Viscous fluid cosmology in Bianchi type-I space-time

DOI10.1007/s10773-008-9865-0zbMath1171.83384OpenAlexW2003204911MaRDI QIDQ2390799

C. P. Singh, Suresh K. Kumar

Publication date: 10 August 2009

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

Full work available at URL: https://doi.org/10.1007/s10773-008-9865-0

zbMATH Keywords

cosmological modelsHubble parameterviscous fluiddeceleration parameter

Mathematics Subject Classification ID

Relativistic cosmology (83F05) Macroscopic interaction of the gravitational field with matter (hydrodynamics, etc.) (83C55)

Related Items (9)

A new class of Bianchi type-I cosmological models in Lyra geometry ⋮ Bulk viscous Bianchi type-V cosmological models with variable gravitational and cosmological constant ⋮ Bulk viscous LRS Bianchi-I universe with variable \(G\) and decaying \(\Lambda \) ⋮ On a Bianchi type-I space-time with bulk viscosity in f(R,T) gravity ⋮ String cosmology with magnetized bulk viscous fluid in Bianchi I universe ⋮ Bianchi type-III bulk viscous and barotropic perfect fluid cosmological models in Lyra's geometry ⋮ Anisotropic dark energy models with constant deceleration parameter ⋮ LRS Bianchi I model with bulk viscosity in \(f(R,T)\) gravity ⋮ Anisotropic cosmological models in f(R,T) gravity with variable deceleration parameter

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