Holographic Ricci dark energy: Current observational constraints, quintom feature, and the reconstruction of scalar-field dark energy

Abstract

In this work, we consider the cosmological constraints on the holographic Ricci dark energy proposed by Gao et al. [Phys. Rev. D 79, 043511 (2009)], by using the observational data currently available. The main characteristic of holographic Ricci dark energy is governed by a positive numerical parameter $\alpha$ in the model. When $\alpha <1/2$, the holographic Ricci dark energy will exhibit a quintomlike behavior; i.e., its equation of state will evolve across the cosmological-constant boundary $w=-1$. The parameter $\alpha$ can be determined only by observations. Thus, in order to characterize the evolving feature of dark energy and to predict the fate of the universe, it is of extraordinary importance to constrain the parameter $\alpha$ by using the observational data. In this paper, we derive constraints on the holographic Ricci dark energy model from the latest observational data including the Union sample of 307 type Ia supernovae, the shift parameter of the cosmic microwave background given by the five-year Wilkinson Microwave Anisotropy Probe observations, and the baryon acoustic oscillation measurement from the Sloan Digital Sky Survey. The joint analysis gives the best-fit results (with 1$\sigma$ uncertainty): $\alpha =0.359_{-0.025}^{+0.024}$ and ${\Omega }_{m0}=0.318_{-0.024}^{+0.026}$. That is to say, according to the observations, the holographic Ricci dark energy takes on the quintom feature. Finally, in light of the results of the cosmological constraints, we discuss the issue of the scalar-field dark energy reconstruction, based on the scenario of the holographic Ricci vacuum energy.

26 pages, 10 figures; published in Phys. Rev. D

References in corpus (119)

