Interacting Ricci Dark Energy with Logarithmic Correction
arXiv:1112.6381 · doi:10.1007/s10509-012-1031-8
Abstract
Motivated by the holographic principle, it has been suggested that the dark energy density may be inversely proportional to the area 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 , the deceleration parameter and 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.
24 pages, accepted for publication in 'Astrophysics and Space Science, DOI:10.1007/s10509-012-1031-8'
References in corpus (42)
- Wilkinson Microwave Anisotropy Probe (WMAP) Three Year Results: Implications for Cosmology
- Dynamics of dark energy
- Cosmology and the Fate of Dilatation Symmetry
- Cosmological parameters from combining the Lyman-alpha forest with CMB, galaxy clustering and SN constraints
- A Dark Energy Model Characterized by the Age of the Universe
- A New Model of Agegraphic Dark Energy
- Infrared cut-off proposal for the Holographic density
- Dark Energy-Dark Matter Interaction and putative violation of the Equivalence Principle from the Abell Cluster A586
- Hawking Radiation of Apparent Horizon in a FRW Universe
- The holographic dark energy in non-flat Brans-Dicke cosmology
- Quantum Tunneling and Back Reaction
- Consequences of dark matter-dark energy interaction on cosmological parameters derived from SNIa data
- Interacting holographic generalized Chaplygin gas model
- Interacting Holographic Phantom
- Constraints on Holographic Dark Energy from Latest Supernovae, Galaxy Clustering, and Cosmic Microwave Background Anisotropy Observations
- Dynamical vacuum energy, holographic quintom, and the reconstruction of scalar-field dark energy
- Holographic Ricci dark energy: Current observational constraints, quintom feature, and the reconstruction of scalar-field dark energy
- Bulk-Brane Interaction and Holographic Dark Energy
- Testing the viability of the interacting holographic dark energy model by using combined observational constraints
- Holographic tachyon model of dark energy
- Holographic dark energy with varying gravitational constant
- Fermion Tunneling Beyond Semiclassical Approximation
- Interacting holographic dark energy in Brans-Dicke theory
- Exact Differential and Corrected Area Law for Stationary Black Holes in Tunneling Method
- Holographic dark energy in Brans-Dicke cosmology with chameleon scalar field
- Thermodynamical Interpretation of the Interacting Holographic Dark Energy Model in a non-flat Universe
- Tachyon dark energy models: dynamics and constraints
- Interacting Modified Variable Chaplygin Gas in Non-flat Universe
- Interacting HDE and NADE in Brans-Dicke Chameleon Cosmology
- Entropy-Corrected Holographic Dark Energy
- The Holographic Model of Dark Energy and Thermodynamics of Non-Flat Accelerated Expanding Universe
- Generalized second law of thermodynamics for FRW cosmology with logarithmic correction
- Statefinder diagnostic and stability of modified gravity consistent with holographic and new agegraphic dark energy
- Interacting entropy-corrected agegraphic-tachyon dark energy
- Correspondence between entropy-corrected holographic and Gauss-Bonnet dark energy models
- Cosmic accelerated expansion and the entropy corrected holographic dark energy
- Reconstructing interacting entropy-corrected holographic scalar field models of dark energy in non-flat universe
- Dark energy generated from a (super)string effective action with higher order curvature corrections and a dynamical dilaton
- Logarithmic entropy--corrected holographic dark energy with non--minimal kinetic coupling
- Proper Matter Collineations of Plane Symmetric Spacetimes
- Parametrization of Tachyon Field
- Interacting entropy-corrected holographic scalar field models in non-flat universe
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- FRW Cosmology in F(R,T) gravity
- Reconstruction of f(T) gravity from the Holographic dark energy
- Bouncing cosmology in modified gravity with higher-order curvature terms
- Reconstruction of f(T) and f(R) gravity according to (m,n)-type holographic dark energy
- Power-Law Entropy Corrected Ricci Dark Energy and Dynamics of Scalar Fields
- Cosmology with Ricci dark energy
- Logarithmic entropy--corrected holographic dark energy with non--minimal kinetic coupling
- Traversable holographic dark energy wormholes constrained by astronomical observations
- Scalar perturbations in cosmological models with dark energy - dark matter interaction
- Power-Law and Logarithmic Entropy-Corrected Ricci Viscous Dark Energy and Dynamics of Scalar Fields
- Statefinder diagnostic of logarithmic entropy corrected holographic dark energy with Granda-Oliveros IR cut-off
- Interacting Ricci Logarithmic Entropy Corrected Holographic Dark Energy in Brans-Dicke Cosmology
- Power Law and Logarithmic Ricci Dark Energy Models in Horava-Lifshitz Cosmology
- Loop Quantum Corrections to Statefinder Parameters of Dark Energy
- Observational constraints and differential diagnosis for cosmic evolutionary models