Ledesma, D.S. - Bellini, M.

En:

Phys Lett Sect B Nucl Elem Part High-Energy Phys 2004;581(1-2):1-8

Fecha:

2004

Formato:

application/pdf

Tipo de documento:

info:eu-repo/semantics/article
info:ar-repo/semantics/artículo
info:eu-repo/semantics/publishedVersion

Idioma:

eng

Descriptores:

article - cosmos - evolution - Kaluza Klein theory - model - surface property - theoretical model

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.

Identificador(es):

http://hdl.handle.net/20.500.12110/paper_03702693_v581_n1-2_p1_Ledesma

Derechos:

info:eu-repo/semantics/openAccess
http://creativecommons.org/licenses/by/2.5/ar

Descargar texto: paper_03702693_v581_n1-2_p1_Ledesma.oai

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Cita bibliográfica:

Ledesma, D.S. (2004). Single field inflationary models with non-compact Kaluza-Klein theory (info:eu-repo/semantics/article). [consultado: ] Disponible en el Repositorio Digital Institucional de la Universidad de Buenos Aires: <http://repositoriouba.sisbi.uba.ar/gsdl/cgi-bin/library.cgi?a=d&c=artiaex&cl=CL1&d=paper_03702693_v581_n1-2_p1_Ledesma_oai>