Non-minimal matter-geometry coupling in the Bianchi-V spacetime within the formalism of f(R, T) = f1(R) + f2(R)f3(T) cosmology

DOI10.1142/S0217732318502346zbMath1405.83045OpenAlexW2900635613MaRDI QIDQ4612167

Vinod K. Bhardwaj

Publication date: 22 January 2019

Published in: Modern Physics Letters A (Search for Journal in Brave)

Full work available at URL: https://doi.org/10.1142/s0217732318502346

zbMATH Keywords

\(f(R, T)\) gravityBianchi type-V spacetimematter-geometry coupling

Mathematics Subject Classification ID

Relativistic cosmology (83F05) Einstein's equations (general structure, canonical formalism, Cauchy problems) (83C05) Relativistic gravitational theories other than Einstein's, including asymmetric field theories (83D05)

Related Items (2)

Some Bianchi type-V accelerating cosmological models in f(R,T) = f1(R) + f2(T) formalism ⋮ Bianchi type-V transitioning model in Brans–Dicke theory with observational constraints

Cites Work

• \(f(R)\) theories
• Anisotropic dark energy models with constant deceleration parameter
• LRS Bianchi type I models with anisotropic dark energy and constant deceleration parameter
• Hybrid expansion law for dark energy dominated universe in \(f(R,T)\) gravity
• Energy conditions in \(F(T,\varTheta)\) gravity and compatibility with a stable de Sitter solution
• Non-vacuum static cylindrically symmetric solution and energy distribution in \(f(R)\) gravity
• Influence of modification of gravity on spherical wormhole models

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