Anisotropic solutions in f(R) Gravity

Abstract

Anisotropic cosmological models are investigated in the frame work of $f(R)$ gravity in the metric formalism. Plane symmetric models are considered to incorporate anisotropy in the expansion rates along different spatial directions. The anisotropy in expansion rates are assumed to be maintained throughout the cosmic evolution. Two accelerating models are constructed by considering different functional forms for f(R). The viability of these models are tested through a stability analysis.

15pages

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Cited by in corpus (12)

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• Traversable wormhole models in $f(R)$ gravity
• Gravitational baryogenesis models comparison in f(R) Gravity
• Dynamical features of an anisotropic cosmological model
• Dynamics of an Anisotropic Universe in $f(R,T)$ Theory
• Dynamics of Bianchi $V{I}_h$ Universe with Bulk Viscous Fluid in Modified Gravity
• f(R) wormholes embedded in a pseudo--Euclidean space $E^5$
• 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
• New symmetry in higher curvature spacetimes