• 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
• Dynamics of dark energy
• Five-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Cosmological Interpretation
• 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
• The World as a Hologram
• Cosmological parameters from SDSS and WMAP
• Cosmological Imprint of an Energy Component with General Equation of State
• A Phantom Menace? Cosmological consequences of a dark energy component with super-negative equation of state
• Cosmological Constant - the Weight of the Vacuum
• The Case for a Positive Cosmological Lambda-term
• Cosmology and the Fate of Dilatation Symmetry
• Quintessence, Cosmic Coincidence, and the Cosmological Constant
• The Cosmological Constant
• A Dynamical Solution to the Problem of a Small Cosmological Constant and Late-time Cosmic Acceleration
• A Model of Holographic Dark Energy
• Essentials of k-essence
• Improved Cosmological Constraints from New, Old and Combined Supernova Datasets
• Effective Field Theory, Black Holes, and the Cosmological Constant
• Dark Energy Constraints from the Cosmic Age and Supernova
• The Second Data Release of the Sloan Digital Sky Survey
• Tachyon Matter
• Accelerated expansion of the universe driven by tachyonic matter
• Late-time cosmology in (phantom) scalar-tensor theory: dark energy and the cosmic speed-up
• Unifying phantom inflation with late-time acceleration: scalar phantom-non-phantom transition model and generalized holographic dark energy
• Reconstruction of a scalar-tensor theory of gravity in an accelerating universe
• Ghost Condensation and a Consistent Infrared Modification of Gravity
• Entropy Bounds and Dark Energy
• Cosmological Evolution of a Quintom Model of Dark Energy
• Inhomogeneous Equation of State of the Universe: Phantom Era, Future Singularity and Crossing the Phantom Barrier
• Can dark energy evolve to the Phantom?
• 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
• A New Model of Agegraphic Dark Energy
• Reconciling dark energy models with f(R) theories
• A Holographic Dark Energy Model from Ricci Scalar Curvature
• Prospects for probing the dark energy via supernova distance measurements
• Constraints on holographic dark energy from type Ia supernova observations
• Infrared cut-off proposal for the Holographic density
• The Holographic Dark Energy in a Non-flat Universe
• Scalar-tensor gravity in an accelerating universe
• Dark Energy: Vacuum Fluctuations, the Effective Phantom Phase, and Holography
• Reconstructing the Cosmic Equation of State from Supernova distances
• Observational constraints on dark energy with generalized equations of state
• Comparison of the Legacy and Gold SnIa Dataset Constraints on Dark Energy Models
• Dilatonic ghost condensate as dark energy
• Statefinder diagnostic for holographic dark energy model
• How to determine an effective potential for a variable cosmological term
• New infrared cut-off for the holographic scalar fields models of dark energy
• Robust Dark Energy Constraints from Supernovae, Galaxy Clustering, and Three-Year Wilkinson Microwave Anisotropy Probe Observations
• Interacting holographic dark energy model in non-flat universe
• Constraints on the interacting holographic dark energy model
• Supernova Constraints on a holographic dark energy model
• Dark Energy and Viscous Cosmology
• Observational Constraints on Dark Energy and Cosmic Curvature
• Constraints on linear-negative potentials in quintessence and phantom models from recent supernova data
• Statefinder diagnostic for coupled quintessence
• Constraints on Holographic Dark Energy from Latest Supernovae, Galaxy Clustering, and Cosmic Microwave Background Anisotropy Observations
• Extended Holographic dark energy
• Quintom models with an equation of state crossing -1
• Interacting dark energy, holographic principle and coincidence problem
• Dynamical vacuum energy, holographic quintom, and the reconstruction of scalar-field dark energy
• B-Inflation
• Reconstructing holographic quintessence
• Cosmological Constraints on New Agegraphic Dark Energy
• Two-field Models of Dark Energy with Equation of State Across -1
• Constraints on holographic dark energy from X-ray gas mass fraction of galaxy clusters
• Crossing w=-1 in Gauss-Bonnet Brane World with Induced Gravity
• Statefinder Diagnosis for Ricci Dark Energy
• Constraints on the Dark Energy from the holographic connection to the small l CMB Suppression
• Future supernovae data and quintessence models
• Crossing the Phantom Divide Barrier with Scalar Tensor Theories
• Interacting holographic dark energy model and generalized second law of thermodynamics in non-flat universe
• A Single Scalar Field Model of Dark Energy with Equation of State Crossing -1
• Thermodynamical description of the interaction between holographic dark energy and dark matter
• Coupled Quintessence in a Power-Law Case and the Cosmic Coincidence Problem
• Holographic Dark Energy in Braneworld Models with a Gauss-Bonnet Term in the Bulk. Interacting Behavior and the w =-1 Crossing
• Cosmic Duality in Quintom Universe
• Statefinder diagnosis for the interacting model of holographic dark energy
• Anthropic Principle Favors the Holographic Dark Energy
• Constraints on the dark energy from holography
• Parametrization of Quintessence and Its Potential
• Statefinder diagnosis in a non-flat universe and the holographic model of dark energy
• Parametrizations of the Dark Energy Density and Scalar Potentials
• Quintom model with O($N$) symmetry
• Agegraphic dark energy as a quintessence
• A String-Inspired Quintom Model Of Dark Energy
• Holographic tachyon model
• Determining the Equation of State of the Expanding Universe: Inverse Problem in Cosmology
• Age Problem in the Holographic Dark Energy Model
• Quintessence reconstruction of the new agegraphic dark energy model
• Some Issues Concerning Holographic Dark Energy
• Features of holographic dark energy under the combined cosmological constraints
• Constraints on holographic dark energy models using the differential ages of passively evolving galaxies
• Statefinder parameters for quintom dark energy model
• Holographic dark energy in a cyclic universe
• Tension and Systematics in the Gold06 SnIa Dataset
• Current constraints on interacting holographic dark energy
• Transition from quintessence to phantom phase in quintom model
• Reconstruction of general scalar-field dark energy models
• Inflation with Holographic Dark Energy
• Holography, UV/IR Relation, Causal Entropy Bound and Dark Energy
• New agegraphic dark energy model with generalized uncertainty principle
• Reconstructing Quintom from Ricci Dark Energy
• Possible theoretical limits on holographic quintessence from weak gravity conjecture
• Accelerating cosmologies tested by distance measures
• Testing the DGP model with ESSENCE
• 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
• Dynamics of holographic vacuum energy in the DGP model
• Reduction of Cosmological Data for the Detection of Time-varying Dark Energy Density
• Accelerating Universe and Cosmological Perturbation in the Ghost Condensate
• Reconstructing generalized ghost condensate model with dynamical dark energy parametrizations and observational datasets
• Operational definition of (brane induced) space-time and constraints on the fundamental parameters
• Dark energy due to effective quantum field theory

