Reconstructing interacting entropy-corrected holographic scalar field models of dark energy in the non-flat universe

2011/01/17 by Kayoomars Karami, K Karami, M. S. Khaledian +2 · 46 citations
Physics and Astronomy · #Black Holes and Theoretical Physics #Cosmology and Gravitation Theories #Dark energy #Dark fluid #Field (mathematics) #Holography #Particle physics theoretical and experimental studies #Scalar (mathematics) #Scalar field #Scalar field dark matter #Universe #hep-th #physics.gen-ph

paper · pdf · doi:10.1088/0031-8949/83/02/025901

published in Physica Scripta 83(2), 025901 (IOP Publishing) · 14 pages, version published in Physica Scripta

openalex publication_date 2011/01/17 · arxiv created 2011/01/19 · arxiv updated 2011/02/21 · openalex created_date 2016/06/24 · openalex updated_date 2026/08/05

Abstract

Here we consider the entropy-corrected version of the holographic dark energy model in the non-flat universe. We obtain the equation of state parameter in the presence of interaction between dark energy and dark matter. Moreover, we reconstruct the potential and the dynamics of the quintessence, tachyon, K-essence and dilaton scalar field models according to the evolutionary behavior of the interacting entropy-corrected holographic dark energy model.

Citations

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