Phantom appearance of non-phantom matter in Bianchi type-I cosmological model

DOI10.1007/s10773-012-1300-xzbMath1263.83200OpenAlexW1984190399MaRDI QIDQ1945621

R. Chaubey, Triloki Singh

Publication date: 8 April 2013

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

Full work available at URL: https://doi.org/10.1007/s10773-012-1300-x

zbMATH Keywords

cosmological modelsphantomcosmological parameters

Mathematics Subject Classification ID

Relativistic cosmology (83F05) Macroscopic interaction of the gravitational field with matter (hydrodynamics, etc.) (83C55) Exact solutions to problems in general relativity and gravitational theory (83C15)

Related Items (1)

Bianchi type I cosmological model with a cosmological constant \((\Lambda)\) in creation-field cosmology

Cites Work

• Dark energy with generalized equation of state in Bianchi type-I cosmological model
• Bianchi type-V cosmological models with perfect fluid and dark energy
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• Cosmological constant -- the weight of the vacuum
• ACCELERATING DARK ENERGY MODELS IN BIANCHI TYPE-V SPACETIME
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• FIELD THEORY OF TACHYON MATTER
• Cosmological Imprint of an Energy Component with General Equation of State
• The cosmological constant problem
• The Large Scale Structure of Space-Time
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• Cosmology with self-adjusting vacuum energy density from a renormalization group fixed point
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