VARIABLE CHAPLYGIN GAS: CONSTRAINTS FROM CMBR ANDSNe Ia
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Publication:3430410
DOI10.1142/S0218271806008644zbMath1119.85305arXivastro-ph/0508491MaRDI QIDQ3430410
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Publication date: 21 March 2007
Published in: International Journal of Modern Physics D (Search for Journal in Brave)
Full work available at URL: https://arxiv.org/abs/astro-ph/0508491
Related Items (7)
Variable modified Chaplygin gas in anisotropic universe with Kaluza-Klein metric ⋮ LRS Bianchi type-I perfect fluid cosmological model with modified generalized chaplygin gas equation of state ⋮ A new variable modified Chaplygin gas model interacting with a scalar field ⋮ Gravitational collapse in higher dimensional Husain space-time ⋮ Viability of variable generalised Chaplygin gas: a thermodynamical approach ⋮ Density evolution in the new modified Chaplygin gas model ⋮ Thermodynamical behavior of the variable Chaplygin gas
Cites Work
- Unification of dark matter and dark energy: the inhomogeneous Chaplygin gas
- Density perturbations in a universe dominated by the Chaplygin gas
- Cosmological constant -- the weight of the vacuum
- Generalized Chaplygin gas as a unified scenario of dark matter/energy: Observational constraints
- BOUND ON THE TIME VARIATION OF THE FINE STRUCTURE CONSTANT DRIVEN BY QUINTESSENCE
- Constraints on alternative models to dark energy
- 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 cosmological constant problem
- An alternative to quintessence
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