Dirac gaugions, R symmetry and the 125 GeV Higgs
Autor(a) principal: | |
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Data de Publicação: | 2015 |
Outros Autores: | , , |
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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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 |
|
_version_ |
1808129494328803328 |