Journal
EUROPEAN PHYSICAL JOURNAL C
Volume 69, Issue 3-4, Pages 575-579Publisher
SPRINGER
DOI: 10.1140/epjc/s10052-010-1427-y
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Funding
- Direccion de Investigacion y Desarrollo, Universidad de La Frontera [DIUFRO DI10-0009]
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In this work we study the dark energy problem by adopting an holographic model proposed recently in the literature. In this model there has been postulated an energy density rho similar to R, where R is the Ricci scalar curvature. Under this consideration, we have obtained a cosmological scenario which arises from considering two non-interacting fluids along the lines of a reasonable Ansatz for the cosmic coincidence parameter. We have adjusted the involved parameters in the model according to the observational data, showing that the equation of state for the dark energy exhibits a cross through the -1 barrier. Additionally, we have found a disagreement of these parameters in comparison with a scalar field theory approach.
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