Matter power spectrum for the generalized Chaplygin gas model: The Newtonian approach

被引:37
|
作者
Fabris, J. C. [1 ]
Goncalves, S. V. B. [1 ]
Velten, H. E. S. [1 ]
Zimdahl, W. [1 ]
机构
[1] Univ Fed Espirito Santo, Dept Fis, BR-29075910 Vitoria, ES, Brazil
来源
PHYSICAL REVIEW D | 2008年 / 78卷 / 10期
关键词
D O I
10.1103/PhysRevD.78.103523
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We model the cosmic medium as the mixture of a generalized Chaplygin gas and a pressureless matter component. Within a neo-Newtonian approach (in which, different from standard Newtonian cosmology, the pressure enters the homogeneous and isotropic background dynamics) we compute the matter power spectrum. The 2dFGRS data are used to discriminate between unified models of the dark sector (a purely baryonic matter component of roughly 5% of the total energy content and roughly 95% generalized Chaplygin gas) and different models, for which there is separate dark matter, in addition to that accounted for by the generalized Chaplygin gas. Leaving the corresponding density parameters free, we find that the unified models are strongly disfavored. On the other hand, using unified model priors, the observational data are also well described, in particular, for small and large values of the generalized Chaplygin gas parameter alpha. The latter result is in agreement with a recent, more qualitative but fully relativistic, perturbation analysis in [V. Gorini, A. Y. Kamenshchik, U. Moschella, O. F. Piatella, and A. A. Starobinsky, J. Cosmol. Astropart. Phys. 02 (2008) 016.].
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页数:10
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