Holographic dark energy interacting with dark matter in a Closed Universe

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dc.creatorCruz, Norman
dc.creatorLepe, Samuel
dc.creatorPena, Francisco
dc.creatorSaavedra, Joel
dc.date2008-07-24
dc.date.accessioned2026-07-07T11:45:03Z
dc.date.available2026-07-07T11:45:03Z
dc.descriptionA cosmological model of an holographic dark energy interacting with dark matter throughout a decaying term of the form $Q=3(λ_1ρ_{DE} + λ_2ρ_m) H$ 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.
dc.description9 pages
dc.identifierhttps://arxiv.org/abs/0807.3854
dc.identifierhttp://arxiv.org/abs/0807.3854
dc.identifierPhys.Lett.B669:271-274,2008
dc.identifierdoi:10.1016/j.physletb.2008.10.008
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/201764
dc.subjectGeneral Relativity and Quantum Cosmology
dc.titleHolographic dark energy interacting with dark matter in a Closed Universe
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