Revisit of the Interaction between Holographic Dark Energy and Dark Matter

Abstract

In this paper we investigate the possible direct, non-gravitational interaction between holographic dark energy (HDE) and dark matter. Firstly, we start with two simple models with the interaction terms $Q\propto {\rho }_{dm}$ and $Q\propto {\rho }_{de}$, and then we move on to the general form $Q\propto {\rho }_m^{\alpha }{\rho }_{de}^{\beta }$. The cosmological constraints of the models are obtained from the joint analysis of the present Union2.1+BAO+CMB+$H_0$ data. We find that the data slightly favor an energy flow from dark matter to dark energy, although the original HDE model still lies in the 95.4% confidence level (CL) region. For all models we find $c<1$ at the 95.4% CL. We show that compared with the cosmic expansion, the effect of interaction on the evolution of ${\rho }_{dm}$ and ${\rho }_{de}$ is smaller, and the relative increment (decrement) amount of the energy in the dark matter component is constrained to be less than 9% (15%) at the 95.4% CL. By introducing the interaction, we find that even when $c<1$ the big rip still can be avoided due to the existence of a de Sitter solution at $z\to -1$. We show that this solution can not be accomplished in the two simple models, while for the general model such a solution can be achieved with a large $\beta$, and the big rip may be avoided at the 95.4% CL.

arXiv comment26 pages, 9 figures, version accepted for publication in JCAP

References in corpus (91)

