Interacting non-minimally coupled canonical, phantom and quintom models of holographic dark energy in non-flat universe - High Energy Physics - TheoryReportar como inadecuado




Interacting non-minimally coupled canonical, phantom and quintom models of holographic dark energy in non-flat universe - High Energy Physics - Theory - Descarga este documento en PDF. Documentación en PDF para descargar gratis. Disponible también para leer online.

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 $L$.



Autor: M R Setare, Alberto Rozas-Fernández

Fuente: https://arxiv.org/



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