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We explore flat ΛCDM models with bulk viscosity, and study the role of the bulk viscosity in the evolution of these universe
models. The dynamical equations for these models are obtained and solved for some cases of bulk viscosity. We obtain differential
equations for the Hubble parameter H and the energy density of dark matter ρ
m
, for which we give analytical solutions for some cases and for the general case we give a numerical solution. Also we calculate
the statefinder parameters for these models and display them in the s–r-plane. 相似文献
2.
In this paper we study the evolution of spatially homogeneous and anisotropic Bianchi type-I Universe models with the cosmological constant, Λ, and filled with nonlinear viscous fluid. The dynamical equations for these models are obtained and solved for some special cases. We calculate the statefinder parameters for the models and display them in the s-r-plane. 相似文献
3.
The cosmological event horizon entropy and the apparent horizon entropy of the ΛCDM and the Bianchi type I Universe model with viscosity has been calculated numerically, and analytically in the large time limit. It is shown that for these Universe models the cosmological event horizon entropy increases with time and for large times it approaches a finite maximum value. The effect of viscosity upon the entropy is also studied and we have found that its role is to decrease the entropy. The bigger the viscosity coefficient is the less the entropy will be. Furthermore, the radiation entropy for the ΛCDM Universe model with and without viscosity is investigated, and together with the cosmological event horizon entropy are used to examine the validity of the generalized second law of thermodynamics, which states that the total rate of change of entropy of the Universe is never negative, in this Universe model. 相似文献
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