Brane Worlds, String Cosmology, and AdS/CFT

Autores
Anchordoqui, Luis Alfredo; Edelstein, José D.; Núñez, Carlos; Pérez Bergliaffa, Santiago Esteban; Schvellinger, Martín Alejandro; Trobo, Marta Liliana; Zyserman, Fabio Iván
Año de publicación
2001
Idioma
inglés
Tipo de recurso
artículo
Estado
versión publicada
Descripción
Using the thin-shell formalism we discuss the motion of domain walls in de Sitter and anti--de Sitter (AdS) time-dependent bulks. This motion results in a dynamics for the brane scale factor. We show that in the case of a clean brane the scale factor describes both singular and nonsingular universes, with phases of contraction and expansion. These phases can be understood as quotients of AdS spacetime by a discrete symmetry group. We discuss this effect in some detail, and suggest how the AdS/CFT correspondence could be applied to obtain a nonperturbative description of brane-world string cosmology.
Facultad de Ciencias Exactas
Materia
Física
ADS/QCD correspondence
Physics
Spacetime
String cosmology
De Sitter universe
Discrete symmetry
Theoretical physics
DS/CFT correspondence
Brane
Classical mechanics
Nivel de accesibilidad
acceso abierto
Condiciones de uso
http://creativecommons.org/licenses/by-nc-sa/4.0/
Repositorio
SEDICI (UNLP)
Institución
Universidad Nacional de La Plata
OAI Identificador
oai:sedici.unlp.edu.ar:10915/126583
Acceder
id SEDICI_7e58bfd84ab931788d46a6eec58c7edb
oai_identifier_str oai:sedici.unlp.edu.ar:10915/126583
network_acronym_str SEDICI
repository_id_str 1329
network_name_str SEDICI (UNLP)
spelling Brane Worlds, String Cosmology, and AdS/CFTAnchordoqui, Luis AlfredoEdelstein, José D.Núñez, CarlosPérez Bergliaffa, Santiago EstebanSchvellinger, Martín AlejandroTrobo, Marta LilianaZyserman, Fabio IvánFísicaADS/QCD correspondencePhysicsSpacetimeString cosmologyDe Sitter universeDiscrete symmetryTheoretical physicsDS/CFT correspondenceBraneClassical mechanicsUsing the thin-shell formalism we discuss the motion of domain walls in de Sitter and anti--de Sitter (AdS) time-dependent bulks. This motion results in a dynamics for the brane scale factor. We show that in the case of a clean brane the scale factor describes both singular and nonsingular universes, with phases of contraction and expansion. These phases can be understood as quotients of AdS spacetime by a discrete symmetry group. We discuss this effect in some detail, and suggest how the AdS/CFT correspondence could be applied to obtain a nonperturbative description of brane-world string cosmology.Facultad de Ciencias Exactas2001-09-26info:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersionArticulohttp://purl.org/coar/resource_type/c_6501info:ar-repo/semantics/articuloapplication/pdfhttp://sedici.unlp.edu.ar/handle/10915/126583enginfo:eu-repo/semantics/altIdentifier/issn/0556-2821info:eu-repo/semantics/altIdentifier/issn/1089-4918info:eu-repo/semantics/altIdentifier/arxiv/hep-th/0106127info:eu-repo/semantics/altIdentifier/doi/10.1103/physrevd.64.084027info:eu-repo/semantics/openAccesshttp://creativecommons.org/licenses/by-nc-sa/4.0/Creative Commons Attribution-NonCommercial-ShareAlike 4.0 International (CC BY-NC-SA 4.0)reponame:SEDICI (UNLP)instname:Universidad Nacional de La Platainstacron:UNLP2025-10-22T17:11:16Zoai:sedici.unlp.edu.ar:10915/126583Institucionalhttp://sedici.unlp.edu.ar/Universidad públicaNo correspondehttp://sedici.unlp.edu.ar/oai/snrdalira@sedici.unlp.edu.arArgentinaNo correspondeNo correspondeNo correspondeopendoar:13292025-10-22 17:11:16.426SEDICI (UNLP) - Universidad Nacional de La Platafalse
dc.title.none.fl_str_mv Brane Worlds, String Cosmology, and AdS/CFT
title Brane Worlds, String Cosmology, and AdS/CFT
spellingShingle Brane Worlds, String Cosmology, and AdS/CFT
Anchordoqui, Luis Alfredo
Física
ADS/QCD correspondence
Physics
Spacetime
String cosmology
De Sitter universe
Discrete symmetry
Theoretical physics
DS/CFT correspondence
Brane
Classical mechanics
title_short Brane Worlds, String Cosmology, and AdS/CFT
title_full Brane Worlds, String Cosmology, and AdS/CFT
title_fullStr Brane Worlds, String Cosmology, and AdS/CFT
title_full_unstemmed Brane Worlds, String Cosmology, and AdS/CFT
title_sort Brane Worlds, String Cosmology, and AdS/CFT
dc.creator.none.fl_str_mv Anchordoqui, Luis Alfredo
Edelstein, José D.
