Dynamics of interacting phantom and quintessence dark energies

Abstract

We present models, in which phantom energy interacts with two different types of dark energies including variable modified Chaplygin gas (VMCG) and new modified Chaplygin gas (NMCG). We then construct potentials for these cases. It has been shown that the potential of the phantom field decreases from a higher value with the evolution of the Universe.

7 pages, 6 figures, accepted for publication in Astrophysics and Space Science

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• Cold, ultracold and Nariai black holes with quintessence
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• On the stability of the dark energy based on generalized uncertainty principle
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