LRS Bianchi type-I perfect fluid cosmological model with modified generalized chaplygin gas equation of state

DOI10.1007/s10509-010-0508-6zbMath1237.83040OpenAlexW2059470016MaRDI QIDQ416160

Abdussattar, S. R. Prajapati

Publication date: 9 May 2012

Published in: Astrophysics and Space Science (Search for Journal in Brave)

Full work available at URL: https://doi.org/10.1007/s10509-010-0508-6

zbMATH Keywords

Chaplygin gasDark energyCosmic accelerationLRS Bianchi type-I space-time

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 (6)

Interacting holographic dark energy in Bianchi type-V and IX universes with variable deceleration parameter ⋮ Plane symmetric solutions to the Einstein's field equations with dark energy ⋮ Reconstruction of cosmic history from a simple parametrization of H ⋮ Two fluids tilted cosmological models in general relativity ⋮ Tilted universe with big rip singularity in Lyra geometry ⋮ LRS Bianchi type I magnetized cosmological model with perfect fluid and with quintessence, Chaplygin gas dark energy in bimetric theory of gravitation

Cites Work

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