entropy-corrected new agegraphic dark energy in hoˇrava-lifshitz cosmology

we study the entropy-corrected version of the new agegraphic dark energy (nade) model and dark matter in a spatially non-flat universe and in the framework of hoˇrava-lifshitz cosmology. for the two cases containing noninteracting and interacting entropy-corrected nade (ecnade) models, we derive the exact differential equation that determines the evolution of the ecnade density parameter. also the deceleration parameter is obtained. furthermore, using a parametrization of the equation of state parameter of the ecnade model as ω_λ(z) = ω₀ +ω₁z, we obtain both ω₀ and ω₁. we find that in the presence of interaction, the equation of state parameter ω₀ of this model can cross the phantom divide line which is compatible with the observation.