Hybrid expansion law for dark energy dominated universe in \(f(R,T)\) gravity

DOI10.1007/S10773-014-2368-2zbMath1327.83240OpenAlexW2027494716MaRDI QIDQ890366

N. E. Zubov

Publication date: 10 November 2015

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

Full work available at URL: https://doi.org/10.1007/s10773-014-2368-2

zbMATH Keywords

early universe\(f(R,T)\) gravity and cosmological parameters

Mathematics Subject Classification ID

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

Related Items (7)

Barrow holographic dark energy with hybrid expansion law ⋮ Bianchi-III transitioning space-time in a nonsingular hybrid universe within Lyra's cosmology ⋮ Barrow holographic dark energy in Bianchi-I universe with k-essence ⋮ Lyra’s cosmology of homogeneous and isotropic universe in Brans–Dicke theory ⋮ Non-minimal matter-geometry coupling in the Bianchi-V spacetime within the formalism of f(R, T) = f₁(R) + f₂(R)f₃(T) cosmology ⋮ Transit dark energy string cosmological models with perfect fluid in F(R,T)-gravity ⋮ Bulk viscous Bianchi-I embedded cosmological model in f(R,T) = f1(R) + f2(R)f3(T) gravity

Cites Work

• Dissipative future universe without big rip
• Kaluza-Klein cosmological model in \(f(R,T)\) gravity
• Bianchi type-\(V\) cosmology in \(f(R,T)\) gravity with \(\varLambda (T)\)
• Acceleration of the universe in the Einstein frame of a metric-affine f ( R ) gravity
• RECONSTRUCTION OF f(R, T) GRAVITY DESCRIBING MATTER DOMINATED AND ACCELERATED PHASES
• Measurements of Ω and Λ from 42 High‐Redshift Supernovae

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