The Holographic dark energy reexamined

Abstract

We have reexamined the holographic dark energy model by considering the spatial curvature. We have refined the model parameter and observed that the holographic dark energy model does not behave as phantom model. Comparing the holographic dark energy model to the supernova observation alone, we found that the closed universe is favored. Combining with the Wilkinson Microwave Anisotropy Probe (WMAP) data, we obtained the reasonable value of the spatial curvature of our universe.

arXiv commentdivided into sections, add one figure, some typos corrected, references added, Accepted for publication in PRD; v3: some typos corrected, title changed

References in corpus (62)

• Observational Evidence from Supernovae for an Accelerating Universe and a Cosmological Constant
• Measurements of Omega and Lambda from 42 High-Redshift Supernovae
• First Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Determination of Cosmological Parameters
• First Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Preliminary Maps and Basic Results
• Type Ia Supernova Discoveries at z>1 From the Hubble Space Telescope: Evidence for Past Deceleration and Constraints on Dark Energy Evolution
• The World as a Hologram
• A Model of Holographic Dark Energy
• The holographic principle
• Effective Field Theory, Black Holes, and the Cosmological Constant
• A Covariant Entropy Conjecture
• Entropy Bounds and Dark Energy
• A measurement by BOOMERANG of multiple peaks in the angular power spectrum of the cosmic microwave background
• Constraints on Cosmological Models from Hubble Space Telescope Observations of High-z Supernovae
• The Emergent Universe: inflationary cosmology with no singularity
• Probable Values of the Cosmological Constant in a Holographic Theory
• The State of the Dark Energy Equation of State
• Dodecahedral space topology as an explanation for weak wide-angle temperature correlations in the cosmic microwave background
• The Holographic Dark Energy in a Non-flat Universe
• Holography in General Space-times
• WMAP constraints on low redshift evolution of dark energy
• The case for dynamical dark energy revisited
• Supernova Constraints on a holographic dark energy model
• Extended Holographic dark energy
• Cosmological Parameters from Cosmic Background Imager Observations and Comparisons with BOOMERANG, DASI, and MAXIMA
• Holography and Variable Cosmological Constant
• Is the Low CMB Quadrupole a Signature of Spatial Curvature?
• Cosmological constraints from Archeops
• Variable Cosmological Constant as a Planck Scale Effect
• Model-Independent Constraints on Dark Energy Density from Flux-averaging Analysis of Type Ia Supernova Data
• Running G and Λat low energies from physics at M_X: possible cosmological and astrophysical implications
• The Holographic Principle for General Backgrounds
• The Cosmic Microwave Background Anisotropy Power Spectrum measured by Archeops
• Holography, Cosmology and the Second Law of Thermodynamics
• CFT and Entropy on the Brane
• Constraints on the dark energy from holography
• Cosmology vs. Holography
• Relating Friedmann equation to Cardy formula in universes with cosmological constant
• Testing the running of the cosmological constant with Type Ia Supernovae at high z
• Pre-bangian origin of our entropy and time arrow
• Cardy-Verlinde Formula and AdS Black Holes
• The Generalized Second Law of Thermodynamics in Cosmology
• Can we have inflation with Omega > 1?
• A Causal Entropy Bound
• WMAP data and the curvature of space
• Expansion, Geometry, and Gravity
• Partition Sums and Entropy Bounds in Weakly Coupled CFT
• Friedmann equation and Cardy formula correspondence in brane universes
• Cardy-Verlinde Formula and Holographic Dark Energy
• Entropy bounds, monotonicity properties and scaling in CFTs
• Probing the curvature of the Universe from supernova measurement
• CFT, Holography, and Causal Entropy Bound
• Holographic entropy and brane FRW-dynamics from AdS black hole in d5 higher derivative gravity
• The Cardy-Verlinde Formula and Taub-Bolt-AdS Spacetimes
• Entropy and holography constraints for inhomogeneous universes
• Casimir Effect of Graviton and the Entropy Bound
• Holographic Bound in Brans-Dicke Cosmology
• A plausible upper limit on the number of e-foldings
• Holography in (2+1)-dimensional cosmological models
• Holography and the generalized second law of thermodynamics in (2+1)-dimensional cosmology
• Observational Implications of Cosmological Event Horizons
• Holography and Eternal Inflation
• Holography, the Cosmological Constant and the Upper Limit of the Number of e-foldings

Cited by in corpus (70)

