Dark energy with generalized equation of state in Bianchi type-I cosmological model

DOI10.1007/S10773-011-0881-0zbMath1242.83138OpenAlexW2060842383MaRDI QIDQ432024

R. Chaubey, Triloki Singh

Publication date: 3 July 2012

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

Full work available at URL: https://doi.org/10.1007/s10773-011-0881-0

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) Hydrodynamic and hydromagnetic problems in astronomy and astrophysics (85A30) Astrophysical cosmology (85A40)

Related Items (2)

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

Cites Work

• Unnamed Item
• Cardassian expansion: a model in which the universe is flat, matter dominated, and accelerating
• Perfect fluids satisfying a less than extremely relativistic equation of state
• DYNAMICS OF DARK ENERGY
• Measurements of Ω and Λ from 42 High‐Redshift Supernovae
• Cosmological Imprint of an Energy Component with General Equation of State
• 4D gravity on a brane in 5D Minkowski space
• \(k\)-inflation

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