Inst Fundamental Res, BR-01140070 Sao Paulo, SP, Brazil-
dc.description.affiliationUniv Estadual Paulista UNESP, Instituto de Física Teórica (IFT), BR-01140070 Sao Paulo, SP, Brazil-
dc.description.affiliationUnespUniv Estadual Paulista UNESP, ICTP, South Amer Inst Fundamental Res, BR-01140070 Sao Paulo, SP, Brazil-
dc.description.affiliationUnespUniv Estadual Paulista UNESP, Inst Fis Teor, BR-01140070 Sao Paulo, SP, Brazil-
dc.description.sponsorshipIdAgence National de la Recherche: ANR 2010 BLANC 0413 01-
dc.description.sponsorshipIdSpanish Ministry MICINN: FPA2010-17747-
dc.description.sponsorshipIdFAPESP: 2011/11973-
dc.description.sponsorshipIdFermi Research Alliance, LLC: DE-AC02-07CH11359-
dc.identifier.doihttp://dx.doi.org/10.1007/JHEP04(2015)089-
dc.identifier.wosWOS:000353551800006-
dc.rights.accessRightsAcesso aberto-
dc.identifier.fileWOS000353551800006.pdf-
dc.relation.ispartofJournal Of High Energy Physics-
Appears in Collections:Artigos, TCCs, Teses e Dissertações da Unesp

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