Cosmological evolution of modified Chaplygin gas with the sign-changeable interactions
From MaRDI portal
Publication:1930595
DOI10.1007/s10773-012-1224-5zbMath1255.83109OpenAlexW2058658753MaRDI QIDQ1930595
Publication date: 11 January 2013
Published in: International Journal of Theoretical Physics (Search for Journal in Brave)
Full work available at URL: https://doi.org/10.1007/s10773-012-1224-5
Relativistic cosmology (83F05) Space-time singularities, cosmic censorship, etc. (83C75) Macroscopic interaction of the gravitational field with matter (hydrodynamics, etc.) (83C55) Relativistic gravitational theories other than Einstein's, including asymmetric field theories (83D05) Exact solutions to problems in general relativity and gravitational theory (83C15)
Related Items
Effects of anisotropy on the sign-changeable interacting Tsallis holographic dark energy ⋮ Statefinder diagnostic for modified Chaplygin gas with the sign-changeable interaction ⋮ Ghost dark energy with sign-changeable interaction term
Cites Work
- Generalized Chaplygin gas model with or without viscosity in the \(w\)-\(w^{\prime}\) plane
- Cosmological evolution of quintessence and phantom with a new type of interaction in dark sector
- Interacting holographic dark energy model in non-flat universe
- Interacting dark energy with inhomogeneous equation of state
- Unification of dark matter and dark energy: the inhomogeneous Chaplygin gas
- Statefinder diagnostic in generalized Chaplygin gas model with and without viscosity
- Cosmological Constraints on the Sign-Changeable Interactions
- DYNAMICAL EVOLUTION OF INTERACTING MODIFIED CHAPLYGIN GAS
- DYNAMICS OF DARK ENERGY
- VISCOUS GENERALIZED CHAPLYGIN GAS
- Role of modified Chaplygin gas in accelerated universe
- Interacting generalized Chaplygin gas
- COSMOLOGICAL EVOLUTION OF MODIFIED CHAPLYGIN GAS INTERACTING WITH BAROTROPIC BACKGROUND FLUID
- Measurements of Ω and Λ from 42 High‐Redshift Supernovae
- Type Ia Supernova Discoveries atz> 1 from theHubble Space Telescope: Evidence for Past Deceleration and Constraints on Dark Energy Evolution
- The heteroclinic orbit and tracking attractor in a cosmological model with a double exponential potential
- An alternative to quintessence
- Interacting quintessence
