Perturbative corrections to technicolor

Detalhes bibliográficos
Autor(a) principal: Aguilar, A. C.
Data de Publicação: 2018
Outros Autores: Doff, A. [UNESP], Natale, A. A. [UNESP]
Tipo de documento: Artigo
Idioma: eng
Título da fonte: Repositório Institucional da UNESP
Texto Completo: http://dx.doi.org/10.1103/PhysRevD.97.115035
http://hdl.handle.net/11449/176575
Resumo: The full solution of technicolor (TC) Schwinger-Dyson equations should include radiative corrections induced by extended technicolor (ETC) (or other) interactions. We verify that when TC is embedded into a larger theory including also QCD, these radiative corrections couple the different strongly interacting Schwinger-Dyson equations, providing a tiny mass to technifermions and changing the ultraviolet behavior of the gap equation solution. We argue about the origin of the different quark masses without appealing for different ETC boson masses, in one scenario where most of the new physics will appear in interactions with the third fermion generation and with a TC scalar boson possibly lighter than the TC characteristic scale (ΛTC).
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spelling Perturbative corrections to technicolorThe full solution of technicolor (TC) Schwinger-Dyson equations should include radiative corrections induced by extended technicolor (ETC) (or other) interactions. We verify that when TC is embedded into a larger theory including also QCD, these radiative corrections couple the different strongly interacting Schwinger-Dyson equations, providing a tiny mass to technifermions and changing the ultraviolet behavior of the gap equation solution. We argue about the origin of the different quark masses without appealing for different ETC boson masses, in one scenario where most of the new physics will appear in interactions with the third fermion generation and with a TC scalar boson possibly lighter than the TC characteristic scale (ΛTC).University of Campinas - UNICAMP Institute of Physics Gleb WataghinUniversidade Tecnológica Federal Do Paraná - UTFPR - DAFIS, Avenida Monteiro Lobato Km 04Instituto de Física Teórica - UNESP, Rua Dr. Bento T. Ferraz, 271, Bloco IIInstituto de Física Teórica - UNESP, Rua Dr. Bento T. Ferraz, 271, Bloco IIUniversidade Estadual de Campinas (UNICAMP)Universidade Tecnológica Federal Do Paraná - UTFPR - DAFISUniversidade Estadual Paulista (Unesp)Aguilar, A. C.Doff, A. [UNESP]Natale, A. A. [UNESP]2018-12-11T17:21:25Z2018-12-11T17:21:25Z2018-06-20info:eu-repo/semantics/publishedVersioninfo:eu-repo/semantics/articlehttp://dx.doi.org/10.1103/PhysRevD.97.115035Physical Review D, v. 97, n. 11, 2018.2470-00292470-0010http://hdl.handle.net/11449/17657510.1103/PhysRevD.97.1150352-s2.0-85049744503Scopusreponame:Repositório Institucional da UNESPinstname:Universidade Estadual Paulista (UNESP)instacron:UNESPengPhysical Review D1,8011,801info:eu-repo/semantics/openAccess2021-10-23T15:08:33Zoai:repositorio.unesp.br:11449/176575Repositório InstitucionalPUBhttp://repositorio.unesp.br/oai/requestopendoar:29462024-08-05T23:03:02.662468Repositório Institucional da UNESP - Universidade Estadual Paulista (UNESP)false
dc.title.none.fl_str_mv Perturbative corrections to technicolor
title Perturbative corrections to technicolor
spellingShingle Perturbative corrections to technicolor
Aguilar, A. C.
title_short Perturbative corrections to technicolor
title_full Perturbative corrections to technicolor
title_fullStr Perturbative corrections to technicolor
title_full_unstemmed Perturbative corrections to technicolor
title_sort Perturbative corrections to technicolor
author Aguilar, A. C.
author_facet Aguilar, A. C.
Doff, A. [UNESP]
Natale, A. A. [UNESP]
author_role author
author2 Doff, A. [UNESP]
Natale, A. A. [UNESP]
author2_role author
author
dc.contributor.none.fl_str_mv Universidade Estadual de Campinas (UNICAMP)
Universidade Tecnológica Federal Do Paraná - UTFPR - DAFIS
Universidade Estadual Paulista (Unesp)
dc.contributor.author.fl_str_mv Aguilar, A. C.
Doff, A. [UNESP]
Natale, A. A. [UNESP]
description The full solution of technicolor (TC) Schwinger-Dyson equations should include radiative corrections induced by extended technicolor (ETC) (or other) interactions. We verify that when TC is embedded into a larger theory including also QCD, these radiative corrections couple the different strongly interacting Schwinger-Dyson equations, providing a tiny mass to technifermions and changing the ultraviolet behavior of the gap equation solution. We argue about the origin of the different quark masses without appealing for different ETC boson masses, in one scenario where most of the new physics will appear in interactions with the third fermion generation and with a TC scalar boson possibly lighter than the TC characteristic scale (ΛTC).
publishDate 2018
dc.date.none.fl_str_mv 2018-12-11T17:21:25Z
2018-12-11T17:21:25Z
2018-06-20
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://dx.doi.org/10.1103/PhysRevD.97.115035
Physical Review D, v. 97, n. 11, 2018.
2470-0029
2470-0010
http://hdl.handle.net/11449/176575
10.1103/PhysRevD.97.115035
2-s2.0-85049744503
url http://dx.doi.org/10.1103/PhysRevD.97.115035
http://hdl.handle.net/11449/176575
identifier_str_mv Physical Review D, v. 97, n. 11, 2018.
2470-0029
2470-0010
10.1103/PhysRevD.97.115035
2-s2.0-85049744503
dc.language.iso.fl_str_mv eng
language eng
dc.relation.none.fl_str_mv Physical Review D
1,801
1,801
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)
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