Holographic dark energy interacting with dark matter in a Closed Universe
Abstract
A cosmological model of an holographic dark energy interacting with dark matter throughout a decaying term of the form Q=3(λ1DE + λ2m) H is investigated. General constraint on the parameters of the model are found when accelerated expansion is imposed and we found a phantom scenarios, without any reference to a specific equation of state for the dark energy. The behavior of equation of stated for dark energy is also discussed.
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