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

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 met...

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Autores principales: Ledesma, D.S., Bellini, M.
Formato: JOUR
Lenguaje:English
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Acceso en línea:http://hdl.handle.net/20.500.12110/paper_03702693_v581_n1-2_p1_Ledesma
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spelling todo:paper_03702693_v581_n1-2_p1_Ledesma2023-10-03T15:28:54Z Single field inflationary models with non-compact Kaluza-Klein theory Ledesma, D.S. Bellini, M. article cosmos evolution Kaluza Klein theory model surface property theoretical model 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. JOUR English info:eu-repo/semantics/openAccess http://creativecommons.org/licenses/by/2.5/ar http://hdl.handle.net/20.500.12110/paper_03702693_v581_n1-2_p1_Ledesma
institution Universidad de Buenos Aires
institution_str I-28
repository_str R-134
collection Biblioteca Digital - Facultad de Ciencias Exactas y Naturales (UBA)
language English
orig_language_str_mv English
topic article
cosmos
evolution
Kaluza Klein theory
model
surface property
theoretical model
spellingShingle article
cosmos
evolution
Kaluza Klein theory
model
surface property
theoretical model
Ledesma, D.S.
Bellini, M.
Single field inflationary models with non-compact Kaluza-Klein theory
topic_facet article
cosmos
evolution
Kaluza Klein theory
model
surface property
theoretical model
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.
format JOUR
author Ledesma, D.S.
Bellini, M.
author_facet Ledesma, D.S.
Bellini, M.
author_sort Ledesma, D.S.
title Single field inflationary models with non-compact Kaluza-Klein theory
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
url http://hdl.handle.net/20.500.12110/paper_03702693_v581_n1-2_p1_Ledesma
work_keys_str_mv AT ledesmads singlefieldinflationarymodelswithnoncompactkaluzakleintheory
AT bellinim singlefieldinflationarymodelswithnoncompactkaluzakleintheory
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