We investigate the holographic dark energy scenario with a varying gravitational constant in a flat background in the context of Ho{r}ava-Lifshitz gravity. We extract the exact differential equation determining the evolution of the dark energy density parameter, which includes G variation term. Also we discuss a cosmological implication of our work by evaluating the dark energy equation of state for low redshifts containing varying G corrections.
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Setare et al. (2010) studied this question.
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