Kantowski-Sachs universe filled with perfect fluid in \(f(R,T)\) theory of gravity
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Publication:379306
DOI10.1007/s10773-013-1556-9zbMath1308.83141OpenAlexW2051830030MaRDI QIDQ379306
Publication date: 11 November 2013
Published in: International Journal of Theoretical Physics (Search for Journal in Brave)
Full work available at URL: https://doi.org/10.1007/s10773-013-1556-9
Relativistic cosmology (83F05) Macroscopic interaction of the gravitational field with matter (hydrodynamics, etc.) (83C55) Relativistic gravitational theories other than Einstein's, including asymmetric field theories (83D05)
Related Items (16)
Dynamics of an anisotropic universe in \(f(R, T)\) theory ⋮ Geometry of the universe described by wet dark fluid in \(f(R, T)\) theory of gravity ⋮ Cosmology of Tsallis and Kaniadakis holographic dark energy in Saez-Ballester theory and consideration of viscous van der Waals fluid ⋮ Cosmology in modified f(R,T)-gravity theory in a variant Λ(T) scenario-revisited ⋮ Imperfect fluid cosmological model in modified gravity ⋮ Static traversable wormholes in \(f(R, T) = R + 2\alpha\ln T\) gravity ⋮ FRW cosmology in f(Q,T) gravity ⋮ Traversable wormholes with exponential shape function in modified gravity and general relativity: A comparative study ⋮ Exact Kantowski-Sachs anisotropic dark energy cosmological models in Brans Dicke theory of gravitation ⋮ FRW cosmology in f(R,T) gravity ⋮ A note on some perfect fluid Kantowski–Sachs and Bianchi type III spacetimes and their conformal vector fields in f(R) theory of gravity ⋮ Cosmological models with a hybrid scale factor in an extended gravity theory ⋮ Binary mixture of perfect fluid and dark energy in modified theory of gravity ⋮ Wormhole modeling supported by non-exotic matter ⋮ Kantowski-Sachs ghost dark energy cosmological model with specific Hubble parameter in \(f(R,T)\) gravity ⋮ Dark energy in spherically symmetric universe coupled with Brans-Dicke scalar field
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