Interacting non-minimally coupled canonical, phantom and quintom models of holographic dark energy in non-flat universe - High Energy Physics - TheoryReport as inadecuate




Interacting non-minimally coupled canonical, phantom and quintom models of holographic dark energy in non-flat universe - High Energy Physics - Theory - Download this document for free, or read online. Document in PDF available to download.

Abstract: Motivated by our recent work \cite{set1}, we generalize this work to theinteracting non-flat case. Therefore in this paper we deal with canonical,phantom and quintom models, with the various fields being non-minimally coupledto gravity, within the framework of interacting holographic dark energy. Weemploy the holographic model of interacting dark energy to obtain the equationof state for the holographic energy density in non-flat closed universeenclosed by the event horizon measured from the sphere of horizon named $L$.



Author: M R Setare, Alberto Rozas-Fernández

Source: https://arxiv.org/



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