Bayesian analysis of the (generalized) Chaplygin gas and cosmological constant models using the 157 gold SNe Ia data

被引:53
作者
Colistete, R [1 ]
Fabris, JC [1 ]
机构
[1] Univ Fed Espirito Santo, Dept Fis, BR-29060900 Vitoria, Espirito Santo, Brazil
关键词
D O I
10.1088/0264-9381/22/14/001
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
The generalized Chaplygin gas model (GCGM) contains five free parameters that must be constrained using the different observational data. These parameters are: the Hubble constant H-0, the parameter (A) over bar related to the sound velocity, the equation of state parameter alpha, the curvature parameter Omega(k0) and the Chaplygin gas density parameter Omega(c0). The pressureless matter parameter Omega(k0) may be obtained as a dependent quantity. Here, these parameters are constrained through the type Ia supernovae data. The 'gold sample' of 157 supemovae data is used. Negative and large positive values for alpha are taken into account. The analysis is made by employing the Bayesian statistics and the prediction for each parameter is obtained by marginalizing on the remaining ones. This procedure leads to the following predictions: alpha = -0.75(-0.24)(+4.04), H-0 = 65.00(-1.75)(+1.77), Omega(k0) = -0.77(-5.94)(+1.14), Omega(m0) = 0.00(-0.00)(+1,95), Omega(c0) = 1.36(-0.85)(+5.36), (A) over bar = 1.000(-0.534)(+0-000). Through the same analysis the specific case of the ordinary Chaplygin gas model (CGM), for which alpha = 1, is studied. In this case, there are now four free parameters and the predictions for them are: H-0 = 65.01(-1.71)(+1.81), Omega(k0) = -2.73(-0.97)(+1.53), Omega(m0) = 0.00(-0.00)(+1.22), Omega(c0) = 1.34(-0.70)(+0.94), (A) over bar = 1.000(-0.270)(+0-000). To complete the analysis the ACDM, with its three free parameters, is considered. For all these models, particular cases are considered where one or two parameters are fixed. The age of the universe, the deceleration parameter and the moment the universe begins to accelerate are also evaluated. The quartessence scenario, that unifies the description for dark matter and dark energy, is favoured. A closed (and in some cases a flat) and accelerating universe is also preferred. The CGM case alpha = 1 is far from been ruled out, and it is even preferred in some particular cases. In most of the cases the ACDM is disfavoured with respect to GCGM and CGM.
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页码:2813 / 2834
页数:22
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