Celestial strings: Field theory, conformally soft limits, and mapping the worldsheet onto the celestial sphere

Autores
Castiblanco, Lina; Giribet, Gaston Enrique; Marin, Gabriel; Rojas, Francisco German
Año de publicación
2024
Idioma
inglés
Tipo de recurso
artículo
Estado
versión publicada
Descripción
We compute the celestial correlators corresponding to tree-level 5-gluon amplitudes in the type I superstring theory. Since celestial correlation functions are obtained by integrating over the full range of energies, there is no obvious analog of the ′→0 limit in this basis. This is manifestly shown by a factorization of the ′ dependence in the celestial string amplitudes. Consequently, the question arises as to how the field theory limit is recovered from string theory in the celestial basis. This problem has been addressed in the literature for the case of 4-gluon amplitudes at tree level, where the forward scattering limit of the stringy factor was identified as a limit in which celestial Yang-Mills 4-point function is recovered. Here, we extend the analysis to the case with five gluons, for which the string moduli space allows for more types of limits, thus allowing us to investigate this aspect in more detail. Based on celestial data only, we study the regime in which one arrives at the correct celestial field theory limit. We also study other properties of the celestial string amplitudes, namely, the conformally soft theorem, effective field theory expansion in the conformal basis, and a map that arises in the regime of high-energy/large-scaling dimension that connects the punctured string world sheet to the insertion of primary operators in the celestial CFT for the massless -point string amplitude.
Fil: Castiblanco, Lina. University of Newcastle; Reino Unido
Fil: Giribet, Gaston Enrique. University of New York; Estados Unidos. Consejo Nacional de Investigaciones Científicas y Técnicas; Argentina
Fil: Marin, Gabriel. Universidad de Chile; Chile
Fil: Rojas, Francisco German. Universidad Adolfo Ibañez; Chile. Consejo Nacional de Investigaciones Científicas y Técnicas; Argentina
Materia
String theory
Celestial holography
Nivel de accesibilidad
acceso abierto
Condiciones de uso
https://creativecommons.org/licenses/by-nc-sa/2.5/ar/
Repositorio
CONICET Digital (CONICET)
Institución
Consejo Nacional de Investigaciones Científicas y Técnicas
OAI Identificador
oai:ri.conicet.gov.ar:11336/264833

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spelling Celestial strings: Field theory, conformally soft limits, and mapping the worldsheet onto the celestial sphereCastiblanco, LinaGiribet, Gaston EnriqueMarin, GabrielRojas, Francisco GermanString theoryCelestial holographyhttps://purl.org/becyt/ford/1.3https://purl.org/becyt/ford/1We compute the celestial correlators corresponding to tree-level 5-gluon amplitudes in the type I superstring theory. Since celestial correlation functions are obtained by integrating over the full range of energies, there is no obvious analog of the ′→0 limit in this basis. This is manifestly shown by a factorization of the ′ dependence in the celestial string amplitudes. Consequently, the question arises as to how the field theory limit is recovered from string theory in the celestial basis. This problem has been addressed in the literature for the case of 4-gluon amplitudes at tree level, where the forward scattering limit of the stringy factor was identified as a limit in which celestial Yang-Mills 4-point function is recovered. Here, we extend the analysis to the case with five gluons, for which the string moduli space allows for more types of limits, thus allowing us to investigate this aspect in more detail. Based on celestial data only, we study the regime in which one arrives at the correct celestial field theory limit. We also study other properties of the celestial string amplitudes, namely, the conformally soft theorem, effective field theory expansion in the conformal basis, and a map that arises in the regime of high-energy/large-scaling dimension that connects the punctured string world sheet to the insertion of primary operators in the celestial CFT for the massless -point string amplitude.Fil: Castiblanco, Lina. University of Newcastle; Reino UnidoFil: Giribet, Gaston Enrique. University of New York; Estados Unidos. Consejo Nacional de Investigaciones Científicas y Técnicas; ArgentinaFil: Marin, Gabriel. Universidad de Chile; ChileFil: Rojas, Francisco