• Dynamics of dark energy
• Dark energy cosmology: the equivalent description via different theoretical models and cosmography tests
• Dark Energy
• Transition of the dark energy equation of state in an interacting holographic dark energy model
• Dark Matter and Dark Energy Interactions: Theoretical Challenges, Cosmological Implications and Observational Signatures
• Holographic Dark Energy
• Interacting holographic generalized Chaplygin gas model
• Interacting Holographic Phantom
• Covariant Generalized Holographic Dark Energy and Accelerating Universe
• Interacting dark energy, holographic principle and coincidence problem
• New generalized Chaplygin gas as a scheme for unification of dark energy and dark matter
• Barrow entropic dark energy: A member of generalized holographic dark energy family
• Constraints on holographic dark energy from X-ray gas mass fraction of galaxy clusters
• Thermodynamical description of the interaction between holographic dark energy and dark matter
• Restoring Holographic Dark Energy in Brane Cosmology
• Unifying Holographic Inflation with Holographic Dark Energy: a Covariant Approach
• Holographic dark energy in Brans-Dicke theory
• Holographic Dark Energy in Braneworld Models with a Gauss-Bonnet Term in the Bulk. Interacting Behavior and the w =-1 Crossing
• Interacting holographic dark energy
• Statefinder diagnosis in a non-flat universe and the holographic model of dark energy
• A Tracker Solution for a Holographic Dark Energy Model
• Age Problem in the Holographic Dark Energy Model
• On holographic dark-energy models
• Observational constraints on two cosmological models of $f(Q)$ theory
• Thermodynamical properties of the Universe with dark energy
• Current constraints on interacting holographic dark energy
• A Modified Holographic Dark Energy Model with Infrared Infinite Extra Dimension(s)
• Holographic Dark Energy in Braneworld Models with Moving Branes and the w=-1 Crossing
• Schwarzschild black hole and the generalized second law in phantom-dominated universe
• Dark energy from vacuum entanglement
• Holographic dark energy in a universe with spatial curvature and massive neutrinos: a full Markov Chain Monte Carlo exploration
• Barrow HDE model for Statefinder diagnostic in FLRW Universe
• Possible theoretical limits on holographic quintessence from weak gravity conjecture
• Particle vs. future event horizon in interacting holographic dark energy model
• Statefinder Diagnostic for Dilaton Dark Energy
• Cosmological models with Lagrange Multiplier Field
• Constraints on the Holographic Dark Energy Model from Type Ia Supernovae, WMAP7, Baryon Acoustic Oscillation and Redshift-Space Distortion
• Thermodynamics in Closed Universe with Entropy Corrections
• Cosmology with Ricci dark energy
• Hologrphy and holographic dark energy model
• Holographic Dark Energy from a Modified GBIG Scenario
• Holographic correspondence of $F(R)$ gravity with/without matter fields
• Notes on interacting holographic dark energy model in a closed universe
• A Braneworld Dark Energy Model with Induced Gravity and the Gauss-Bonnet Effect
• Reconstruction of interaction rate in Holographic dark energy
• A New Type of Dark Energy Model
• Barrow Holographic Dark Energy Model with GO Cut-off -- An Alternative Perspective
• The dynamical behavior of the Extended Holographic Dark Energy with Hubble Horizon
• Constraints to Holographic Dark Energy Model via Type Ia Supernovae, Baryon Acoustic Oscillation and WMAP
• The mass and the coupling of the Dark Particle
• Exponential Potentials and Attractor Solution of Dilatonic Cosmology
• Thermodynamics of Shearing Massless Scalar Field Spacetimes is Inconsistent With the Weyl Curvature Hypothesis
• Holographic Dark Information Energy
• Non-existence of Extended Holographic Dark Energy with Hubble Horizon
• Interacting holographic tachyon model of dark energy
• Possible Equilibria of Interacting Dark Energy Models
• Stephani Cosmology: Entropically Viable But Observationally Challenged
• Constraining the Lattice Fluid Dark Energy from SNe Ia, BAO and OHD
• Holographic dark information energy: Predicted dark energy measurement
• Can Holographic dark energy increase the mass of the wormhole?
• Particle Production and Universal Thermodynamics
• Reexamining RHDE Models in FRW Universe with two IR cut-off with redshift parametrization
• A Dynamic Dark Information Energy Consistent with Planck Data
• Potentials of Coupled Quintessence Based on a Dilaton
• Zero Cosmological Constant and Nonzero Dark Energy from Holographic Principle
• Holographic Principle and the Second Law in Stephani Cosmology Revisited
• Generalized Semi-Holographic Universe
• Dark energy and the future fate of the Universe
• On curvature coupling and quintessence fine-tuning
• Quintessence reconstruction of interacting HDE in a non-flat universe