Phantom-like GCG and the constraints of its parameters via cosmological dynamics
arXiv:astro-ph/0404154 · doi:10.1016/j.physletb.2004.11.079
Abstract
We extend the equation of state of GCG (Generalized Chaplygin Gas) to regime and show, from the point of view of dynamics, that the parameters of GCG should be in the range of . Also, dynamical analysis indicate that the phase is a dynamical attractor and the equation of state of GCG approaches it from either or depending on the choice of its initial cosmic density parameter and the ratio of pressure to critical energy density.
12 pages, 4 eps figures. Final version to appear in Phys. Lett. B
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