Stability of viscous fluid in Bianchi type-VI model with cosmological constant

Abstract

In this paper, we investigate Bianchi type-$VI$ cosmological model for the universe filled with dark energy and viscous fluid in the presence of cosmological constant. Also, we show accelerating expansion of the universe by drawing volume scale, pressure and energy density versus cosmic time. In order to solve the Einstein field equations, we assume the expansion scalar is proportional to a component of the shear tensor. Therefore, we obtain the directional scale factors and show the EOS parameter crosses over phantom divided-line.

12 pages, 7 Postscript figures

References in corpus (3)

• f(R,T) gravity
• Interacting dark energy in $f(R)$ gravity
• Bianchi Type-I Anisotropic Dark Energy Models with Constant Deceleration Parameter

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• Thermodynamics and stability of $f(T,B)$ gravity with viscous fluid by observational constraints
• Observational constraints and stability in viscous $f(T,\mathcal{T})$ gravity
• Extended Bose-Einstein condensate dark matter in viscous Gauss-Bonnet gravity
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• Viscous interacting and stability on dark matter Bose-Einstein condensation with modified Chaplygin gas
• The Hubble IR cutoff in holographic ellipsoidal cosmologies