Entropy-Corrected Holographic Dark Energy

Abstract

The holographic dark energy (HDE) is now an interesting candidate of dark energy, which has been studied extensively in the literature. In the derivation of HDE, the black hole entropy plays an important role. In fact, the entropy-area relation can be modified due to loop quantum gravity or other reasons. With the modified entropy-area relation, we propose the so-called ``entropy-corrected holographic dark energy'' (ECHDE) in the present work. We consider many aspects of ECHDE and find some interesting results. In addition, we briefly consider the so-called ``entropy-corrected agegraphic dark energy'' (ECADE).

11 pages, 2 tables, revtex4; v2: references added

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• Power-Law Entropy Corrected Holographic Dark Energy Model
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• Interacting holographic dark energy with logarithmic correction
• Generalized second law of thermodynamics for FRW cosmology with logarithmic correction
• Reconstructing f(R) modified gravity from ordinary and entropy-corrected versions of the holographic and new agegraphic dark energy models
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• Correspondence between entropy-corrected holographic and Gauss-Bonnet dark energy models
• Interacting Entropy-Corrected Holographic Dark Energy and IR Cut-Off Length
• Interacting Ricci Dark Energy with Logarithmic Correction
• Holographic dark energy in Brans-Dicke theory with log correction
• Interacting entropy-corrected new agegraphic dark energy in Brans-Dicke cosmology
• Cosmic accelerated expansion and the entropy corrected holographic dark energy
• Interacting entropy-corrected new agegraphic tachyon, K-essence and dilaton scalar field models of dark energy in non-flat universe
• Reconstructing interacting entropy-corrected holographic scalar field models of dark energy in non-flat universe
• Bounce cosmology in $f(\mathcal{R})$ gravity
• Two-Fluid Dark Energy Models in Bianchi Type-III Universe with Variable Deceleration Parameter
• Thermodynamics and stability of $f(T,B)$ gravity with viscous fluid by observational constraints
• Interacting entropy-corrected new agegraphic dark energy in non-flat universe
• Stability and interacting $f(T,\mathcal{T})$ gravity with modified Chaplygin gas
• An interacting New Holographic Dark Energy in the framework of fractal cosmology
• Interacting $F(R,T)$ gravity with modified Chaplygin gas
• Scalar Field Reconstruction of Power-Law Entropy-Corrected HDE
• Reconstructions of $f(T)$ Gravity from Entropy Corrected Holographic and New Agegraphic Dark Energy Models in Power-law and Logarithmic Versions
• Power-law entropy-corrected HDE and NADE in Brans-Dicke cosmology
• Interacting entropy-corrected holographic dark energy with apparent horizon as an infrared cutoff
• Interacting entropy-corrected holographic Chaplygin gas model
• Logarithmic entropy corrected holographic dark energy with $F(R,T)$ gravity
• A stable flat entropy-corrected FRW universe
• Cosmological Tests of $f(R,G,T)$ Dark Energy Model in FRW Universe
• Interacting entropy-corrected holographic scalar field models in non-flat universe
• Power-Law and Logarithmic Entropy-Corrected Ricci Viscous Dark Energy and Dynamics of Scalar Fields
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• Irreversible thermodynamics of dark energy on entropy-corrected apparent horizon
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• Reconstructing $f(T)$ modified gravity from ECHDE and ECNADE models
• Gravitational Collapse With Dark Energy And Dark Matter In Hořava-Lifshitz Gravity
• Entropy-corrected new agegraphic dark energy in Horava-Lifshitz cosmology
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• The interaction of extended Bose-Einstein condensate dark matter with viscous $f(T,B)$ gravity
• Thermodynamics of an Evolving Lorentzian Wormhole with Entropy Corrections
• Thermodynamics of interacting holographic dark energy
• Power Law and Logarithmic Ricci Dark Energy Models in Horava-Lifshitz Cosmology
• Inflation via logarithmic entropy-corrected holographic dark energy model
• Entropy-Corrected New Agegraphic Dark Energy Model in Horava-Lifshitz Gravity
• Holographic dark energy models with Interactions and entropy corrections for different cutoffs in the Brans-Dicke cosmology
• Correspondence between particle creation and dark components interaction in the context of $f(\mathcal{G})$ gravity