Interacting Holographic Phantom

Abstract

In this paper we consider the holographic model of interacting dark energy in non-flat universe. With the choice of $c\le 0.84$, the interacting holographic dark energy can be described by a phantom scalar field. Then we show this phantomic description of the holographic dark energy with $c\le 0.84$ and reconstruct the potential of the phantom scalar field.

15 pages, no figures, text extended, references added

References in corpus (1)

• Cosmological Evolution of a Quintom Model of Dark Energy

Cited by in corpus (15)

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• Holographic Dark Energy in Braneworld Models with a Gauss-Bonnet Term in the Bulk. Interacting Behavior and the w =-1 Crossing
• Coupled oscillators as models of quintom dark energy
• Quintom model with O($N$) symmetry
• Age Problem in the Holographic Dark Energy Model
• Thermodynamical Interpretation of the Interacting Holographic Dark Energy Model in a non-flat Universe
• Shape invariance method for quintom model in the bent brane background
• Crossing the phantom divide in an interacting generalized Chaplygin gas
• The Coincidence Problem and Interacting Holographic Dark Energy
• Bouncing Universe with Non-minimally Coupled Quintom Matter
• Possible Equilibria of Interacting Dark Energy Models