Viscous generalized Chaplygin gas
Viscous GCG(generalized Chaplygin gas) cosmology is discussed, assuming that there is bulk viscosity in the barotropic fluid and GCG. The dynamical analysis indicates that the phase $w_g=-1+\sqrt{3}γκτ_{g}/(γ-\sqrt{3}κτ_γ)$ is a dynamical attractor and the equation of state of GCG approaches it from either $w_g>-1$ or $w_g<-1$ depending on the choice of its initial cosmic density parameter and the ratio of pressure to critical energy density. Obviously, the equation of state $w_g$ can cross the boundary $w_g=-1$. Also, from the point of view of dynamics, the parameters of viscous GCG should be in the range of $γ>\sqrt{3}κτ_γ/(1-\sqrt{3}κτ_{g})$ and $0<α<1+\sqrt{3} κγτ_{g}/(γ-\sqrt{3}κτ_γ-\sqrt{3}κγ\t au_{g})$.
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