Perturbative corrections to technicolor
Autor(a) principal: | |
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Data de Publicação: | 2018 |
Outros Autores: | , |
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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2946 |
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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) |
repository.mail.fl_str_mv |
|
_version_ |
1808129485200949248 |