The cosmology in f(R,τ) gravity without dark energy

DOI10.1142/S0218271816500383zbMath1336.83038arXiv1510.01061OpenAlexW3103091523MaRDI QIDQ2806280

Gang Sun, Yong-Chang Huang

Publication date: 17 May 2016

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

Full work available at URL: https://arxiv.org/abs/1510.01061

zbMATH Keywords

dark energy\(f(R,\tau)\) gravitylate-time cosmic acceleration

Mathematics Subject Classification ID

Relativistic cosmology (83F05) Relativistic gravitational theories other than Einstein's, including asymmetric field theories (83D05) Observational and experimental questions in relativity and gravitational theory (83B05)

Related Items (7)

Conformally symmetric Friedmann–Robertson–Walker metric in f(R,T) gravity ⋮ \(H_0\) tension in torsion-based modified gravity ⋮ Dynamical variables and evolution of the universe ⋮ Interpretation of f(R,T) gravity in terms of a conserved effective fluid ⋮ Measure of complexity for dynamical self-gravitating structures ⋮ Constraining \(f(R,T)\) gravity from the dark energy density parameter \(\Omega_{\Lambda} \) ⋮ Stability of anisotropic perturbed Einstein universe in f(R,T) theory

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