Núñez, Carlos
Pérez Bergliaffa, Santiago Esteban
Schvellinger, Martín Alejandro
Trobo, Marta Liliana
Zyserman, Fabio Iván
author Anchordoqui, Luis Alfredo
author_facet Anchordoqui, Luis Alfredo
Edelstein, José D.
Núñez, Carlos
Pérez Bergliaffa, Santiago Esteban
Schvellinger, Martín Alejandro
Trobo, Marta Liliana
Zyserman, Fabio Iván
author_role author
author2 Edelstein, José D.
Núñez, Carlos
Pérez Bergliaffa, Santiago Esteban
Schvellinger, Martín Alejandro
Trobo, Marta Liliana
Zyserman, Fabio Iván
author2_role author
author
author
author
author
author
dc.subject.none.fl_str_mv Física
ADS/QCD correspondence
Physics
Spacetime
String cosmology
De Sitter universe
Discrete symmetry
Theoretical physics
DS/CFT correspondence
Brane
Classical mechanics
topic Física
ADS/QCD correspondence
Physics
Spacetime
String cosmology
De Sitter universe
Discrete symmetry
Theoretical physics
DS/CFT correspondence
Brane
Classical mechanics
dc.description.none.fl_txt_mv Using the thin-shell formalism we discuss the motion of domain walls in de Sitter and anti--de Sitter (AdS) time-dependent bulks. This motion results in a dynamics for the brane scale factor. We show that in the case of a clean brane the scale factor describes both singular and nonsingular universes, with phases of contraction and expansion. These phases can be understood as quotients of AdS spacetime by a discrete symmetry group. We discuss this effect in some detail, and suggest how the AdS/CFT correspondence could be applied to obtain a nonperturbative description of brane-world string cosmology.
Facultad de Ciencias Exactas
description Using the thin-shell formalism we discuss the motion of domain walls in de Sitter and anti--de Sitter (AdS) time-dependent bulks. This motion results in a dynamics for the brane scale factor. We show that in the case of a clean brane the scale factor describes both singular and nonsingular universes, with phases of contraction and expansion. These phases can be understood as quotients of AdS spacetime by a discrete symmetry group. We discuss this effect in some detail, and suggest how the AdS/CFT correspondence could be applied to obtain a nonperturbative description of brane-world string cosmology.
publishDate 2001
dc.date.none.fl_str_mv 2001-09-26
dc.type.none.fl_str_mv info:eu-repo/semantics/article
info:eu-repo/semantics/publishedVersion
Articulo
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://sedici.unlp.edu.ar/handle/10915/126583
url http://sedici.unlp.edu.ar/handle/10915/126583
dc.language.none.fl_str_mv eng
language eng
dc.relation.none.fl_str_mv info:eu-repo/semantics/altIdentifier/issn/0556-2821
info:eu-repo/semantics/altIdentifier/issn/1089-4918
info:eu-repo/semantics/altIdentifier/arxiv/hep-th/0106127
info:eu-repo/semantics/altIdentifier/doi/10.1103/physrevd.64.084027
dc.rights.none.fl_str_mv info:eu-repo/semantics/openAccess
http://creativecommons.org/licenses/by-nc-sa/4.0/
Creative Commons Attribution-NonCommercial-ShareAlike 4.0 International (CC BY-NC-SA 4.0)
eu_rights_str_mv openAccess
rights_invalid_str_mv http://creativecommons.org/licenses/by-nc-sa/4.0/
Creative Commons Attribution-NonCommercial-ShareAlike 4.0 International (CC BY-NC-SA 4.0)
dc.format.none.fl_str_mv application/pdf
dc.source.none.fl_str_mv reponame:SEDICI (UNLP)
instname:Universidad Nacional de La Plata
instacron:UNLP
reponame_str SEDICI (UNLP)
collection SEDICI (UNLP)
instname_str Universidad Nacional de La Plata
instacron_str UNLP
institution UNLP
repository.name.fl_str_mv SEDICI (UNLP) - Universidad Nacional de La Plata
repository.mail.fl_str_mv alira@sedici.unlp.edu.ar
_version_ 1846783460210900992
score 12.982451

Publicaciones similares