Dynamics of an anisotropic universe in \(f(R, T)\) theory
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Publication:2364284
DOI10.1155/2016/8543560zbMath1366.83082arXiv1607.03382OpenAlexW2474150335WikidataQ59121912 ScholiaQ59121912MaRDI QIDQ2364284
Sankarsan Tarai, B. Mishra, Sunil Kumar Tripathy
Publication date: 18 July 2017
Published in: Advances in High Energy Physics (Search for Journal in Brave)
Full work available at URL: https://arxiv.org/abs/1607.03382
Relativistic cosmology (83F05) Relativistic gravitational theories other than Einstein's, including asymmetric field theories (83D05)
Related Items (12)
Dynamics of an anisotropic universe in \(f(R, T)\) theory ⋮ A periodic varying deceleration parameter in f(R, T) gravity ⋮ Bouncing cosmological models in a functional form of \(F(R)\) gravity ⋮ Influence of modification of gravity on spherical wormhole models ⋮ Cosmic transit and anisotropic models in \(f(R, T)\) gravity ⋮ Phantom cosmology in an extended theory of gravity ⋮ \(f(R)\) gravity for a FLRW universe in a deformed phase space ⋮ Static traversable wormholes in \(f(R, T) = R + 2\alpha\ln T\) gravity ⋮ Dynamics of Bianchi V Ih universe with bulk viscous fluid in modified gravity ⋮ Cosmological models with a hybrid scale factor in an extended gravity theory ⋮ De Sitter and bounce solutions from anisotropy in extended gravity cosmology ⋮ Cosmological models with squared trace in modified gravity
Cites Work
- Kantowski-Sachs universe filled with perfect fluid in \(f(R,T)\) theory of gravity
- Modified Gauss-Bonnet theory as gravitational alternative for dark energy
- Exact solutions of Bianchi type \(V\) spacetime in \(f(R,T)\) gravity
- Dynamics of an anisotropic universe in \(f(R, T)\) theory
- Bianchi type-\(V\) cosmology in \(f(R,T)\) gravity with \(\varLambda (T)\)
- Evolution of the universe in inverse and \(\ln f(R)\) gravity
- A new class of Bianchi cosmological models in \(f(R,T)\) gravity
- RECONSTRUCTING f(R, T) GRAVITY FROM HOLOGRAPHIC DARK ENERGY
- INTRODUCTION TO MODIFIED GRAVITY AND GRAVITATIONAL ALTERNATIVE FOR DARK ENERGY
- Cosmological parameters from SDSS and WMAP
- Measurements of Ω and Λ from 42 High‐Redshift Supernovae
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