Interacting generalized Chaplygin gas model in non-flat universe

Details Interacting generalized Chaplygin gas model in non-flat universe Interacting generalized Chaplygin gas model in non-flat universe

2007-11-04

arxiv.org/abs/0711.0524v1

Eur.Phys.J.C52:689-692,2007

Astronomy and Astrophysics

Astrophysics

General Relativity and Quantum Cosmology

8 pages, no figure

Scientific paper

10.1140/epjc/s10052-007-0405-5

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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