Dynamical features of an anisotropic cosmological model

Abstract

The dynamical features of Bianchi type $V{I}_h$ $(BV{I}_h)$ universe are investigated in $f(R,T)$ theory of gravity. The field equations and the physical properties of the model are derived considering a power law expansion of the universe. The effect of anisotropy on the dynamics of the universe as well on the energy conditions are studied. The assumed anisotropy of the model is found to have substantial effects on the energy condition and dynamical parameters.

11 pages, 7 figures

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• Accelerating models with a hybrid scale factor in extended gravity
• Cosmological models with squared trace in modified gravity
• 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
• Magnetized cosmological model with variable deceleration parameter
• Bouncing cosmological models in a functional form of F(R) gravity
• Cosmological models with Big rip and Pseudo rip Scenarios in extended theory of gravity