Celestial IR divergences in general most-subleading-color gluon and gravity amplitudes
Autor(a) principal: | |
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Data de Publicação: | 2022 |
Outros Autores: | , |
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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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 |
|
_version_ |
1808128901780602880 |