2011/12/31 by Antonio Pasqua, A. Khodam-Mohammadi, Mubasher Jamil +2 · 1 citation
Physics and Astronomy · #Apparent horizon #Astrophysics #Black Holes and Theoretical Physics #Cosmology #Cosmology and Gravitation Theories #Dark energy #Dark fluid #Dark matter #Deceleration parameter #Equation of state #Event (particle physics) #Event horizon #Friedmann–Lemaître–Robertson–Walker metric #Galaxies: Formation, Evolution, Phenomena #Mathematical physics #Physics #Quantum mechanics #Quintessence #Scalar field dark matter #Tachyon #Theoretical physics #Universe #gr-qc #hep-th
paper · pdf · doi:10.1007/s10509-012-1031-8
published as Astrophysics and Space Science: Volume 340, 199-208, (2012) · 24 pages, accepted for publication in 'Astrophysics and Space Science, DOI:10.1007/s10509-012-1031-8'
arxiv created 2012/03/03 · openalex publication_date 2012/03/07 · arxiv updated 2012/06/06 · openalex created_date 2025/10/10 · openalex updated_date 2026/08/05
Motivated by the holographic principle, it has been suggested that the dark energy density may be inversely proportional to the area A of the event horizon of the universe. However, such a model would have a causality problem. In this work, we consider the entropy-corrected version of the holographic dark energy model in the non-flat FRW universe and we propose to replace the future event horizon area with the inverse of the Ricci scalar curvature. We obtain the equation of state (EoS) parameter ωΛ, the deceleration parameter q and ΩD' in the presence of interaction between Dark Energy (DE) and Dark Matter (DM). Moreover, we reconstruct the potential and the dynamics of the tachyon, K-essence, dilaton and quintessence scalar field models according to the evolutionary behavior of the interacting entropy-corrected holographic dark energy model.