Interacting modified cosmic Chaplygin gas with variable cosmological constant and viscosity
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Publication:487434
DOI10.1007/S10773-014-2167-9zbMath1308.83182OpenAlexW1976586269MaRDI QIDQ487434
Publication date: 22 January 2015
Published in: International Journal of Theoretical Physics (Search for Journal in Brave)
Full work available at URL: https://doi.org/10.1007/s10773-014-2167-9
Cites Work
- Two-fluid dark energy models in Bianchi type-III universe with variable deceleration parameter
- Viscous varying generalized Chaplygin gas with cosmological constant and space curvature
- Generalized Chaplygin gas model with or without viscosity in the \(w\)-\(w^{\prime}\) plane
- An interacting and non-interacting two-fluid dark energy models in FRW universe with time dependent deceleration parameter
- Holographic dark energy model with interaction and cosmological constant in the flat space-time
- Effect of varying bulk viscosity on generalized Chaplygin gas
- Interacting new agegraphic viscous dark energy with varying \(G\)
- Holographic Chaplygin gas model
- Genesis of dark energy: Dark energy as consequence of release and two-stage tracking of cosmological nuclear energy
- Unification of dark matter and dark energy: the inhomogeneous Chaplygin gas
- Density perturbations in a universe dominated by the Chaplygin gas
- FRW cosmological model with modified Chaplygin gas and dynamical system
- Modified Chaplygin gas cosmology
- Viscous generalized Chaplygin gas with arbitrary \(\alpha\)
- Viscous Chaplygin gas in non-flat universe
- Interacting entropy-corrected holographic dark energy and IR cut-off length
- Dynamics of interacting generalized cosmic Chaplygin gas in brane-world scenario
- Interacting two-component fluid models with varying EoS parameter
- VISCOUS GENERALIZED CHAPLYGIN GAS
- Can an interacting varying Chaplygin gas and tachyonic matter accelerate universe?
- Role of modified Chaplygin gas in accelerated universe
- Generalized Chaplygin gas as a unified scenario of dark matter/energy: Observational constraints
- Measurements of Ω and Λ from 42 High‐Redshift Supernovae
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