Single field inflationary models with non-compact Kaluza-Klein theory

Autores
Ledesma, D.S.; Bellini, M.
Año de publicación
2004
Idioma
inglés
Tipo de recurso
artículo
Estado
versión publicada
Descripción
We discuss a semiclassical treatment to inflationary models from Kaluza-Klein theory without the cylinder condition. We conclude that the evolution of the early universe could be described by a geodesic trajectory of a cosmological 5D metric here proposed, so that the effective 4D FRW background metric should be a hypersurface on a constant fifth dimension. © 2003 Elsevier B.V. All rights reserved.
Fuente
Phys Lett Sect B Nucl Elem Part High-Energy Phys 2004;581(1-2):1-8
Materia
article
cosmos
evolution
Kaluza Klein theory
model
surface property
theoretical model
Nivel de accesibilidad
acceso abierto
Condiciones de uso
http://creativecommons.org/licenses/by/2.5/ar
Repositorio
Biblioteca Digital (UBA-FCEN)
Institución
Universidad Nacional de Buenos Aires. Facultad de Ciencias Exactas y Naturales
OAI Identificador
paperaa:paper_03702693_v581_n1-2_p1_Ledesma
Acceder
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oai_identifier_str paperaa:paper_03702693_v581_n1-2_p1_Ledesma
network_acronym_str BDUBAFCEN
repository_id_str 1896
network_name_str Biblioteca Digital (UBA-FCEN)
spelling Single field inflationary models with non-compact Kaluza-Klein theoryLedesma, D.S.Bellini, M.articlecosmosevolutionKaluza Klein theorymodelsurface propertytheoretical modelWe discuss a semiclassical treatment to inflationary models from Kaluza-Klein theory without the cylinder condition. We conclude that the evolution of the early universe could be described by a geodesic trajectory of a cosmological 5D metric here proposed, so that the effective 4D FRW background metric should be a hypersurface on a constant fifth dimension. © 2003 Elsevier B.V. All rights reserved.2004info:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersionhttp://purl.org/coar/resource_type/c_6501info:ar-repo/semantics/articuloapplication/pdfhttp://hdl.handle.net/20.500.12110/paper_03702693_v581_n1-2_p1_LedesmaPhys Lett Sect B Nucl Elem Part High-Energy Phys 2004;581(1-2):1-8reponame:Biblioteca Digital (UBA-FCEN)instname:Universidad Nacional de Buenos Aires. Facultad de Ciencias Exactas y Naturalesinstacron:UBA-FCENenginfo:eu-repo/semantics/openAccesshttp://creativecommons.org/licenses/by/2.5/ar2025-11-06T09:39:44Zpaperaa:paper_03702693_v581_n1-2_p1_LedesmaInstitucionalhttps://digital.bl.fcen.uba.ar/Universidad públicaNo correspondehttps://digital.bl.fcen.uba.ar/cgi-bin/oaiserver.cgiana@bl.fcen.uba.arArgentinaNo correspondeNo correspondeNo correspondeopendoar:18962025-11-06 09:39:45.58Biblioteca Digital (UBA-FCEN) - Universidad Nacional de Buenos Aires. Facultad de Ciencias Exactas y Naturalesfalse
dc.title.none.fl_str_mv Single field inflationary models with non-compact Kaluza-Klein theory
title Single field inflationary models with non-compact Kaluza-Klein theory
spellingShingle Single field inflationary models with non-compact Kaluza-Klein theory
Ledesma, D.S.
article
cosmos
evolution
Kaluza Klein theory
model
surface property
theoretical model
title_short Single field inflationary models with non-compact Kaluza-Klein theory
title_full Single field inflationary models with non-compact Kaluza-Klein theory
title_fullStr Single field inflationary models with non-compact Kaluza-Klein theory
title_full_unstemmed Single field inflationary models with non-compact Kaluza-Klein theory
title_sort Single field inflationary models with non-compact Kaluza-Klein theory
dc.creator.none.fl_str_mv Ledesma, D.S.
Bellini, M.
author Ledesma, D.S.
author_facet Ledesma, D.S.
Bellini, M.
author_role author
author2 Bellini, M.
author2_role author
dc.subject.none.fl_str_mv article
cosmos
evolution
Kaluza Klein theory
model
surface property
theoretical model
topic article
cosmos
evolution
Kaluza Klein theory
model
surface property
theoretical model
dc.description.none.fl_txt_mv We discuss a semiclassical treatment to inflationary models from Kaluza-Klein theory without the cylinder condition. We conclude that the evolution of the early universe could be described by a geodesic trajectory of a cosmological 5D metric here proposed, so that the effective 4D FRW background metric should be a hypersurface on a constant fifth dimension. © 2003 Elsevier B.V. All rights reserved.
description We discuss a semiclassical treatment to inflationary models from Kaluza-Klein theory without the cylinder condition. We conclude that the evolution of the early universe could be described by a geodesic trajectory of a cosmological 5D metric here proposed, so that the effective 4D FRW background metric should be a hypersurface on a constant fifth dimension. © 2003 Elsevier B.V. All rights reserved.
publishDate 2004
dc.date.none.fl_str_mv 2004
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/20.500.12110/paper_03702693_v581_n1-2_p1_Ledesma
url http://hdl.handle.net/20.500.12110/paper_03702693_v581_n1-2_p1_Ledesma
dc.language.none.fl_str_mv eng
language eng
dc.rights.none.fl_str_mv info:eu-repo/semantics/openAccess
http://creativecommons.org/licenses/by/2.5/ar
eu_rights_str_mv openAccess
rights_invalid_str_mv http://creativecommons.org/licenses/by/2.5/ar
dc.format.none.fl_str_mv application/pdf
dc.source.none.fl_str_mv Phys Lett Sect B Nucl Elem Part High-Energy Phys 2004;581(1-2):1-8
reponame:Biblioteca Digital (UBA-FCEN)
instname:Universidad Nacional de Buenos Aires. Facultad de Ciencias Exactas y Naturales
instacron:UBA-FCEN
reponame_str Biblioteca Digital (UBA-FCEN)
collection Biblioteca Digital (UBA-FCEN)
instname_str Universidad Nacional de Buenos Aires. Facultad de Ciencias Exactas y Naturales
instacron_str UBA-FCEN
institution UBA-FCEN
repository.name.fl_str_mv Biblioteca Digital (UBA-FCEN) - Universidad Nacional de Buenos Aires. Facultad de Ciencias Exactas y Naturales
repository.mail.fl_str_mv ana@bl.fcen.uba.ar
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score 13.087074

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