Interacting non-minimally coupled canonical, phantom and quintom models of holographic dark energy in non-flat universe

Details Interacting non-minimally coupled canonical, phantom and quintom models of holographic dark energy in non-flat universe Interacting non-minimally coupled canonical, phantom and quintom models of holographic dark energy in non-flat universe

2009-06-10

arxiv.org/abs/0906.1936v3

Physics

High Energy Physics

High Energy Physics - Theory

18 pages, 3 figures. Accepted for publication in IJMPD (2010)

Scientific paper

Motivated by our recent work \cite{set1}, we generalize this work to the interacting non-flat case. Therefore in this paper we deal with canonical, phantom and quintom models, with the various fields being non-minimally coupled to gravity, within the framework of interacting holographic dark energy. We employ the holographic model of interacting dark energy to obtain the equation of state for the holographic energy density in non-flat (closed) universe enclosed by the event horizon measured from the sphere of horizon named $L$.

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