LRS Bianchi type II bulk viscous fluid universe with decaying vacuum energy density \(\Lambda \)

DOI10.1007/s10773-008-9918-4zbMath1171.83382arXiv0805.3469OpenAlexW1971867433MaRDI QIDQ2390868

Anirudh Pradhan, Shyam Sundar Kumhar

Publication date: 10 August 2009

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

Full work available at URL: https://arxiv.org/abs/0805.3469

zbMATH Keywords

cosmological constantbulk viscous fluidLRS Bianchi type II

Mathematics Subject Classification ID

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

Related Items (11)

Late time isotropy viewed through Bianchi type I cosmological models with vacuum energy ⋮ Bulk viscous fluid hypersurface-homogeneous cosmological models with time varying G and \(\Lambda \) ⋮ Bianchi type V universe models with specific expansion anisotropy ⋮ Anisotropic bulk viscous fluid cosmological model with zero-rest-mass scalar field and time-dependent cosmological term ⋮ Bianchi type V viscous fluid cosmological models in presence of decaying vacuum energy ⋮ Anisotropic Bianchi type-I and type-II bulk viscous string cosmological models coupled with zero mass scalar field ⋮ Non-existence of a massive scalar field for the Marder universe in Lyra and Riemannian geometries ⋮ Dark energy models in LRS Bianchi type-II space-time in the new perspective of time-dependent deceleration parameter ⋮ Magnetized string cosmology in anisotropic Bianchi-II space-time with variable cosmological term-\(\Lambda\) ⋮ Hypersurface-homogeneous bulk viscous fluid space-times with time-dependent cosmological term ⋮ Bulk viscous Bianchi type-III cosmological model with time-dependent \(G\) and \(\Lambda \)

Cites Work

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