AbstractIn this Letter, a modified Chaplygin gas (MCG) model of unifying dark energy and dark matter with the exotic equation of state pMCG=BρMCG−AρMCGα is constrained from recently observed data: the 182 Gold SNe Ia, the 3-year WMAP and the SDSS baryon acoustic peak. It is shown that the best fit value of the three parameters (B,Bs,α) in MCG model are (−0.085,0.822,1.724). Furthermore, we find the best fit w(z) crosses −1 in the past and the present best fit value w(0)=−1.114<−1, and the 1σ confidence level of w(0) is −0.946⩽w(0)⩽−1.282. Finally, we find that the MCG model has the smallest χmin2 value in all eight given models. According to the Akaike Information Criterion (AIC) of model selection, we conclude that recent observational dat...
In this paper, we use the latest observations of quasars covering the redshift range of $$0.04<z<5.1...
With considerations of the recently released WMAP year three and supernova legacy survey (SNLS) data...
Using various latest cosmological datasets including Type-Ia supernovae, cosmic microwave background...
AbstractIn this Letter, a modified Chaplygin gas (MCG) model of unifying dark energy and dark matter...
AbstractThe Modified Chaplygin Gas (MCG) model belongs to the class of a unified models of dark ener...
We examine observational constraints on the generalized Chaplygin gas (GCG) model for dark energy fr...
We investigate observational constraints on the generalized Chaplygin gas (GCG) model as the unifica...
A modified Chaplygin gas model (MCG), ρ MCG/ρ MCG0=[B s +(1−B s )a −3(1+B)(1+α)]1/(1+α), as a unif...
The generalized Chaplygin gas (GCG), is studied in this paper by using the latest observational data...
We investigate the cosmological constraints on the Variable Chaplygin gas model from the latest obse...
We investigate the cosmological constraints on the Variable Chaplygin gas model from the latest obse...
AbstractThe Modified Chaplygin Gas (MCG) model belongs to the class of a unified models of dark ener...
We have assumed FRW model of the universe in Einstein-Aether gravity filled with dark matter and mod...
The modified Chaplygin gas could be considered to abide by the unified dark fluid model because the ...
AbstractThe generalized Chaplygin gas (GCG) model explains the recent accelerated expansion of the U...
In this paper, we use the latest observations of quasars covering the redshift range of $$0.04<z<5.1...
With considerations of the recently released WMAP year three and supernova legacy survey (SNLS) data...
Using various latest cosmological datasets including Type-Ia supernovae, cosmic microwave background...
AbstractIn this Letter, a modified Chaplygin gas (MCG) model of unifying dark energy and dark matter...
AbstractThe Modified Chaplygin Gas (MCG) model belongs to the class of a unified models of dark ener...
We examine observational constraints on the generalized Chaplygin gas (GCG) model for dark energy fr...
We investigate observational constraints on the generalized Chaplygin gas (GCG) model as the unifica...
A modified Chaplygin gas model (MCG), ρ MCG/ρ MCG0=[B s +(1−B s )a −3(1+B)(1+α)]1/(1+α), as a unif...
The generalized Chaplygin gas (GCG), is studied in this paper by using the latest observational data...
We investigate the cosmological constraints on the Variable Chaplygin gas model from the latest obse...
We investigate the cosmological constraints on the Variable Chaplygin gas model from the latest obse...
AbstractThe Modified Chaplygin Gas (MCG) model belongs to the class of a unified models of dark ener...
We have assumed FRW model of the universe in Einstein-Aether gravity filled with dark matter and mod...
The modified Chaplygin gas could be considered to abide by the unified dark fluid model because the ...
AbstractThe generalized Chaplygin gas (GCG) model explains the recent accelerated expansion of the U...
In this paper, we use the latest observations of quasars covering the redshift range of $$0.04<z<5.1...
With considerations of the recently released WMAP year three and supernova legacy survey (SNLS) data...
Using various latest cosmological datasets including Type-Ia supernovae, cosmic microwave background...