German. Universidad Adolfo Ibañez; Chile. Consejo Nacional de Investigaciones Científicas y Técnicas; ArgentinaAmerican Physical Society2024-12info:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersionhttp://purl.org/coar/resource_type/c_6501info:ar-repo/semantics/articuloapplication/pdfapplication/pdfhttp://hdl.handle.net/11336/264833Castiblanco, Lina; Giribet, Gaston Enrique; Marin, Gabriel; Rojas, Francisco German; Celestial strings: Field theory, conformally soft limits, and mapping the worldsheet onto the celestial sphere; American Physical Society; Physical Review D: Particles, Fields, Gravitation and Cosmology; 110; 12; 12-2024; 1-162470-00102470-0029CONICET DigitalCONICETenginfo:eu-repo/semantics/altIdentifier/url/https://link.aps.org/doi/10.1103/PhysRevD.110.126001info:eu-repo/semantics/altIdentifier/doi/10.1103/PhysRevD.110.126001info:eu-repo/semantics/openAccesshttps://creativecommons.org/licenses/by-nc-sa/2.5/ar/reponame:CONICET Digital (CONICET)instname:Consejo Nacional de Investigaciones Científicas y Técnicas2025-09-29T10:14:54Zoai:ri.conicet.gov.ar:11336/264833instacron:CONICETInstitucionalhttp://ri.conicet.gov.ar/Organismo científico-tecnológicoNo correspondehttp://ri.conicet.gov.ar/oai/requestdasensio@conicet.gov.ar; lcarlino@conicet.gov.arArgentinaNo correspondeNo correspondeNo correspondeopendoar:34982025-09-29 10:14:54.407CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicasfalse
dc.title.none.fl_str_mv Celestial strings: Field theory, conformally soft limits, and mapping the worldsheet onto the celestial sphere
title Celestial strings: Field theory, conformally soft limits, and mapping the worldsheet onto the celestial sphere
spellingShingle Celestial strings: Field theory, conformally soft limits, and mapping the worldsheet onto the celestial sphere
Castiblanco, Lina
String theory
Celestial holography
title_short Celestial strings: Field theory, conformally soft limits, and mapping the worldsheet onto the celestial sphere
title_full Celestial strings: Field theory, conformally soft limits, and mapping the worldsheet onto the celestial sphere
title_fullStr Celestial strings: Field theory, conformally soft limits, and mapping the worldsheet onto the celestial sphere
title_full_unstemmed Celestial strings: Field theory, conformally soft limits, and mapping the worldsheet onto the celestial sphere
title_sort Celestial strings: Field theory, conformally soft limits, and mapping the worldsheet onto the celestial sphere
dc.creator.none.fl_str_mv Castiblanco, Lina
Giribet, Gaston Enrique
Marin, Gabriel
Rojas, Francisco German
author Castiblanco, Lina
author_facet Castiblanco, Lina
Giribet, Gaston Enrique
Marin, Gabriel
Rojas, Francisco German
author_role author
author2 Giribet, Gaston Enrique
Marin, Gabriel
Rojas, Francisco German
author2_role author
author
author
dc.subject.none.fl_str_mv String theory
Celestial holography
topic String theory
Celestial holography
purl_subject.fl_str_mv https://purl.org/becyt/ford/1.3
https://purl.org/becyt/ford/1
dc.description.none.fl_txt_mv We compute the celestial correlators corresponding to tree-level 5-gluon amplitudes in the type I superstring theory. Since celestial correlation functions are obtained by integrating over the full range of energies, there is no obvious analog of the ′→0 limit in this basis. This is manifestly shown by a factorization of the ′ dependence in the celestial string amplitudes. Consequently, the question arises as to how the field theory limit is recovered from string theory in the celestial basis. This problem has been addressed in the literature for the case of 4-gluon amplitudes at tree level, where the forward scattering limit of the stringy factor was identified as a limit in which celestial Yang-Mills 4-point function is recovered. Here, we extend the analysis to the case with five gluons, for which the string moduli space allows for more types of limits, thus allowing us to investigate this aspect in more detail. Based on celestial data only, we study the regime in which one arrives at the correct celestial field theory limit. We also study other properties of the celestial string amplitudes, namely, the conformally soft theorem, effective field theory expansion in the conformal basis, and a map that arises in the regime of high-energy/large-scaling dimension that connects the punctured string world sheet to the insertion of primary operators in the celestial CFT for the massless -point string amplitude.