• 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
• 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
• The Cosmological Constant and Dark Energy
• First Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Preliminary Maps and Basic Results
• Detection of the Baryon Acoustic Peak in the Large-Scale Correlation Function of SDSS Luminous Red Galaxies
• Cosmological parameters from SDSS and WMAP
• Cosmological parameters from CMB and other data: a Monte-Carlo approach
• Cosmological Constant - the Weight of the Vacuum
• The Case for a Positive Cosmological Lambda-term
• The 6dF Galaxy Survey: Baryon Acoustic Oscillations and the Local Hubble Constant
• Baryonic Features in the Matter Transfer Function
• Dark Energy and the Accelerating Universe
• A Model of Holographic Dark Energy
• Baryon Acoustic Oscillations in the Sloan Digital Sky Survey Data Release 7 Galaxy Sample
• The 3D power spectrum of galaxies from the SDSS
• The Hubble Space Telescope Cluster Supernova Survey: V. Improving the Dark Energy Constraints Above z>1 and Building an Early-Type-Hosted Supernova Sample
• A 3% Solution: Determination of the Hubble Constant with the Hubble Space Telescope and Wide Field Camera 3
• 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
• The 6dF Galaxy Survey: Final Redshift Release (DR3) and Southern Large-Scale Structures
• The WiggleZ Dark Energy Survey: mapping the distance-redshift relation with baryon acoustic oscillations
• Small Scale Cosmological Perturbations: An Analytic Approach
• Unifying phantom inflation with late-time acceleration: scalar phantom-non-phantom transition model and generalized holographic dark energy
• Dark Energy
• Reconstructing Dark Energy
• Transition of the dark energy equation of state in an interacting holographic dark energy model
• A Dark Energy Model Characterized by the Age of the Universe
• The WiggleZ Dark Energy Survey: Survey Design and First Data Release
• A Holographic Dark Energy Model from Ricci Scalar Curvature
• Constraints on holographic dark energy from type Ia supernova observations
• The Holographic Dark Energy in a Non-flat Universe
• Comparison of the Legacy and Gold SnIa Dataset Constraints on Dark Energy Models
• The Hubble Constant
• Dynamics of dark energy with a coupling to dark matter
• Statefinder diagnostic for holographic dark energy model
• Constraints on the interacting holographic dark energy model
• Supernova Constraints on a holographic dark energy model
• Holographic dark energy models: A comparison from the latest observational data
• Entropy Bounds and Black Hole Remnants
• Constraints on linear-negative potentials in quintessence and phantom models from recent supernova data
• Constraints on Holographic Dark Energy from Latest Supernovae, Galaxy Clustering, and Cosmic Microwave Background Anisotropy Observations
• Dynamical vacuum energy, holographic quintom, and the reconstruction of scalar-field dark energy
• Reconstructing $f(R,T)$ gravity from holographic dark energy
• Holographic Ricci dark energy: Current observational constraints, quintom feature, and the reconstruction of scalar-field dark energy
• Reconstructing holographic quintessence
• Constraints on holographic dark energy from X-ray gas mass fraction of galaxy clusters
• Constraints on the Dark Energy from the holographic connection to the small l CMB Suppression
• 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
• Probing interaction and spatial curvature in the holographic dark energy model
• Observational Constraints on Cosmological Models with the Updated Long Gamma-Ray Bursts
• Statefinder diagnosis for the interacting model of holographic dark energy
• Statefinder Diagnostic and w-w' Analysis for the Agegraphic Dark Energy Models without and with Interaction
• Anthropic Principle Favors the Holographic Dark Energy
• Constraints on the dark energy from holography
• Quantum UV/IR Relations and Holographic Dark Energy from Entropic Force
• Holographic tachyon 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
• Features of holographic dark energy under the combined cosmological constraints
• Observational constraints on phantom-like braneworld cosmologies
• Holographic dark energy in a cyclic universe
• Tension and Systematics in the Gold06 SnIa Dataset
• Comparison of dark energy models: A perspective from the latest observational data
• Thermodynamics second law and $\omega =-1$ crossing(s) in interacting holographic dark energy model
• A Modified Holographic Dark Energy Model with Infrared Infinite Extra Dimension(s)
• On using the CMB shift parameter in tests of models of dark energy
• Inflation with Holographic Dark Energy
• Heal the world: Avoiding the cosmic doomsday in the holographic dark energy model
• Casimir Energy, Holographic Dark Energy and Electromagnetic Metamaterial Mimicking de Sitter
• Dark energy from vacuum entanglement
• Possible theoretical limits on holographic quintessence from weak gravity conjecture
• Holographic Ricci dark energy: Interacting model and cosmological constraints
• Revisit of cosmic age problem
• Interacting model of new agegraphic dark energy: observational constraints and age problem
• Holographic Ricci dark energy in Randall-Sundrum braneworld: Avoidance of big rip and steady state future
• Present Acceleration of Universe, Holographic Dark Energy and Brans-Dicke Theory
• More studies on Metamaterials Mimicking de Sitter space
• Holographic Gas as Dark Energy
• Holographic Cosmological Constant and Dark Energy
• Cosmic age test in inhomogeneous cosmological models mimicking $\Lambda$CDM on the light cone
• Holographic interacting dark energy in the braneworld cosmology
• Density perturbations in decaying holographic dark energy models
• Age problem in holographic dark energy

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• Probing the interaction between dark energy and dark matter with future fast radio burst observations
• Constraints on neutrino mass in the scenario of vacuum energy interacting with cold dark matter after Planck 2018
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• Cosmic sign-reversal: non-parametric reconstruction of interacting dark energy with DESI DR2
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• Differentiating dark interactions with perturbation
• Cosmological constraints on the new holographic dark energy model with action principle
• Density perturbation in an interacting holographic dark energy model
• Forecast Analysis on Interacting Dark Energy Models from Future Generation PICO and DESI Missions
• Rényi Holographic Dark Energy
• Prospects for weighing neutrinos in interacting dark energy models using joint observations of gravitational waves and $\gamma$-ray bursts
• Interacting Agegraphic Dark Energy Model in DGP Braneworld Cosmology: Dynamical System Approach
• Revisiting the phenomenologically emergent dark energy model: is non-zero equation of state of dark matter favored by DESI DR2?
• Holographic Dark Energy from the Anti-de Sitter Black Hole
• Measuring neutrino mass in light of ACT DR6 and DESI DR2
• Perturbation in an interacting dark universe
• Multicomponent holographic dark energy model with generalized entropy
• Generalized Semi-Holographic Universe
• How Holographic is the Dark Energy? A Spline Nodal reconstruction approach
• Conditional variational autoencoders for cosmological model discrimination and anomaly detection in cosmic microwave background power spectra