Probing interaction and spatial curvature in the holographic dark energy model

Abstract

In this paper we place observational constraints on the interaction and spatial curvature in the holographic dark energy model. We consider three kinds of phenomenological interactions between holographic dark energy and matter, i.e., the interaction term $Q$ is proportional to the energy densities of dark energy (${\rho }_{\Lambda }$), matter (${\rho }_m$), and matter plus dark energy (${\rho }_m+{\rho }_{\Lambda }$). For probing the interaction and spatial curvature in the holographic dark energy model, we use the latest observational data including the type Ia supernovae (SNIa) Constitution data, the shift parameter of the cosmic microwave background (CMB) given by the five-year Wilkinson Microwave Anisotropy Probe (WMAP5) observations, and the baryon acoustic oscillation (BAO) measurement from the Sloan Digital Sky Survey (SDSS). Our results show that the interaction and spatial curvature in the holographic dark energy model are both rather small. Besides, it is interesting to find that there exists significant degeneracy between the phenomenological interaction and the spatial curvature in the holographic dark energy model.

11 pages, 5 figures; to appear in JCAP

References in corpus (61)

• Seven-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Cosmological Interpretation
• Wilkinson Microwave Anisotropy Probe (WMAP) Three Year Results: Implications for Cosmology
• Dynamics of dark energy
• Five-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Cosmological Interpretation
• Cosmology and the Fate of Dilatation Symmetry
• Dark Energy and the Accelerating Universe
• Cosmological Constraints from the SDSS Luminous Red Galaxies
• Three Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Polarization Analysis
• Improved Dark Energy Constraints from ~100 New CfA Supernova Type Ia Light Curves
• A Dark Energy Model Characterized by the Age of the Universe
• A New Model of Agegraphic Dark Energy
• A Holographic Dark Energy Model from Ricci Scalar Curvature
• Unified First Law and Thermodynamics of Apparent Horizon in FRW Universe
• Hawking Radiation of Apparent Horizon in a FRW Universe
• Holographic dark energy models: A comparison from the latest observational data
• Constraints on Holographic Dark Energy from Latest Supernovae, Galaxy Clustering, and Cosmic Microwave Background Anisotropy Observations
• Friedmann Equations and Thermodynamics of Apparent Horizons
• 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
• Reconstructing holographic quintessence
• Cosmological Constraints on New Agegraphic Dark Energy
• Thermodynamics of Apparent Horizon in Brane World Scenario
• Testing the viability of the interacting holographic dark energy model by using combined observational constraints
• Statefinder Diagnosis for Ricci Dark Energy
• Three-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Beam Profiles, Data Processing, Radiometer Characterization and Systematic Error Limits
• Dynamical Dark Energy or Simply Cosmic Curvature?
• Thermodynamical description of the interaction between holographic dark energy and dark matter
• Statefinder diagnosis for the interacting model of holographic dark energy
• Agegraphic dark energy as a quintessence
• Holographic tachyon model
• Interacting agegraphic dark energy models in non-flat universe
• Quintessence reconstruction of the new agegraphic dark energy model
• Age Problem in the Holographic Dark Energy Model
• Some Issues Concerning Holographic Dark Energy
• Constraints on holographic dark energy models using the differential ages of passively evolving galaxies
• Holographic dark energy in a cyclic universe
• Thermodynamics of Apparent Horizon in Brane World Scenarios
• Current constraints on interacting holographic dark energy
• Thermodynamics second law and $\omega =-1$ crossing(s) in interacting holographic dark energy model
• Reconstruction of Hessence Dark Energy and the Latest Type Ia Supernovae Gold Dataset
• Inflation with Holographic Dark Energy
• New agegraphic dark energy model with generalized uncertainty principle
• Heal the world: Avoiding the cosmic doomsday in the holographic dark energy model
• Casimir Energy, Holographic Dark Energy and Electromagnetic Metamaterial Mimicking de Sitter
• Reconstructing Quintom from Ricci Dark Energy
• Alleviation of Cosmic Age Problem In Interacting Dark Energy Model
• Possible theoretical limits on holographic quintessence from weak gravity conjecture
• Holographic Dark Energy Model with Hubble Horizon as an IR Cut-off
• 2-loop Quantum Yang-Mills Condensate as Dark Energy
• Holographic Ricci dark energy in Randall-Sundrum braneworld: Avoidance of big rip and steady state future
• Reconstructing $f(R)$ Theory from Ricci Dark Energy
• 3-loop Yang-Mills Condensate Dark Energy Model And Its Cosmological Constraints
• The Coincidence Problem and Interacting Holographic Dark Energy
• Holographic Gas as Dark Energy
• Remarks on Dynamical Dark Energy Measured by the Conformal Age of the Universe
• New Agegraphic Dark Energy in Brans-Dicke Theory
• Holographic Cosmological Constant and Dark Energy
• Holographic dark energy interacting with dark matter in a Closed Universe
• Ricci Dark Energy in Brans-Dicke theory
• Observational Constraints on Agegraphic Dark Energy
• Current observational constraints on holographic dark energy model

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• New holographic scalar field models of dark energy in non-flat universe
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• Constraints on neutrino mass in the scenario of vacuum energy interacting with cold dark matter after Planck 2018
• Reexploration of interacting holographic dark energy model: Cases of interaction term excluding the Hubble parameter
• A new holographic dark energy model in Brans-Dicke theory with logarithmic scalar field
• Statefinder diagnosis for the extended holographic Ricci dark energy model without and with interaction
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• Dark energy versus modified gravity: Impacts on measuring neutrino mass
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