Fil: Castiblanco, Lina. University of Newcastle; Reino Unido
Fil: Giribet, Gaston Enrique. University of New York; Estados Unidos. Consejo Nacional de Investigaciones Científicas y Técnicas; Argentina
Fil: Marin, Gabriel. Universidad de Chile; Chile
Fil: Rojas, Francisco German. Universidad Adolfo Ibañez; Chile. Consejo Nacional de Investigaciones Científicas y Técnicas; Argentina
description We compute the celestial correlators corresponding to tree-level 5-gluon amplitudes in the type I superstring theory. Since celestial correlation functions are obtained by integrating over the full range of energies, there is no obvious analog of the ′→0 limit in this basis. This is manifestly shown by a factorization of the ′ dependence in the celestial string amplitudes. Consequently, the question arises as to how the field theory limit is recovered from string theory in the celestial basis. This problem has been addressed in the literature for the case of 4-gluon amplitudes at tree level, where the forward scattering limit of the stringy factor was identified as a limit in which celestial Yang-Mills 4-point function is recovered. Here, we extend the analysis to the case with five gluons, for which the string moduli space allows for more types of limits, thus allowing us to investigate this aspect in more detail. Based on celestial data only, we study the regime in which one arrives at the correct celestial field theory limit. We also study other properties of the celestial string amplitudes, namely, the conformally soft theorem, effective field theory expansion in the conformal basis, and a map that arises in the regime of high-energy/large-scaling dimension that connects the punctured string world sheet to the insertion of primary operators in the celestial CFT for the massless -point string amplitude.
publishDate 2024
dc.date.none.fl_str_mv 2024-12
dc.type.none.fl_str_mv info:eu-repo/semantics/article
info:eu-repo/semantics/publishedVersion
http://purl.org/coar/resource_type/c_6501
info:ar-repo/semantics/articulo
format article
status_str publishedVersion
dc.identifier.none.fl_str_mv http://hdl.handle.net/11336/264833
Castiblanco, Lina; Giribet, Gaston Enrique; Marin, Gabriel; Rojas, Francisco German; Celestial strings: Field theory, conformally soft limits, and mapping the worldsheet onto the celestial sphere; American Physical Society; Physical Review D: Particles, Fields, Gravitation and Cosmology; 110; 12; 12-2024; 1-16
2470-0010
2470-0029
CONICET Digital
CONICET
url http://hdl.handle.net/11336/264833
identifier_str_mv Castiblanco, Lina; Giribet, Gaston Enrique; Marin, Gabriel; Rojas, Francisco German; Celestial strings: Field theory, conformally soft limits, and mapping the worldsheet onto the celestial sphere; American Physical Society; Physical Review D: Particles, Fields, Gravitation and Cosmology; 110; 12; 12-2024; 1-16
2470-0010
2470-0029
CONICET Digital
CONICET
dc.language.none.fl_str_mv eng
language eng
dc.relation.none.fl_str_mv info:eu-repo/semantics/altIdentifier/url/https://link.aps.org/doi/10.1103/PhysRevD.110.126001
info:eu-repo/semantics/altIdentifier/doi/10.1103/PhysRevD.110.126001
dc.rights.none.fl_str_mv info:eu-repo/semantics/openAccess
https://creativecommons.org/licenses/by-nc-sa/2.5/ar/
eu_rights_str_mv openAccess
rights_invalid_str_mv https://creativecommons.org/licenses/by-nc-sa/2.5/ar/
dc.format.none.fl_str_mv application/pdf
application/pdf
dc.publisher.none.fl_str_mv American Physical Society
publisher.none.fl_str_mv American Physical Society
dc.source.none.fl_str_mv reponame:CONICET Digital (CONICET)
instname:Consejo Nacional de Investigaciones Científicas y Técnicas
reponame_str CONICET Digital (CONICET)
collection CONICET Digital (CONICET)
instname_str Consejo Nacional de Investigaciones Científicas y Técnicas
repository.name.fl_str_mv CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicas
repository.mail.fl_str_mv dasensio@conicet.gov.ar; lcarlino@conicet.gov.ar
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