Constraining \(f(R,T)\) gravity from the dark energy density parameter \(\Omega_{\Lambda} \)

DOI10.1134/S0202289320030032zbMath1454.83088arXiv1908.06759OpenAlexW3105496780MaRDI QIDQ2215233

P. K. Sahoo, Snehasish Bhattacharjee

Publication date: 11 December 2020

Published in: Gravitation \& Cosmology (Search for Journal in Brave)

Full work available at URL: https://arxiv.org/abs/1908.06759

zbMATH Keywords

dark energy\(f(R)\) gravity

Mathematics Subject Classification ID

Relativistic gravitational theories other than Einstein's, including asymmetric field theories (83D05) Astrophysical cosmology (85A40) Dark matter and dark energy (83C56)

Related Items (2)

Dark energy nature in logarithmic f(R,T) cosmology ⋮ Radial oscillations and stability of compact stars in f(R, T) = R+ 2β T gravity

Cites Work

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• Wormhole geometries in \(f(R,T)\) gravity
• Propagation of polar gravitational waves in \(f(R, T)\) scenario
• Exact solutions of Bianchi type \(V\) spacetime in \(f(R,T)\) gravity
• The cosmology in f(R,τ) gravity without dark energy
• DYNAMICS OF DARK ENERGY
• A periodic varying deceleration parameter in f(R, T) gravity
• RECONSTRUCTION OF f(R, T) GRAVITY DESCRIBING MATTER DOMINATED AND ACCELERATED PHASES
• Phantom fluid supporting traversable wormholes in alternative gravity with extra material terms
• Analytical general solutions for static wormholes inf(R,T) gravity
• Charged wormholes in f(R,T)-extended theory of gravity
• Measurements of Ω and Λ from 42 High‐Redshift Supernovae

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