Bulk viscous Bianchi type V cosmological models with decaying cosmological term \(\Lambda \)

DOI10.1007/S10773-010-0466-3zbMath1205.83083OpenAlexW2048237982MaRDI QIDQ613634

Sumit K. Garg

Publication date: 21 December 2010

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

Full work available at URL: https://doi.org/10.1007/s10773-010-0466-3

zbMATH Keywords

cosmological modelsbulk viscosityBianchi space-timevariable cosmological term \(\Lambda\)

Mathematics Subject Classification ID

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) Exact solutions to problems in general relativity and gravitational theory (83C15)

Related Items (5)

Bianchi type V viscous fluid cosmological models with varying cosmological term ⋮ Late time isotropy viewed through Bianchi type I cosmological models with vacuum energy ⋮ Bianchi type V universe models with specific expansion anisotropy ⋮ Bulk viscosity and decaying vacuum density in Friedmann universe ⋮ LRS Bianchi I model with bulk viscosity in \(f(R,T)\) gravity

Cites Work

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• BIANCHI TYPE I MAGNETOFLUID COSMOLOGICAL MODELS WITH VARIABLE COSMOLOGICAL CONSTANT REVISITED
• Dissipative cosmology

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