Effects of Electromagnetic Field on the Dynamics of Bianchi type $V{I}_0$ Universe with Anisotropic Dark Energy

Abstract

Spatially homogeneous and anisotropic Bianchi type $V{I}_0$ cosmological models with cosmological constant are investigated in the presence of anisotropic dark energy. We examine the effects of electromagnetic field on the dynamics of the universe and anisotropic behavior of dark energy. The law of variation of the mean Hubble parameter is used to find exact solutions of the Einstein field equations. We find that electromagnetic field promotes anisotropic behavior of dark energy which becomes isotropic for future evolution. It is concluded that the isotropic behavior of the universe model is seen even in the presence of electromagnetic field and anisotropic fluid.

arXiv comment21 pages, 10 figures, accepted for publication in Int. J. Mod. Phys. D

References in corpus (25)

• Observational Evidence from Supernovae for an Accelerating Universe and a Cosmological Constant
• Measurements of Omega and Lambda from 42 High-Redshift Supernovae
• First Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Determination of Cosmological Parameters
• Wilkinson Microwave Anisotropy Probe (WMAP) Three Year Results: Implications for Cosmology
• The Cosmological Constant and Dark Energy
• First Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Preliminary Maps and Basic Results
• Cosmological Constant - the Weight of the Vacuum
• The Case for a Positive Cosmological Lambda-term
• The Cosmological Constant
• Discovery of a Supernova Explosion at Half the Age of the Universe and its Cosmological Implications
• Five-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Data Processing, Sky Maps, and Basic Results
• Measurements of the Cosmological Parameters Omega and Lambda from the First 7 Supernovae at z >= 0.35
• Can the dark energy equation-of-state parameter w be less than -1?
• Magnetic Fields in the Early Universe
• The 2dF Galaxy Redshift Survey: correlation functions, peculiar velocities and the matter density of the Universe
• The 2dF Galaxy Redshift Survey: The bias of galaxies and the density of the Universe
• Dark Matter and Dark Energy
• Bianchi type III models with anisotropic dark energy
• Accelerating Cosmologies with an Anisotropic Equation of State
• Homogeneous cosmologies with cosmological constant
• Exact Solutions of Bianchi Types $I$ and $V$ Spacetimes in $f(R)$ Theory of Gravity
• A Gauge-invariant Analysis of Magnetic Fields in General Relativistic Cosmology
• Gauge-invariant magnetic perturbations in perfect-fluid cosmologies
• Dynamics of a magnetized Bianchi I universe with vacuum energy
• Cosmological magnetic fields

Cited by in corpus (13)

• Anisotropic Universe Models in f(T) Gravity
• Anisotropic Fluid and Bianchi Type III Model in f(R) Gravity
• Thermodynamic Behavior of particular $f(R,T)$ Gravity Models
• Anisotropic Universe Models in Brans-Dicke Theory
• Non-vacuum Solutions of Bianchi Type VI_0 Universe in f(R) Gravity
• Bianchi type-I, type-III and Kantowski-Sachs solutions in f(T) gravity
• Generalized Second Law of Thermodynamic in Modified Teleparallel Theory
• Cosmological Evolution for Dark Energy Models in f(T) Gravity
• Anisotropic Dark Energy Bianchi Type III Cosmological Models in Brans Dicke Theory of Gravity
• Bianchi type II models in the presence of perfect fluid and anisotropic dark energy
• Anisotropic cosmology and inflation from tilted Bianchi IX model
• Thermodynamics in a Modified Gravity Involving Higher-Order Torsion Derivative Terms
• Some anisotropic universes in the presence of imperfect fluid coupling with spatial curvature