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
- Institución
- Consejo Nacional de Investigaciones Científicas y Técnicas
- OAI Identificador
- oai:ri.conicet.gov.ar:11336/264833
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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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1844614080610959361 |
score |
13.070432 |