Astronomy and Astrophysics – Astrophysics – Cosmology and Extragalactic Astrophysics
Scientific paper
2009-02-26
JCAP 0906:016,2009
Astronomy and Astrophysics
Astrophysics
Cosmology and Extragalactic Astrophysics
25 pages, 9 figures, comments and references added, accepted by JCAP
Scientific paper
10.1088/1475-7516/2009/06/016
We model the dark sector of the cosmic substratum by a viscous fluid with an equation of state $p=-\zeta \Theta$, where $\Theta$ is the fluid-expansion scalar and $\zeta$ is the coefficient of bulk viscosity for which we assume a dependence $\zeta \propto \rho^{\nu}$ on the energy density $\rho$. The homogeneous and isotropic background dynamics coincides with that of a generalized Chaplygin gas with equation of state $p = - A/\rho^{\alpha}$. The perturbation dynamics of the viscous model, however, is intrinsically non-adiabatic and qualitatively different from the Chaplygin-gas case. In particular, it avoids short-scale instabilities and/or oscillations which apparently have ruled out unified models of the Chaplygin-gas type. We calculate the matter power spectrum and demonstrate that the non-adiabatic model is compatible with the data from the 2dFGRS and the SDSS surveys. A $\chi^{2}$-analysis shows, that for certain parameter combinations the viscous-dark-fluid (VDF) model is well competitive with the $\Lambda$CDM model. These results indicate that \textit{non-adiabatic} unified models can be seen as potential contenders for a General-Relativity-based description of the cosmic substratum.
Hipólito-Ricaldi Wiliam S.
Velten H. E. S.
Zimdahl Winfried
No associations
LandOfFree
Non-adiabatic dark fluid cosmology does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.
If you have personal experience with Non-adiabatic dark fluid cosmology, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Non-adiabatic dark fluid cosmology will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-571217