Bulk viscous Bianchi type-III cosmological model with time-dependent \(G\) and \(\Lambda \)

DOI10.1007/S10773-010-0248-YzbMath1190.83131OpenAlexW1990367288MaRDI QIDQ975717

B. E. Eshmatov

Publication date: 11 June 2010

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

Full work available at URL: https://doi.org/10.1007/s10773-010-0248-y

zbMATH Keywords

bulk viscosityvariable \(G\) and \(\Lambda \)Bianchi-III

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 (3)

Energy conditions for inhomogeneous EOS and its thermodynamics analysis with the resolution on finite time future singularity problems ⋮ Anisotropic Bianchi type-III bulk viscous fluid universe in Lyra geometry ⋮ Anisotropic bulk viscous fluid cosmological model with zero-rest-mass scalar field and time-dependent cosmological term

Cites Work

• Cosmological models with variable cosmological and gravitational ``constants and bulk viscous models
• The inflationary Kantowski-Sachs cosmological model in general relativity
• The cosmological constant is back
• Anisotropic bulk viscous cosmological models with variable \(G\) and \(\Lambda \)
• LRS Bianchi type II bulk viscous fluid universe with decaying vacuum energy density \(\Lambda \)
• A model to explain varying \(\Lambda\), \(G\) and \(\sigma^{2}\) simultaneously
• Early viscous universe with variable gravitational and cosmological ‘constants’
• Some FRW models with variable G and
• Dissipative cosmology
• THE COSMOLOGICAL CONSTANT PROBLEM
• Measurements of Ω and Λ from 42 High‐Redshift Supernovae
• Type Ia Supernova Discoveries atz> 1 from theHubble Space Telescope: Evidence for Past Deceleration and Constraints on Dark Energy Evolution
• The cosmological constant problem

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