Trimuon production at the LHC
Autor(a) principal: | |
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Data de Publicação: | 2020 |
Outros Autores: | |
Tipo de documento: | Artigo |
Idioma: | eng |
Título da fonte: | Repositório Institucional da UNESP |
Texto Completo: | http://dx.doi.org/10.1103/PhysRevD.101.015024 http://hdl.handle.net/11449/228767 |
Resumo: | No process without a standard model (SM) background has been observed so far. As a tool in the study of a class of models containing doubly charged vector bileptons, we propose one such process that, violating lepton flavor number conservation, has no contribution from the SM: pp→μ+μ+μ-e-. By carefully isolating the parameters to keep them free, we are able to acquire a notion of how a possible PMNS-like matrix present in the relevant charged current parametrization could affect the observables. We find that an interesting section of the space of parameters can be explored at the current LHC in the specified conditions. |
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Repositório Institucional da UNESP |
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Trimuon production at the LHCNo process without a standard model (SM) background has been observed so far. As a tool in the study of a class of models containing doubly charged vector bileptons, we propose one such process that, violating lepton flavor number conservation, has no contribution from the SM: pp→μ+μ+μ-e-. By carefully isolating the parameters to keep them free, we are able to acquire a notion of how a possible PMNS-like matrix present in the relevant charged current parametrization could affect the observables. We find that an interesting section of the space of parameters can be explored at the current LHC in the specified conditions.Instituto de Física Teórica Universidade Estadual Paulista, R. Dr. Bento Teobaldo Ferraz 271Instituto de Física Teórica Universidade Estadual Paulista, R. Dr. Bento Teobaldo Ferraz 271Universidade Estadual Paulista (UNESP)Barela, Mario W. [UNESP]Pleitez, V. [UNESP]2022-04-29T08:28:33Z2022-04-29T08:28:33Z2020-01-28info:eu-repo/semantics/publishedVersioninfo:eu-repo/semantics/articlehttp://dx.doi.org/10.1103/PhysRevD.101.015024Physical Review D, v. 101, n. 1, 2020.2470-00292470-0010http://hdl.handle.net/11449/22876710.1103/PhysRevD.101.0150242-s2.0-85078544794Scopusreponame:Repositório Institucional da UNESPinstname:Universidade Estadual Paulista (UNESP)instacron:UNESPengPhysical Review Dinfo:eu-repo/semantics/openAccess2022-04-29T08:28:33Zoai:repositorio.unesp.br:11449/228767Repositório InstitucionalPUBhttp://repositorio.unesp.br/oai/requestopendoar:29462024-08-06T00:01:23.635558Repositório Institucional da UNESP - Universidade Estadual Paulista (UNESP)false |
dc.title.none.fl_str_mv |
Trimuon production at the LHC |
title |
Trimuon production at the LHC |
spellingShingle |
Trimuon production at the LHC Barela, Mario W. [UNESP] |
title_short |
Trimuon production at the LHC |
title_full |
Trimuon production at the LHC |
title_fullStr |
Trimuon production at the LHC |
title_full_unstemmed |
Trimuon production at the LHC |
title_sort |
Trimuon production at the LHC |
author |
Barela, Mario W. [UNESP] |
author_facet |
Barela, Mario W. [UNESP] Pleitez, V. [UNESP] |
author_role |
author |
author2 |
Pleitez, V. [UNESP] |
author2_role |
author |
dc.contributor.none.fl_str_mv |
Universidade Estadual Paulista (UNESP) |
dc.contributor.author.fl_str_mv |
Barela, Mario W. [UNESP] Pleitez, V. [UNESP] |
description |
No process without a standard model (SM) background has been observed so far. As a tool in the study of a class of models containing doubly charged vector bileptons, we propose one such process that, violating lepton flavor number conservation, has no contribution from the SM: pp→μ+μ+μ-e-. By carefully isolating the parameters to keep them free, we are able to acquire a notion of how a possible PMNS-like matrix present in the relevant charged current parametrization could affect the observables. We find that an interesting section of the space of parameters can be explored at the current LHC in the specified conditions. |
publishDate |
2020 |
dc.date.none.fl_str_mv |
2020-01-28 2022-04-29T08:28:33Z 2022-04-29T08:28:33Z |
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/PhysRevD.101.015024 Physical Review D, v. 101, n. 1, 2020. 2470-0029 2470-0010 http://hdl.handle.net/11449/228767 10.1103/PhysRevD.101.015024 2-s2.0-85078544794 |
url |
http://dx.doi.org/10.1103/PhysRevD.101.015024 http://hdl.handle.net/11449/228767 |
identifier_str_mv |
Physical Review D, v. 101, n. 1, 2020. 2470-0029 2470-0010 10.1103/PhysRevD.101.015024 2-s2.0-85078544794 |
dc.language.iso.fl_str_mv |
eng |
language |
eng |
dc.relation.none.fl_str_mv |
Physical Review D |
dc.rights.driver.fl_str_mv |
info:eu-repo/semantics/openAccess |
eu_rights_str_mv |
openAccess |
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_ |
1808129573537185792 |