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We investigate canonical, phantom and quintom models, with the various fieldsbeing non-minimally coupled to gravity, in the framework of holographic darkenergy. We classify them and we discuss their cosmological implications. Inparticular, we examine the present value of the dark energy equation-of-stateparameter and the crossing through the phantom divide, and we extract theconditions for a future cosmological singularity. The combined scenarios are inagreement with observations and reveal interesting cosmological behaviors.

Non-minimally coupled canonical, phantom and quintom models of holographic dark energy