Statefinder Parameters for Interacting Phantom Energy with Dark Matter

Abstract

We apply in this paper the statefinder parameters to the interacting phantom energy with dark matter. There are two kinds of scaling solutions in this model. It is found that the evolving trajectories of these two scaling solutions in the statefinder parameter plane are quite different, and that are also different from the statefinder diagnostic of other dark energy models.

9 pages, 12 figures, some references are added, some words are modified

References in corpus (5)

• Cosmological Evolution of a Quintom Model of Dark Energy
• Cosmological coincidence problem in interacting dark energy models
• Cosmological Evolution of Interacting Phantom Energy with Dark Matter
• Interacting Phantom Energy
• Cosmological Scaling Solutions and Cross-coupling Exponential Potential

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