Bulk viscous cosmological models with variable \(G\) and \(\Lambda\)

DOI10.1023/A:1018866107585zbMath0915.53049MaRDI QIDQ1289182

W. S. Mbokazi, Tarkeshwar Singh, Aroonkumar Beesham

Publication date: 12 July 1999

Published in: General Relativity and Gravitation (Search for Journal in Brave)

zbMATH Keywords

bulk viscosityvariable cosmological constantvariable gravitational constant

Mathematics Subject Classification ID

Relativistic cosmology (83F05) Applications of differential geometry to physics (53Z05)

Related Items (16)

Perfect fluid Bianchi I model with variable \(G\) and \(\Lambda \) ⋮ Anisotropic bulk viscous cosmological models with variable \(G\) and \(\Lambda \) ⋮ BIANCHI I WITH VARIABLE G AND Λ: SELF-SIMILAR APPROACH ⋮ Anisotropic cosmological models with bulk viscosity for variable \(G\) and \(\Lambda\) ⋮ Particle creation in cosmological models with varying gravitational and cosmological constants ⋮ Laboratory bounds for the cosmological term gradient ⋮ FULL CAUSAL BULK VISCOUS COSMOLOGIES WITH TIME-VARYING CONSTANTS ⋮ PERFECT FLUID COSMOLOGICAL MODELS WITH TIME-VARYING CONSTANTS ⋮ About Bianchi I with VSL ⋮ FRW cosmology with variable \(G\) and \(\Lambda \) ⋮ Higher dimensional cosmological model with gravitational and cosmological constants ⋮ Bianchi II with time varying constants. Self-similar approach ⋮ Viscous cosmology for early- and late-time universe ⋮ Anisotropic viscous cosmology with variable \(G\) and \(\Lambda\) ⋮ Causal viscous cosmological models with variable \(G\) and \(\Lambda\) ⋮ Causal dissipative cosmology with variable \(G\) and \(\lambda\)

Cites Work

• Cosmological models with variable cosmological and gravitational ``constants and bulk viscous models
• Viscous inflationary universe models
• A critical density cosmological model with varying gravitational and cosmological ``constants
• Static universe in a modified Brans-Dicke cosmology
• Variable-G cosmology and creation
• Cosmological models with variable gravitational and cosmological ``constants
• The cosmological constant is back
• Some FRW models with variable G and
• THE COSMOLOGICAL CONSTANT PROBLEM
• Late-Time Mild Inflation: A Possible Solution of a Dilemma: The Cosmic Age and the Hubble Parameter
• The cosmological constant problem
• The Cosmological Constants

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