Anisotropic viscous fluid cosmological models from deceleration to acceleration in string cosmology
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Publication:379264
DOI10.1007/S10773-013-1540-4zbMath1309.83057OpenAlexW2109782359MaRDI QIDQ379264
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/s10773-013-1540-4
Relativistic cosmology (83F05) Macroscopic interaction of the gravitational field with matter (hydrodynamics, etc.) (83C55)
Related Items (6)
Dark energy models in \(f(R,T)\) theory with variable deceleration parameter ⋮ Study of Frw Type Kaluza-Klein Domain Wall Cosmological Models in the Presence of Massive Scalar Field in a Modified Gravity ⋮ Marder space-time with Tsallis holographic dark energy ⋮ Viscous cosmology and thermodynamics of apparent horizon in modified Friedman-Robertson-Walkers universe ⋮ Induced equation of state for the universe epochs constrained by the Hubble parameter ⋮ Bianchi type-I string dust models with bulk viscosity in Lyra geometry
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