Future [Formula presented] Colliders’ Sensitivity to [Formula presented] Coupling and [Formula presented] Violation
Autor(a) principal: | |
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Data de Publicação: | 2003 |
Outros Autores: | , , |
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. |
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Repositório Institucional da UNESP |
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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:29462024-08-05T23:29:24.530321Repositório 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_ |
1808129525094023168 |