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Journal ArticleDOI

Bianchi Type V Cosmological Models with Constant Deceleration Parameter in General Relativity

J. P. Singh, +1 more
- 01 Feb 2009 - 
- Vol. 48, Iss: 2, pp 449-462
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TLDR
In this article, Bianchi type V cosmological models with bulk viscous fluid source were investigated and exact solutions of the Einstein field equations were presented via a suitable power law assumption for the Hubble parameter.
Abstract
We investigate Bianchi type V cosmological models with bulk viscous fluid source. Exact solutions of the Einstein field equations are presented via a suitable power law assumption for the Hubble parameter. We show that the corresponding solutions retain the well established features of the standard cosmology and in addition, are in accordance with recent type Ia supernovae observations. Some observational parameters for the models have also been discussed.

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Bianchi type III models with anisotropic dark energy

TL;DR: In this article, the general form of the anisotropy parameter of the expansion for Bianchi type-III metric is obtained in the presence of a single diagonal imperfect fluid with a dynamically anisotropic equation of state parameter and a dynamical energy density in general relativity.
Journal ArticleDOI

Bianchi Type-I Anisotropic Dark Energy Models with Constant Deceleration Parameter

TL;DR: In this article, the dark energy models in anisotropic Bianchi type-I (B-I) space-time with variable EoS parameter and constant deceleration parameter have been investigated.
Journal ArticleDOI

Bianchi Type-I Anisotropic Dark Energy Model with Constant Deceleration Parameter

TL;DR: In this article, a new dark energy model in anisotropic Bianchi type-I (B-I) space-time with time dependent equation of state (EoS) parameter and constant deceleration parameter was investigated.
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An interacting and non-interacting two-fluid scenario for dark energy in FRW universe with constant deceleration parameter

TL;DR: In this article, the evolution of the dark energy parameter within the scope of a spatially homogeneous and isotropic FRW universe filled with barotropic fluid and dark energy was studied.
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Anisotropic Bianchi Type-I String Cosmological Models in Normal Gauge for Lyra’s Manifold with Constant Deceleration Parameter

TL;DR: In this paper, a spatially homogeneous and anisotropic Bianchi type-I cosmological models representing massive strings in normal gauge for Lyra's manifold by applying the variation law for generalized Hubble's parameter that yields a constant value of deceleration parameter.
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