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Holographic dark energy interacting with dark matter in a Closed Universe

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 نشر من قبل Joel Saavedra
 تاريخ النشر 2008
  مجال البحث فيزياء
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A cosmological model of an holographic dark energy interacting with dark matter throughout a decaying term of the form $Q=3(lambda_1rho_{DE} + lambda_2rho_m) H$ 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.



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