Dirac gaugions, R symmetry and the 125 GeV Higgs

Detalhes bibliográficos
Autor(a) principal: Bertuzzo, Enrico
Data de Publicação: 2015
Outros Autores: Frugiuele, Claudia, Gregoire, Thomas, Ponton, Eduardo [UNESP]
Tipo de documento: Artigo
Idioma: eng
Título da fonte: Repositório Institucional da UNESP
Texto Completo: http://link.springer.com/article/10.1007%2FJHEP04%282015%29089
http://hdl.handle.net/11449/128946
Resumo: We 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.
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spelling Dirac gaugions, R symmetry and the 125 GeV HiggsHiggs PhysicsBeyond Standard ModelSupersymmetric Standard ModelWe 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.Agence National de la RechercheSpanish Ministry MICINNNatural Sciences and Engineering Research Council of Canada (NSERC)Fundação de Amparo à Pesquisa do Estado de São Paulo (FAPESP)Fermi Research Alliance, LLCUnited States Department of EnergyCEA Saclay, Inst Phys Theor, F-91191 Gif Sur Yvette, FranceUniv Autonoma Barcelona, IFAE, E-08193 Barcelona, SpainFermilab Natl Accelerator Lab, Batavia, IL 60510 USACarleton Univ, Ottawa Carleton Inst Phys, Dept Phys, Ottawa, ON K1S 5B6, CanadaUniv Estadual Paulista UNESP, ICTP, South Amer Inst Fundamental Res, BR-01140070 Sao Paulo, SP, BrazilUniv Estadual Paulista UNESP, Instituto de Física Teórica (IFT), BR-01140070 Sao Paulo, SP, BrazilUniv Estadual Paulista UNESP, ICTP, South Amer Inst Fundamental Res, BR-01140070 Sao Paulo, SP, BrazilUniv Estadual Paulista UNESP, Inst Fis Teor, BR-01140070 Sao Paulo, SP, BrazilAgence National de la Recherche: ANR 2010 BLANC 0413 01Spanish Ministry MICINN: FPA2010-17747FAPESP: 2011/11973Fermi Research Alliance, LLC: DE-AC02-07CH11359SpringerCEA SaclayUniv Autonoma BarcelonaFermilab Natl Accelerator LabCarleton UnivUniversidade Estadual Paulista (Unesp)Bertuzzo, EnricoFrugiuele, ClaudiaGregoire, ThomasPonton, Eduardo [UNESP]2015-10-21T17:03:34Z2015-10-21T17:03:34Z2015-04-20info:eu-repo/semantics/publishedVersioninfo:eu-repo/semantics/article1-22application/pdfhttp://link.springer.com/article/10.1007%2FJHEP04%282015%29089Journal Of High Energy Physics. New York: Springer, n. 4, p. 1-22, 2015.1029-8479http://hdl.handle.net/11449/12894610.1007/JHEP04(2015)089WOS:000353551800006WOS000353551800006.pdfWeb of Sciencereponame:Repositório Institucional da UNESPinstname:Universidade Estadual Paulista (UNESP)instacron:UNESPengJournal Of High Energy Physics5.5411,227info:eu-repo/semantics/openAccess2024-01-16T06:29:16Zoai:repositorio.unesp.br:11449/128946Repositório InstitucionalPUBhttp://repositorio.unesp.br/oai/requestopendoar:29462024-08-05T23:08:37.353600Repositório Institucional da UNESP - Universidade Estadual Paulista (UNESP)false
dc.title.none.fl_str_mv Dirac gaugions, R symmetry and the 125 GeV Higgs
title Dirac gaugions, R symmetry and the 125 GeV Higgs
spellingShingle Dirac gaugions, R symmetry and the 125 GeV Higgs
Bertuzzo, Enrico
Higgs Physics
Beyond Standard Model
Supersymmetric Standard Model
title_short Dirac gaugions, R symmetry and the 125 GeV Higgs
title_full Dirac gaugions, R symmetry and the 125 GeV Higgs
title_fullStr Dirac gaugions, R symmetry and the 125 GeV Higgs
title_full_unstemmed Dirac gaugions, R symmetry and the 125 GeV Higgs
title_sort Dirac gaugions, R symmetry and the 125 GeV Higgs
author Bertuzzo, Enrico
author_facet Bertuzzo, Enrico
Frugiuele, Claudia
Gregoire, Thomas
Ponton, Eduardo [UNESP]
author_role author
author2 Frugiuele, Claudia
Gregoire, Thomas
Ponton, Eduardo [UNESP]
author2_role author
author
author
dc.contributor.none.fl_str_mv CEA Saclay
Univ Autonoma Barcelona
Fermilab Natl Accelerator Lab
Carleton Univ
Universidade Estadual Paulista (Unesp)
dc.contributor.author.fl_str_mv Bertuzzo, Enrico
Frugiuele, Claudia
Gregoire, Thomas
Ponton, Eduardo [UNESP]
dc.subject.por.fl_str_mv Higgs Physics
Beyond Standard Model
Supersymmetric Standard Model
topic Higgs Physics
Beyond Standard Model
Supersymmetric Standard Model
description We 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.
publishDate 2015
dc.date.none.fl_str_mv 2015-10-21T17:03:34Z
2015-10-21T17:03:34Z
2015-04-20
dc.type.status.fl_str_mv info:eu-repo/semantics/publishedVersion
dc.type.driver.fl_str_mv info:eu-repo/semantics/article
format article
status_str publishedVersion
dc.identifier.uri.fl_str_mv http://link.springer.com/article/10.1007%2FJHEP04%282015%29089
Journal Of High Energy Physics. New York: Springer, n. 4, p. 1-22, 2015.
1029-8479
http://hdl.handle.net/11449/128946
10.1007/JHEP04(2015)089
WOS:000353551800006
WOS000353551800006.pdf
url http://link.springer.com/article/10.1007%2FJHEP04%282015%29089
http://hdl.handle.net/11449/128946
identifier_str_mv Journal Of High Energy Physics. New York: Springer, n. 4, p. 1-22, 2015.
1029-8479
10.1007/JHEP04(2015)089
WOS:000353551800006
WOS000353551800006.pdf
dc.language.iso.fl_str_mv eng
language eng
dc.relation.none.fl_str_mv Journal Of High Energy Physics
5.541
1,227
dc.rights.driver.fl_str_mv info:eu-repo/semantics/openAccess
eu_rights_str_mv openAccess
dc.format.none.fl_str_mv 1-22
application/pdf
dc.publisher.none.fl_str_mv Springer
publisher.none.fl_str_mv Springer
dc.source.none.fl_str_mv Web of Science
reponame:Repositório Institucional da UNESP
instname:Universidade Estadual Paulista (UNESP)
instacron:UNESP
instname_str Universidade Estadual Paulista (UNESP)
instacron_str UNESP
institution UNESP
reponame_str Repositório Institucional da UNESP
collection Repositório Institucional da UNESP
repository.name.fl_str_mv Repositório Institucional da UNESP - Universidade Estadual Paulista (UNESP)
repository.mail.fl_str_mv
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