On a Bianchi type-I space-time with bulk viscosity in f(R,T) gravity

DOI10.1142/S0219887822500384OpenAlexW4200381374MaRDI QIDQ6196405

Mohamed Bennai, M. Koussour

Publication date: 14 March 2024

Published in: International Journal of Geometric Methods in Modern Physics (Search for Journal in Brave)

Full work available at URL: https://doi.org/10.1142/s0219887822500384

zbMATH Keywords

bulk viscosityenergy conditionsBianchi model\(f(R, T)\) gravity

Mathematics Subject Classification ID

Relativistic cosmology (83F05) Macroscopic interaction of the gravitational field with matter (hydrodynamics, etc.) (83C55) Relativistic gravitational theories other than Einstein's, including asymmetric field theories (83D05)

Related Items (3)

Observational constraints on teleparallel effective equation of state ⋮ Square-root parametrization of dark energy in \(f(Q)\) cosmology ⋮ A model-independent method with phantom divide line crossing in Weyl-type \(f(Q, T)\) gravity

Cites Work

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• Effective field theory from modified gravity with massive modes
• Anisotropic cosmological models in f(R,T) gravity with variable deceleration parameter
• The Large Scale Structure of Space-Time
• General Relativity
• An alternative to quintessence

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