Cosmological models with cubically varying deceleration parameter in \(f(R, T)\) gravity

DOI10.1007/S13370-022-00964-3zbMath1499.83028OpenAlexW4213311866MaRDI QIDQ2115663

M. Koussour, Mohamed Bennai

Publication date: 17 March 2022

Published in: Afrika Matematika (Search for Journal in Brave)

Full work available at URL: https://doi.org/10.1007/s13370-022-00964-3

zbMATH Keywords

dark energy\(f(R, T)\) gravityBianchi type-I spacetimevarying deceleration parameter

Mathematics Subject Classification ID

Relativistic cosmology (83F05) Relativistic gravitational theories other than Einstein's, including asymmetric field theories (83D05) Astrophysical cosmology (85A40)

Related Items (6)

Holographic dark energy in Gauss-Bonnet gravity with Granda-Oliveros cut-off ⋮ Stability analysis of anisotropic Bianchi type-I cosmological model in teleparallel gravity ⋮ Observational constraints on teleparallel effective equation of state ⋮ Flat FLRW Universe in logarithmic symmetric teleparallel gravity with observational constraints ⋮ Barrow holographic dark energy models in f(Q) symmetric teleparallel gravity with Lambert function distribution ⋮ Square-root parametrization of dark energy in \(f(Q)\) cosmology

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