Classical Bianchi Type I Cosmology in K-Essence Theory

We use one of the simplest forms of the K-essence theory and we apply it to the classical anisotropic Bianchi type I cosmological model, with a barotropic perfect fluid (p=γρ) modeling the usual matter content and with cosmological constant Λ. Classical exact solutions for any γ≠1 and Λ=0 are found...

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Main Authors: J. Socorro, Luis O. Pimentel, Abraham Espinoza-García
Format: Article
Language:English
Published: Wiley 2014-01-01
Series:Advances in High Energy Physics
Online Access:http://dx.doi.org/10.1155/2014/805164
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author J. Socorro
Luis O. Pimentel
Abraham Espinoza-García
author_facet J. Socorro
Luis O. Pimentel
Abraham Espinoza-García
author_sort J. Socorro
collection DOAJ
description We use one of the simplest forms of the K-essence theory and we apply it to the classical anisotropic Bianchi type I cosmological model, with a barotropic perfect fluid (p=γρ) modeling the usual matter content and with cosmological constant Λ. Classical exact solutions for any γ≠1 and Λ=0 are found in closed form, whereas solutions for Λ≠0 are found for particular values in the barotropic parameter. We present the possible isotropization of the cosmological model Bianchi I using the ratio between the anisotropic parameters and the volume of the universe. We also include a qualitative analysis of the analog of the Friedmann equation.
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spelling doaj-art-4db7722041c54bf09c5b9bc040a385272025-08-20T02:38:45ZengWileyAdvances in High Energy Physics1687-73571687-73652014-01-01201410.1155/2014/805164805164Classical Bianchi Type I Cosmology in K-Essence TheoryJ. Socorro0Luis O. Pimentel1Abraham Espinoza-García2Departamento de Física, DCeI, Universidad de Guanajuato, Campus León, Apartado Postal E-143, 37150 León, GTO, MexicoDepartamento de Física, Universidad Autónoma Metropolitana, Apartado Postal 55-534, 09340 México, DF, MexicoDepartamento de Física, DCeI, Universidad de Guanajuato, Campus León, Apartado Postal E-143, 37150 León, GTO, MexicoWe use one of the simplest forms of the K-essence theory and we apply it to the classical anisotropic Bianchi type I cosmological model, with a barotropic perfect fluid (p=γρ) modeling the usual matter content and with cosmological constant Λ. Classical exact solutions for any γ≠1 and Λ=0 are found in closed form, whereas solutions for Λ≠0 are found for particular values in the barotropic parameter. We present the possible isotropization of the cosmological model Bianchi I using the ratio between the anisotropic parameters and the volume of the universe. We also include a qualitative analysis of the analog of the Friedmann equation.http://dx.doi.org/10.1155/2014/805164
spellingShingle J. Socorro
Luis O. Pimentel
Abraham Espinoza-García
Classical Bianchi Type I Cosmology in K-Essence Theory
Advances in High Energy Physics
title Classical Bianchi Type I Cosmology in K-Essence Theory
title_full Classical Bianchi Type I Cosmology in K-Essence Theory
title_fullStr Classical Bianchi Type I Cosmology in K-Essence Theory
title_full_unstemmed Classical Bianchi Type I Cosmology in K-Essence Theory
title_short Classical Bianchi Type I Cosmology in K-Essence Theory
title_sort classical bianchi type i cosmology in k essence theory
url http://dx.doi.org/10.1155/2014/805164
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AT luisopimentel classicalbianchitypeicosmologyinkessencetheory
AT abrahamespinozagarcia classicalbianchitypeicosmologyinkessencetheory