Late time Acceleration and Role of Skewness in Anisotropic models

Abstract

We study cosmological models with anisotropy in expansion rates in the context of the recent observations predicting an accelerating universe. In the absence of any anisotropy in the cosmic fluid, it is shown that the role of skewness in directional Hubble rates is crucial in deciding the behavior of the model. We find that incorporation of skewness leads to a more evolving effective equation of state parameter.

arXiv comment15 pages, 4 figures, Astrophysics Space Science, 2014

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• Anisotropic cosmological reconstruction in $f(R,T)$ gravity
• Anisotropic solutions in f(R) Gravity
• Dark Energy Cosmological Models with General forms of Scale Factor
• Cosmological models with a Hybrid Scale Factor
• Unified Dark Fluid and Cosmic Transit Models in Brans-Dicke Theory
• Dynamical features of an anisotropic cosmological model
• Energy and momentum of Bianchi Type VI_h Universes
• Accelerating Dark Energy Cosmological Model in Two Fluid with Hybrid Scale Factor
• Role of Extended Gravity Theory in Matter Bounce Dynamics
• Cosmic Acceleration and Anisotropic models with Magnetic field
• Investigating the physical and geometrical parameters of the cosmological models with anisotropic background
• Stability, dark energy parameterization and swampland aspect of Bianchi Type-$V{I}_h$ cosmological models with f(R, T)-gravity
• Brane Viscous Cosmology in the Plasma Era
• Cosmological models with Big rip and Pseudo rip Scenarios in extended theory of gravity