Spatially homogeneous Bianchi type-I universes with variable \(G\) and \(\Lambda \)

DOI10.1007/s10773-013-1678-0zbMath1274.83039OpenAlexW1967061757MaRDI QIDQ379417

Mohammad Hasan, H. S. Yoon

Publication date: 11 November 2013

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

Full work available at URL: https://doi.org/10.1007/s10773-013-1678-0

zbMATH Keywords

cosmological constantbulk viscosityBianchi type space-timegravitational constant

Mathematics Subject Classification ID

Classes of solutions; algebraically special solutions, metrics with symmetries for problems in general relativity and gravitational theory (83C20)

Related Items (7)

Magnetized emergent universe with null radiation flow ⋮ Bianchi type-III magnetized string cosmological models for perfect fluid distribution in \(f(R,T)\) gravity ⋮ Generalized holographic Ricci dark energy and generalized second law of thermodynamics in Bianchi type I universe ⋮ Modified Chaplygin gas cosmology with observational constraints ⋮ Unnamed Item ⋮ Bianchi type-I cosmological models for integral representation formula and some solutions in spacetime ⋮ Bianchi type-III cosmological models in Lyra's geometry in the presence of massive scalar field

Cites Work

• Unnamed Item
• Unnamed Item
• FRW cosmology with variable \(G\) and \(\Lambda \)
• Cosmological models with variable cosmological and gravitational ``constants and bulk viscous models
• Viscous inflationary universe models
• Bianchi-I space-time with variable gravitational and cosmological ``constants
• Hypersurface-homogeneous bulk viscous fluid space-times with time-dependent cosmological term
• Bianchi type I cosmological models with variable \(G\) and \(\Lambda\)
• Plane-symmetric mesonic viscous fluid cosmological model
• Bianchi type IX string cosmological models with bulk viscous fluid in general relativity
• Cosmological models with variable G and \(\Lambda\)
• Anisotropic viscous cosmology with variable \(G\) and \(\Lambda\)
• Some spatially homogeneous string cosmological models
• Anisotropic cosmological models with bulk viscosity for variable \(G\) and \(\Lambda\)
• Anisotropic cosmological model with variable G and \(\varLambda\)
• Some Bianchi type III string cosmological models with bulk viscosity
• Anisotropic cosmological models with perfect fluid and dark energy reexamined
• Mach's Principle and a Relativistic Theory of Gravitation
• Early viscous universe with variable gravitational and cosmological ‘constants’
• BIANCHI TYPE I UNIVERSES WITH CAUSAL BULK VISCOUS COSMOLOGICAL FLUID
• Canonical measure and the flatness of a FRW universe
• Bulk Viscosity and Particle Creation in Brans - Dicke Theory
• A new theory of gravitation
• 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
• A new basis for cosmology
• The Thermodynamics of Irreversible Processes. III. Relativistic Theory of the Simple Fluid

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