Anisotropic cosmological reconstruction in $f(R,T)$ gravity

Abstract

Anisotropic cosmological models are constructed in $f(R,T)$ gravity theory to investigate the dynamics of universe concerning the late time cosmic acceleration. Using a more general and simple approach, the effect of the coupling constant and anisotropy on the cosmic dynamics have been investigated. Cosmic anisotropy is found affect substantially the cosmic dynamics.

7 pages, 3 figures

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Cited by in corpus (18)

• Wormholes in exponential $f(R,T)$ gravity
• Existence of bulk viscous universe in $f(R,T)$ gravity and confrontation with observational data
• Phantom cosmology in an Extended Theory of Gravity
• Anisotropic stars in modified gravity: An extended gravitational decoupling approach
• Bouncing Models in an Extended Gravity Theory
• Reconstruction and Stability Analysis of Some Cosmological Bouncing Solutions in $F(\mathcal{R},T)$ Theory
• Bouncing cosmology in extended gravity and its reconstruction as dark energy model
• Rip cosmologies, Wormhole Solutions and Big Trip in the $f(T,\mathcal{T})$ theory of gravity
• Role of Extended Gravity Theory in Matter Bounce Dynamics
• 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
• Bouncing cosmological model with general relativistic hydrodynamics in extended gravity
• Dynamical Wormhole Solutions in $f(R,T)$ Gravity
• Cosmological models with Big rip and Pseudo rip Scenarios in extended theory of gravity
• Dynamics of quasi de Sitter and linear combination of exponential models in extended gravity