Bulk viscous Bianchi type I cosmological models with time-dependent cosmological term \(\Lambda \)

DOI10.1007/s10773-008-9764-4zbMath1255.83096OpenAlexW2014080924MaRDI QIDQ1008284

J. Martínez

Publication date: 24 March 2009

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

Full work available at URL: https://doi.org/10.1007/s10773-008-9764-4

zbMATH Keywords

cosmological constanttime dependentBianchi Ibulk viscous

Mathematics Subject Classification ID

Relativistic cosmology (83F05) Relativistic gravitational theories other than Einstein's, including asymmetric field theories (83D05) Exact solutions to problems in general relativity and gravitational theory (83C15)

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Cites Work

• Unnamed Item
• Cosmological constant -- the weight of the vacuum
• The cosmological constant is back
• Some Bianchi type I viscous fluid cosmological models with a variable cosmological constant
• A model to explain varying \(\Lambda\), \(G\) and \(\sigma^{2}\) simultaneously
• 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
• The cosmological constant and dark energy
• Early viscous universe with variable gravitational and cosmological ‘constants’
• BULK VISCOUS ANISOTROPIC COSMOLOGICAL MODELS WITH VARIABLE G AND Λ
• BIANCHI TYPE I MAGNETOFLUID COSMOLOGICAL MODELS WITH VARIABLE COSMOLOGICAL CONSTANT REVISITED
• Dissipative cosmology
• THE COSMOLOGICAL CONSTANT PROBLEM
• Late-Time Mild Inflation: A Possible Solution of a Dilemma: The Cosmic Age and the Hubble Parameter
• Anisotropic cosmological models with spinor field and viscous fluid in the presence of a Λ term: qualitative solutions
• The cosmological constant problem
• BIANCHI TYPE I ANISOTROPIC MAGNETIZED COSMOLOGICAL MODELS WITH VARYING Λ
• BIANCHI TYPE I UNIVERSE WITH VISCOUS FLUID
• The Thermodynamics of Irreversible Processes. III. Relativistic Theory of the Simple Fluid

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