Scalar field cosmology in three-dimensions

Fuente: Redalyc
Enregistré dans:
Détails bibliographiques
Auteur principal: G. Oliveira-Neto
Format: Artículo científico
Langue:en
Publié: Sociedade Brasileira de Física 2001
Sujets:
Accès en ligne:
Tags: Ajouter un tag
Pas de tags, Soyez le premier à ajouter un tag!
_version_ 1876428715173347328
author G. Oliveira-Neto
author_facet G. Oliveira-Neto
contents Scalar field cosmology in three-dimensions G. Oliveira-Neto Física, Astronomía y Matemáticas We study an analytical solution to the Einstein's equations in 2 + 1-dimensions. The space-time is dynamical and has a line symmetry. The matter content is a minimally coupled, massless, scalar field. Depending on the value of certain parameters, this solution represents three distinct space-times. The first one is at space-time. Then, we have a big bang model with a negative curvature scalar and a real scalar field. The last case is a big bang model with event horizons where the curvature scalar vanishes and the scalar field changes from real to purely imaginary. 2001 artículo científico 0103-9733 https://www.redalyc.org/articulo.oa?id=46413502017 en http://www.redalyc.org/revista.oa?id=464 Brazilian Journal of Physics application/pdf Sociedade Brasileira de Física Brazilian Journal of Physics (Brasil) Num.3 Vol.31
format Artículo científico
id redalyc_46413502017
institution Redalyc
language en
publishDate 2001
publisher Sociedade Brasileira de Física
spellingShingle Scalar field cosmology in three-dimensions
G. Oliveira-Neto
Física, Astronomía y Matemáticas
Scalar field cosmology in three-dimensions G. Oliveira-Neto Física, Astronomía y Matemáticas We study an analytical solution to the Einstein's equations in 2 + 1-dimensions. The space-time is dynamical and has a line symmetry. The matter content is a minimally coupled, massless, scalar field. Depending on the value of certain parameters, this solution represents three distinct space-times. The first one is at space-time. Then, we have a big bang model with a negative curvature scalar and a real scalar field. The last case is a big bang model with event horizons where the curvature scalar vanishes and the scalar field changes from real to purely imaginary. 2001 artículo científico 0103-9733 https://www.redalyc.org/articulo.oa?id=46413502017 en http://www.redalyc.org/revista.oa?id=464 Brazilian Journal of Physics application/pdf Sociedade Brasileira de Física Brazilian Journal of Physics (Brasil) Num.3 Vol.31
title Scalar field cosmology in three-dimensions
topic Física, Astronomía y Matemáticas
url https://www.redalyc.org/articulo.oa?id=46413502017