Dark energy models in \(f(R,T)\) theory with variable deceleration parameter

DOI10.1007/s10773-015-2766-0zbMath1336.83015OpenAlexW2503021456MaRDI QIDQ264832

F. Blanchet-Sadri, M. Dambrine

Publication date: 1 April 2016

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

Full work available at URL: https://doi.org/10.1007/s10773-015-2766-0

zbMATH Keywords

dark energy\(f(R,T)\) gravity theoryBianchi type-II space-timeEoS parametermodified \(f(R,T)\) gravity theoryvariable deceleration parameter

Mathematics Subject Classification ID

Relativistic cosmology (83F05) Classes of solutions; algebraically special solutions, metrics with symmetries for problems in general relativity and gravitational theory (83C20) Relativistic gravitational theories other than Einstein's, including asymmetric field theories (83D05) Astrophysical cosmology (85A40)

Related Items (7)

Some Bianchi type-V accelerating cosmological models in f(R,T) = f1(R) + f2(T) formalism ⋮ Marder space-time with Tsallis holographic dark energy ⋮ The study of Bianchi type-III, V, and VI₀ models in modified theory ⋮ Transit cosmological models with domain walls in \(f(R,T)\) gravity ⋮ Various dark energy models for variables G and Λ in f(R, T) modified theory ⋮ Magnetized string cosmological models of accelerated expansion of the Universe in f(R,T) theory of gravity ⋮ Various dark energy models with time-varying G and Λ in f(R, T) gravitation theory

Cites Work

• Anisotropic viscous fluid cosmological models from deceleration to acceleration in string cosmology
• Dark energy model in anisotropic Bianchi type-III space-time with variable eos parameter
• Bianchi type-II string cosmological model with magnetic field in \(f(R,T)\) gravity
• Bianchi type-II dark energy model in \(f(R,T)\) gravity
• Bianchi type-I anisotropic dark energy model with constant deceleration parameter
• LRS Bianchi type I models with anisotropic dark energy and constant deceleration parameter
• Bianchi type III models with anisotropic dark energy
• Cosmological constant -- the weight of the vacuum
• Dark energy models with variable equation of state parameter
• Bianchi type III anisotropic dark energy models with constant deceleration parameter
• Measurements of Ω and Λ from 42 High‐Redshift Supernovae

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