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arxiv: 0710.4283 · v3 · submitted 2007-10-23 · ✦ hep-th

Crossing the phantom divide in an interacting generalized Chaplygin gas

classification ✦ hep-th
keywords darkdensitieschaplygindivideenergygeneralizedphantomsolution
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Unified generalized Chaplygin gas models assuming an interaction between dark energy and dark matter fluids have been previously proposed. Following these ideas, we consider a particular relation between dark densities, which allows the possibility of a time varying equation of state for dark energy that crosses the phantom divide at a recent epoch. Moreover, these densities decay during all the evolution of the Universe, avoiding a Big Rip. We find also a scaling solution, i.e. these densities are asymptotically proportional in the future, which contributes to the solution of the coincidence problem.

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