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

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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
Autores principales: Ledesma, D.S., Bellini, M.
Formato: Artículo publishedVersion
Lenguaje:Inglés
Publicado: 2004
Materias:
article
cosmos
evolution
Kaluza Klein theory
model
surface property
theoretical model
Acceso en línea:http://hdl.handle.net/20.500.12110/paper_03702693_v581_n1-2_p1_Ledesma
https://repositoriouba.sisbi.uba.ar/gsdl/cgi-bin/library.cgi?a=d&c=artiaex&d=paper_03702693_v581_n1-2_p1_Ledesma_oai
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Repositorio Digital de la Universidad de Buenos Aires (UBA) de Universidad de Buenos Aires
Descripción
Sumario: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.

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