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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Detalles Bibliográficos
Publicado: 2004
Materias:
article
cosmos
evolution
Kaluza Klein theory
model
surface property
theoretical model
Acceso en línea:https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_03702693_v581_n1-2_p1_Ledesma
http://hdl.handle.net/20.500.12110/paper_03702693_v581_n1-2_p1_Ledesma
Aporte de:
Biblioteca Digital - Facultad de Ciencias Exactas y Naturales (UBA) de Universidad de Buenos Aires
id paper:paper_03702693_v581_n1-2_p1_Ledesma
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spelling paper:paper_03702693_v581_n1-2_p1_Ledesma2023-06-08T15:36:40Z Single field inflationary models with non-compact Kaluza-Klein theory 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. 2004 https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_03702693_v581_n1-2_p1_Ledesma 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)
topic article
cosmos
evolution
Kaluza Klein theory
model
surface property
theoretical model
spellingShingle article
cosmos
evolution
Kaluza Klein theory
model
surface property
theoretical model
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.
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
publishDate 2004
url https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_03702693_v581_n1-2_p1_Ledesma
http://hdl.handle.net/20.500.12110/paper_03702693_v581_n1-2_p1_Ledesma
_version_ 1768546117379686400

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