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• Probing interaction and spatial curvature in the holographic dark energy model
• Unifying Holographic Inflation with Holographic Dark Energy: a Covariant Approach
• Observational constraint on interacting Tsallis holographic dark energy in logarithmic Brans-Dicke theory
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• Search for sterile neutrinos in holographic dark energy cosmology: Reconciling Planck observation with the local measurement of the Hubble constant
• A Modified Holographic Dark Energy Model with Infrared Infinite Extra Dimension(s)
• Comparison of dark energy models after Planck 2015
• Ricci-Gauss-Bonnet holographic dark energy
• Negative cosmological constant in the dark energy sector: tests from JWST photometric and spectroscopic observations of high-redshift galaxies
• Reconstruction and constraining of the jerk parameter from OHD and SNe Ia observations
• Revisit of the Interaction between Holographic Dark Energy and Dark Matter
• Interacting new agegraphic tachyon, K-essence and dilaton scalar field models of dark energy in non-flat universe
• A Critique of Holographic Dark Energy
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• Holographic dark energy in a universe with spatial curvature and massive neutrinos: a full Markov Chain Monte Carlo exploration
• Dynamical analysis and statefinder of Barrow holographic dark energy
• Generalized Holographic and Ricci Dark Energy Models
• Holographic Ricci dark energy: Interacting model and cosmological constraints
• Interacting Ricci Dark Energy with Logarithmic Correction
• Cosmic evolution and thermal stability of Barrow holographic dark energy in nonflat Friedmann-Robertson-Walker Universe
• Observational Constraints to Ricci Dark Energy Model by Using: SN, BAO, OHD, fgas Data Sets
• Holographic Ricci dark energy in Randall-Sundrum braneworld: Avoidance of big rip and steady state future
• Sandage-Loeb test for the new agegraphic and Ricci dark energy models
• New Tsallis Holographic Dark Energy
• Reconstructing interacting entropy-corrected holographic scalar field models of dark energy in non-flat universe
• New agegraphic dark energy as a rolling tachyon
• Cosmic age problem revisited in the holographic dark energy model
• Effects of time-varying $\beta$ in SNLS3 on constraining interacting dark energy models
• Prospect for constraining holographic dark energy with gravitational wave standard sirens from the Einstein Telescope
• Impacts of gravitational-wave standard siren observations from Einstein Telescope and Cosmic Explorer on weighing neutrinos in interacting dark energy models
• Searching for sterile neutrinos in dynamical dark energy cosmologies
• Modified holographic Ricci dark energy coupled to interacting dark matter and a non interacting baryonic component
• Can Holographic dark energy models fit the observational data?
• Model selection and constraints from Holographic dark energy scenarios
• A comprehensive numerical study on four categories of holographic dark energy models
• Cosmology with Ricci dark energy
• A forecast of using fast radio burst observations to constrain holographic dark energy
• Interacting viscous ghost tachyon, K-essence and dilaton scalar field models of dark energy
• Revisit of constraints on holographic dark energy: SNLS3 dataset with the effects of time-varying $\beta$ and different light-curve fitters
• A global fit study on the new agegraphic dark energy model
• Generalized Holographic Dark Energy and its Observational Constraints
• Holographic correspondence of $F(R)$ gravity with/without matter fields
• Probing Cosmic Acceleration by Using the SNLS3 SNIa Dataset
• Interacting entropy-corrected new agegraphic dark energy in non-flat universe
• Comparing holographic dark energy models with statefinder
• A more general interacting model of holographic dark energy
• Reexploration of interacting holographic dark energy model: Cases of interaction term excluding the Hubble parameter
• Redshift drift constraints on holographic dark energy
• Statefinder diagnosis for the extended holographic Ricci dark energy model without and with interaction
• Self-interacting holographic dark energy
• Robust evidence for dynamical dark energy in light of DESI DR2 and joint ACT, SPT, and Planck data
• Interacting Ricci Dark Energy and its Statefinder Description
• A New Type of Dark Energy Model
• Barrow Holographic Dark Energy Model with GO Cut-off -- An Alternative Perspective
• Generalized holographic Ricci dark energy and generalized second law of thermodynamics in Bianchi Type I universe
• Statefinder hierarchy exploration of the extended Ricci dark energy
• QCD modified ghost scalar field dark energy models
• Theoretical Limits on Agegraphic Quintessence from Weak Gravity Conjecture
• Crossing the phantom divide line in the Holographic dark energy model in a closed universe
• Instability in interacting dark sector: An appropriate Holographic Ricci dark energy model
• Effects of a time-varying color-luminosity parameter $\beta$ on the cosmological constraints of modified gravity models
• Multi-fluid cosmology in Einstein gravity: analytical solutions
• