Future [Formula presented] Colliders’ Sensitivity to [Formula presented] Coupling and [Formula presented] Violation

Detalhes bibliográficos
Autor(a) principal: Braguta, V.
Data de Publicação: 2003
Outros Autores: Chalov, A., Likhoded, A. [UNESP], Rosenfeld, R. [UNESP]
Tipo de documento: Artigo
Idioma: eng
Título da fonte: Repositório Institucional da UNESP
Texto Completo: http://dx.doi.org/10.1103/PhysRevLett.90.241801
http://hdl.handle.net/11449/228476
Resumo: We perform a complete simulation of the process [Formula presented], where [Formula presented] can be an electron, muon, or tau neutrino, in the context of a general Higgs coupling to [Formula presented] quarks. We parametrize the [Formula presented] coupling as [Formula presented]. Taking into account interference effects between pure Higgs and Standard Model contributions, we find that sensitivities of the order of [Formula presented] and [Formula presented] can be obtained at a future [Formula presented] collider for deviations of the [Formula presented] and [Formula presented] parameters, respectively, from their Standard Model values. Combining our analysis with an independent measurement of [Formula presented] can provide evidence about the [Formula presented] nature of the Higgs sector. © 2003 The American Physical Society.
id UNSP_2b0653c85c4d2a48e1f905a8d53f97c8
oai_identifier_str oai:repositorio.unesp.br:11449/228476
network_acronym_str UNSP
network_name_str Repositório Institucional da UNESP
repository_id_str 2946
spelling Future [Formula presented] Colliders’ Sensitivity to [Formula presented] Coupling and [Formula presented] ViolationWe perform a complete simulation of the process [Formula presented], where [Formula presented] can be an electron, muon, or tau neutrino, in the context of a general Higgs coupling to [Formula presented] quarks. We parametrize the [Formula presented] coupling as [Formula presented]. Taking into account interference effects between pure Higgs and Standard Model contributions, we find that sensitivities of the order of [Formula presented] and [Formula presented] can be obtained at a future [Formula presented] collider for deviations of the [Formula presented] and [Formula presented] parameters, respectively, from their Standard Model values. Combining our analysis with an independent measurement of [Formula presented] can provide evidence about the [Formula presented] nature of the Higgs sector. © 2003 The American Physical Society.Institute of High Energy Physics, ProtvinoInstituto de Física Teórica–UNESP, Rua Pamplona 145, São Paulo, 01405-900Instituto de Física Teórica–UNESP, Rua Pamplona 145, São Paulo, 01405-900Institute of High Energy PhysicsUniversidade Estadual Paulista (UNESP)Braguta, V.Chalov, A.Likhoded, A. [UNESP]Rosenfeld, R. [UNESP]2022-04-29T08:26:55Z2022-04-29T08:26:55Z2003-01-01info:eu-repo/semantics/publishedVersioninfo:eu-repo/semantics/article3http://dx.doi.org/10.1103/PhysRevLett.90.241801Physical Review Letters, v. 90, n. 24, p. 3-, 2003.1079-71140031-9007http://hdl.handle.net/11449/22847610.1103/PhysRevLett.90.2418012-s2.0-85038339413Scopusreponame:Repositório Institucional da UNESPinstname:Universidade Estadual Paulista (UNESP)instacron:UNESPengPhysical Review Lettersinfo:eu-repo/semantics/openAccess2022-04-29T08:26:55Zoai:repositorio.unesp.br:11449/228476Repositório InstitucionalPUBhttp://repositorio.unesp.br/oai/requestopendoar:29462024-05-23T21:13:14.870843Repositório Institucional da UNESP - Universidade Estadual Paulista (UNESP)false
dc.title.none.fl_str_mv Future [Formula presented] Colliders’ Sensitivity to [Formula presented] Coupling and [Formula presented] Violation
title Future [Formula presented] Colliders’ Sensitivity to [Formula presented] Coupling and [Formula presented] Violation
spellingShingle Future [Formula presented] Colliders’ Sensitivity to [Formula presented] Coupling and [Formula presented] Violation
Braguta, V.
title_short Future [Formula presented] Colliders’ Sensitivity to [Formula presented] Coupling and [Formula presented] Violation
title_full Future [Formula presented] Colliders’ Sensitivity to [Formula presented] Coupling and [Formula presented] Violation
title_fullStr Future [Formula presented] Colliders’ Sensitivity to [Formula presented] Coupling and [Formula presented] Violation
title_full_unstemmed Future [Formula presented] Colliders’ Sensitivity to [Formula presented] Coupling and [Formula presented] Violation
title_sort Future [Formula presented] Colliders’ Sensitivity to [Formula presented] Coupling and [Formula presented] Violation
author Braguta, V.
author_facet Braguta, V.
Chalov, A.
Likhoded, A. [UNESP]
Rosenfeld, R. [UNESP]
author_role author
author2 Chalov, A.
Likhoded, A. [UNESP]
Rosenfeld, R. [UNESP]
author2_role author
author
author
dc.contributor.none.fl_str_mv Institute of High Energy Physics
Universidade Estadual Paulista (UNESP)
dc.contributor.author.fl_str_mv Braguta, V.
Chalov, A.
Likhoded, A. [UNESP]
Rosenfeld, R. [UNESP]
description We perform a complete simulation of the process [Formula presented], where [Formula presented] can be an electron, muon, or tau neutrino, in the context of a general Higgs coupling to [Formula presented] quarks. We parametrize the [Formula presented] coupling as [Formula presented]. Taking into account interference effects between pure Higgs and Standard Model contributions, we find that sensitivities of the order of [Formula presented] and [Formula presented] can be obtained at a future [Formula presented] collider for deviations of the [Formula presented] and [Formula presented] parameters, respectively, from their Standard Model values. Combining our analysis with an independent measurement of [Formula presented] can provide evidence about the [Formula presented] nature of the Higgs sector. © 2003 The American Physical Society.
publishDate 2003
dc.date.none.fl_str_mv 2003-01-01
2022-04-29T08:26:55Z
2022-04-29T08:26:55Z
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://dx.doi.org/10.1103/PhysRevLett.90.241801
Physical Review Letters, v. 90, n. 24, p. 3-, 2003.
1079-7114
0031-9007
http://hdl.handle.net/11449/228476
10.1103/PhysRevLett.90.241801
2-s2.0-85038339413
url http://dx.doi.org/10.1103/PhysRevLett.90.241801
http://hdl.handle.net/11449/228476
identifier_str_mv Physical Review Letters, v. 90, n. 24, p. 3-, 2003.
1079-7114
0031-9007
10.1103/PhysRevLett.90.241801
2-s2.0-85038339413
dc.language.iso.fl_str_mv eng
language eng
dc.relation.none.fl_str_mv Physical Review Letters
dc.rights.driver.fl_str_mv info:eu-repo/semantics/openAccess
eu_rights_str_mv openAccess
dc.format.none.fl_str_mv 3
dc.source.none.fl_str_mv Scopus
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_ 1803045727622922240

Registros relacionados