ANISOTROPIC BIANCHI-V PERFECT FLUID SPACE–TIME WITH VARIABLES G AND Λ

DOI10.1142/S0217751X10050123zbMath1194.83050MaRDI QIDQ3590709

C. P. Singh, Aroonkumar Beesham

Publication date: 13 September 2010

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

zbMATH Keywords

cosmological constantHubble parameterdeceleration parametergravitational constant

Mathematics Subject Classification ID

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

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Cites Work

• A critical density cosmological model with varying gravitational and cosmological ``constants
• Static universe in a modified Brans-Dicke cosmology
• Bianchi type I cosmological models with variable \(G\) and \(\Lambda\)
• Cosmological constant -- the weight of the vacuum
• Bianchi type I cosmological models with variable \(G\) and \(\Lambda\): A comment
• Anisotropic cosmological models with a perfect fluid and a \(\Lambda\) term
• Bianchi type in universe with viscous fluid and a \(\Lambda\) term: a qualitative analysis
• DIRAC SPINOR IN BIANCHI-I UNIVERSE WITH TIME-DEPENDENT GRAVITATIONAL AND COSMOLOGICAL CONSTANTS
• Some FRW models with variable G and
• 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
• The Cosmological Constants

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