Generalized Chaplygin gas dominated anisotropic Bianchi type-I cosmological models
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Publication:1013731
DOI10.1007/s10773-008-9781-3zbMath1163.85003OpenAlexW1972167159MaRDI QIDQ1013731
Publication date: 21 April 2009
Published in: International Journal of Theoretical Physics (Search for Journal in Brave)
Full work available at URL: https://doi.org/10.1007/s10773-008-9781-3
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) Astrophysical cosmology (85A40)
Related Items (2)
LRS Bianchi type-I perfect fluid cosmological model with modified generalized chaplygin gas equation of state ⋮ Statefinder diagnostic for variable modified Chaplygin gas in LRS Bianchi type I universe
Cites Work
- Holographic Chaplygin gas model
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- Density perturbations in a universe dominated by the Chaplygin gas
- Cardassian expansion: a model in which the universe is flat, matter dominated, and accelerating
- Cosmological constant -- the weight of the vacuum
- Bianchi type in universe with viscous fluid and a \(\Lambda\) term: a qualitative analysis
- The cosmological constant and dark energy
- RECONSTRUCTING DARK ENERGY
- A method for generating exact Bianchi type II cosmological models
- Role of modified Chaplygin gas in accelerated universe
- Cosmological Imprint of an Energy Component with General Equation of State
- The cosmological constant problem
- 4D gravity on a brane in 5D Minkowski space
- Generation of Bianchi type V universes filled with a perfect fluid
- An alternative to quintessence
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