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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Acceso en línea: | http://hdl.handle.net/20.500.12110/paper_03702693_v581_n1-2_p1_Ledesma |
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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 |
_version_ |
1807321041451614208 |