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
- Institución
- Universidad Nacional de La Plata
- OAI Identificador
- oai:sedici.unlp.edu.ar:10915/126583
Ver los metadatos del registro completo
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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:UNLP2025-09-29T11:30:22Zoai: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:13292025-09-29 11:30:23.213SEDICI (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) |
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openAccess |
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http://creativecommons.org/licenses/by-nc-sa/4.0/ Creative Commons Attribution-NonCommercial-ShareAlike 4.0 International (CC BY-NC-SA 4.0) |
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application/pdf |
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SEDICI (UNLP) - Universidad Nacional de La Plata |
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