Interacting generalized Chaplygin gas model in non-flat universe

Abstract

We employ the generalized Chaplygin gas of interacting dark energy to obtain the equation of state for the generalized Chaplygin gas energy density in non-flat universe. By choosing a negative value for $B$ we see that $w_{\mathrm{\Lambda }}^{eff}<-1$, that corresponds to a universe dominated by phantom dark energy.

8 pages, no figure

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