Celestial IR divergences in general most-subleading-color gluon and gravity amplitudes

Detalhes bibliográficos
Autor(a) principal: Nastase, Horatiu [UNESP]
Data de Publicação: 2022
Outros Autores: Rojas, Francisco, Rubio, Carlos
Tipo de documento: Artigo
Idioma: eng
Título da fonte: Repositório Institucional da UNESP
Texto Completo: http://dx.doi.org/10.1007/JHEP01(2022)136
http://hdl.handle.net/11449/230306
Resumo: Gluon amplitudes at most-subleading order in the 1/N expansion share a remarkable simplicity with graviton amplitudes: collinear divergences are completely absent in both and, as a consequence, their full IR behavior arises from soft gluon/graviton exchange among the external states. In this paper we study the effect of all-loop IR divergences of celestial most-subleading color gluon amplitudes and their similarities with the celestial gravity case. In particular, a simple celestial exponentiation formula for the dipole part can be written. We also analize how this exponentiation is modified by non-dipole contributions. Finally we also show that, in the Regge limit, the soft factor satisfies the Knizhnik-Zamolodchikov equation hinting at the possibility that, in this limit, an effective Wess-Zumino-Witten model would describe the dynamics of the infrared sector.
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spelling Celestial IR divergences in general most-subleading-color gluon and gravity amplitudesConformal Field TheoryScattering AmplitudesGluon amplitudes at most-subleading order in the 1/N expansion share a remarkable simplicity with graviton amplitudes: collinear divergences are completely absent in both and, as a consequence, their full IR behavior arises from soft gluon/graviton exchange among the external states. In this paper we study the effect of all-loop IR divergences of celestial most-subleading color gluon amplitudes and their similarities with the celestial gravity case. In particular, a simple celestial exponentiation formula for the dipole part can be written. We also analize how this exponentiation is modified by non-dipole contributions. Finally we also show that, in the Regge limit, the soft factor satisfies the Knizhnik-Zamolodchikov equation hinting at the possibility that, in this limit, an effective Wess-Zumino-Witten model would describe the dynamics of the infrared sector.Instituto de Física Teórica UNESP-Universidade Estadual Paulista, R. Dr. Bento T. Ferraz 271, Bl. II, SPFacultad de Ingeniería y Ciencias Universidad Adolfo Ibáñez, Diagonal Las Torres 2640, SantiagoInstituto de Física Teórica UNESP-Universidade Estadual Paulista, R. Dr. Bento T. Ferraz 271, Bl. II, SPUniversidade Estadual Paulista (UNESP)Universidad Adolfo IbáñezNastase, Horatiu [UNESP]Rojas, FranciscoRubio, Carlos2022-04-29T08:39:09Z2022-04-29T08:39:09Z2022-01-01info:eu-repo/semantics/publishedVersioninfo:eu-repo/semantics/articlehttp://dx.doi.org/10.1007/JHEP01(2022)136Journal of High Energy Physics, v. 2022, n. 1, 2022.1029-8479http://hdl.handle.net/11449/23030610.1007/JHEP01(2022)1362-s2.0-85123768094Scopusreponame:Repositório Institucional da UNESPinstname:Universidade Estadual Paulista (UNESP)instacron:UNESPengJournal of High Energy Physicsinfo:eu-repo/semantics/openAccess2022-04-29T08:39:10Zoai:repositorio.unesp.br:11449/230306Repositório InstitucionalPUBhttp://repositorio.unesp.br/oai/requestopendoar:29462024-08-05T18:08:57.129220Repositório Institucional da UNESP - Universidade Estadual Paulista (UNESP)false
dc.title.none.fl_str_mv Celestial IR divergences in general most-subleading-color gluon and gravity amplitudes
title Celestial IR divergences in general most-subleading-color gluon and gravity amplitudes
spellingShingle Celestial IR divergences in general most-subleading-color gluon and gravity amplitudes
Nastase, Horatiu [UNESP]
Conformal Field Theory
Scattering Amplitudes
title_short Celestial IR divergences in general most-subleading-color gluon and gravity amplitudes
title_full Celestial IR divergences in general most-subleading-color gluon and gravity amplitudes
title_fullStr Celestial IR divergences in general most-subleading-color gluon and gravity amplitudes
title_full_unstemmed Celestial IR divergences in general most-subleading-color gluon and gravity amplitudes
title_sort Celestial IR divergences in general most-subleading-color gluon and gravity amplitudes
author Nastase, Horatiu [UNESP]
author_facet Nastase, Horatiu [UNESP]
Rojas, Francisco
Rubio, Carlos
author_role author
author2 Rojas, Francisco
Rubio, Carlos
author2_role author
author
dc.contributor.none.fl_str_mv Universidade Estadual Paulista (UNESP)
Universidad Adolfo Ibáñez
dc.contributor.author.fl_str_mv Nastase, Horatiu [UNESP]
Rojas, Francisco
Rubio, Carlos
dc.subject.por.fl_str_mv Conformal Field Theory
Scattering Amplitudes
topic Conformal Field Theory
Scattering Amplitudes
description Gluon amplitudes at most-subleading order in the 1/N expansion share a remarkable simplicity with graviton amplitudes: collinear divergences are completely absent in both and, as a consequence, their full IR behavior arises from soft gluon/graviton exchange among the external states. In this paper we study the effect of all-loop IR divergences of celestial most-subleading color gluon amplitudes and their similarities with the celestial gravity case. In particular, a simple celestial exponentiation formula for the dipole part can be written. We also analize how this exponentiation is modified by non-dipole contributions. Finally we also show that, in the Regge limit, the soft factor satisfies the Knizhnik-Zamolodchikov equation hinting at the possibility that, in this limit, an effective Wess-Zumino-Witten model would describe the dynamics of the infrared sector.
publishDate 2022
dc.date.none.fl_str_mv 2022-04-29T08:39:09Z
2022-04-29T08:39:09Z
2022-01-01
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/10.1007/JHEP01(2022)136
Journal of High Energy Physics, v. 2022, n. 1, 2022.
1029-8479
http://hdl.handle.net/11449/230306
10.1007/JHEP01(2022)136
2-s2.0-85123768094
url http://dx.doi.org/10.1007/JHEP01(2022)136
http://hdl.handle.net/11449/230306
identifier_str_mv Journal of High Energy Physics, v. 2022, n. 1, 2022.
1029-8479
10.1007/JHEP01(2022)136
2-s2.0-85123768094
dc.language.iso.fl_str_mv eng
language eng
dc.relation.none.fl_str_mv Journal of High Energy Physics
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
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