Some Issues Concerning Holographic Dark Energy
arXiv:0801.1407 · doi:10.1088/1475-7516/2008/05/023
Abstract
We study perturbation of holographic dark energy and find it be stable. We study the fate of the universe when interacting holographic dark energy is present, and discuss a simple phenomenological classification of the interacting holographic dark energy models. We also discuss the cosmic coincidence problem in the context of holographic dark energy. We find that the coincidence problem can not be completely solved by adding an interacting term. Inflation may provide a better solution of the coincidence problem.
19 pages, 6 figures. final version published in JCAP
References in corpus (49)
- 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
- Wilkinson Microwave Anisotropy Probe (WMAP) Three Year Results: Implications for Cosmology
- Dynamics of dark energy
- The Cosmological Constant and Dark Energy
- 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
- Cosmological parameters from SDSS and WMAP
- The Case for a Positive Cosmological Lambda-term
- A Model of Holographic Dark Energy
- The 3D power spectrum of galaxies from the SDSS
- New Hubble Space Telescope Discoveries of Type Ia Supernovae at z > 1: Narrowing Constraints on the Early Behavior of Dark Energy
- Cosmological Results from High-z Supernovae
- New Constraints on , , and w from an Independent Set of Eleven High-Redshift Supernovae Observed with HST
- Effective Field Theory, Black Holes, and the Cosmological Constant
- Cosmological Constraints from the SDSS Luminous Red Galaxies
- Three Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Polarization Analysis
- Cosmological parameter analysis including SDSS Ly-alpha forest and galaxy bias: constraints on the primordial spectrum of fluctuations, neutrino mass, and dark energy
- First Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Foreground Emission
- Three-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Temperature Analysis
- Holographic dark energy and cosmic coincidence
- Transition of the dark energy equation of state in an interacting holographic dark energy model
- Constraints on holographic dark energy from type Ia supernova observations
- The Holographic Dark Energy in a Non-flat Universe
- Statefinder diagnostic for holographic dark energy model
- Supernova Constraints on a holographic dark energy model
- Constraints on Holographic Dark Energy from Latest Supernovae, Galaxy Clustering, and Cosmic Microwave Background Anisotropy Observations
- Interacting dark energy, holographic principle and coincidence problem
- Bulk-Brane Interaction and Holographic Dark Energy
- Testing the viability of the interacting holographic dark energy model by using combined observational constraints
- Three-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Beam Profiles, Data Processing, Radiometer Characterization and Systematic Error Limits
- Instability of holographic dark energy models
- Why the cosmological constant is small and positive
- Statefinder diagnosis for the interacting model of holographic dark energy
- Anthropic Principle Favors the Holographic Dark Energy
- The Cosmological Dynamics of Interacting Holographic Dark Energy Model
- Age Problem in the Holographic Dark Energy Model
- Holographic dark energy in a cyclic universe
- Current constraints on interacting holographic dark energy
- Thermodynamics second law and crossing(s) in interacting holographic dark energy model
- Phantom Dark Energy, Cosmic Doomsday, and the Coincidence Problem
- Interacting Dark Energy and the Cosmic Coincidence Problem
- Inflation with Holographic Dark Energy
- Particle vs. future event horizon in interacting holographic dark energy model
- Holographic Cosmological Constant and Dark Energy
- Constraints on the solid dark universe model
- Insights into Dark Energy: Interplay Between Theory and Observation
- Constraining interacting dark energy models with flux destabilization
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- Statefinder Diagnosis for Ricci Dark Energy
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- Unifying Holographic Inflation with Holographic Dark Energy: a Covariant Approach
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- Features of holographic dark energy under the combined cosmological constraints
- Thermodynamical Interpretation of the Interacting Holographic Dark Energy Model in a non-flat Universe
- Large-scale stable interacting dark energy model: Cosmological perturbations and observational constraints
- Comparison of dark energy models: A perspective from the latest observational data
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- Dynamical analysis and statefinder of Barrow holographic dark energy
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- Reconstructing Theory from Ricci Dark Energy
- Growth of matter perturbations in clustered holographic dark energy cosmologies
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- New Agegraphic Dark Energy in Gravity
- Holographic Gas as Dark Energy
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- New Agegraphic Dark Energy in Brans-Dicke Theory
- Holographic Dark Energy with Cosmological Constant
- Revisiting the holographic dark energy in a non-flat universe: alternative model and cosmological parameter constraints
- Effects of Anisotropy on the Sign-Changeable Interacting Tsallis Holographic Dark Energy
- Exploring interacting holographic dark energy in a perturbed universe with parameterized post-Friedmann approach
- Revisit of constraints on holographic dark energy: SNLS3 dataset with the effects of time-varying and different light-curve fitters
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- Strong gravitational lensing constraints on holographic dark energy
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- Crossing the phantom divide line in the Holographic dark energy model in a closed universe
- Entropy In The Present And Early Universe: New Small Parameters And Dark Energy Problem
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- Effects of a time-varying color-luminosity parameter on the cosmological constraints of modified gravity models
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- Interacting non-minimally coupled canonical, phantom and quintom models of holographic dark energy in non-flat universe
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- Cosmology in holographic non-minimal derivative coupling theory: constraints from inflation and variation of gravitational constant
- How Holographic is the Dark Energy? A Spline Nodal reconstruction approach