Interacting generalized Chaplygin gas model in non-flat universe
classification
🌀 gr-qc
keywords
chaplyginenergygeneralizeduniversedarkinteractingnon-flatchoosing
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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 $w_{\rm \Lambda}^{eff}< -1$, that corresponds to a universe dominated by phantom dark energy.
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