Interacting Entropy-Corrected Holographic Dark Energy and IR Cut-Off Length

Abstract

In this paper we consider holographic dark energy model with corrected holographic energy density and show that this model may be equivalent to the modified Chaplygin gas model. Then we obtain relation between entropy corrected holographic dark energy model and scalar field models. We do these works by using choices of IR cut-off length proportional to the Hubble radius, the event horizon radius, the Ricci length, and the Granda-Oliveros length.

13 pages, 2 figures added in revised version. References added

References in corpus (15)

• Cosmology and the Fate of Dilatation Symmetry
• Infrared cut-off proposal for the Holographic density
• New infrared cut-off for the holographic scalar fields models of dark energy
• Quantum Tunneling and Back Reaction
• Interacting holographic generalized Chaplygin gas model
• Non-minimally coupled canonical, phantom and quintom models of holographic dark energy
• Black hole quantum tunnelling and black hole entropy correction
• Holographic dark energy with varying gravitational constant
• Dark energy models with variable equation of state parameter
• FRW Bulk Viscous Cosmology with Modified Chaplygin Gas in Flat Space
• 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
• Entropy-Corrected Holographic Dark Energy
• Interaction between viscous varying modified cosmic Chaplygin gas and Tachyonic fluid
• Interacting entropy-corrected holographic scalar field models in non-flat universe

Cited by in corpus (27)

• Higher order corrections of the extended Chaplygin gas cosmology with varying $G$ and $\Lambda$
• Interacting Quintessence Models of Dark Energy
• The universe dominated by the extended Chaplygin gas
• Extended Chaplygin Gas in Horava-Lifshitz Gravity
• Higher derivative corrections of $f(R)$ gravity with varying equation of state in the case of variable $G$ and $\Lambda$
• Interacting two-component fluid models with varying EoS parameter
• Thermodynamics of the viscous $f(T,B)$ gravity in the new agegraphic dark energy model
• Interacting Holographic Extended Chaplygin Gas and Phantom Cosmology in the Light of BICEP2
• Thermodynamics and stability of $f(T,B)$ gravity with viscous fluid by observational constraints
• An effective quintessence field with a power-law potential
• Stability and interacting $f(T,\mathcal{T})$ gravity with modified Chaplygin gas
• Phenomenological Fluids from Interacting Tachyonic Scalar Fields
• Logarithmic corrected $F(R)$ gravity in the light of Planck 2015
• Mutually interacting Tachyon dark energy with variable $G$ and $\Lambda$
• Cosmological Tests of $f(R,G,T)$ Dark Energy Model in FRW Universe
• Interaction between modified Chaplygin gas and ghost dark energy in presence of extra dimensions
• A Universe with a generalized ghost dark energy and Van der Waals fluid interacting with a fluid
• Dark Energy and Tachyon Field in Bianchi Type-V Space-time
• Observational constraints and stability in viscous $f(T,\mathcal{T})$ gravity
• Observational Hubble parameter data constraints on the interactive model of $f(T)$ gravity with particle creation
• Quintessence Cosmology with an Effective $\Lambda$-Term in Lyra Manifold
• Warm Inflation with Barrow Holographic Dark Energy
• Viscous interacting and stability on dark matter Bose-Einstein condensation with modified Chaplygin gas
• Time dependent dark energy and the thermodynamics of many-body systems
• Interacting Dark Energy and Its Implications for Unified Dark Sector
• Revisiting Holographic Dark Energy in Cyclic Cosmology
• Toy models of Universe with an Effective varying $\Lambda$-Term in Lyra Manifold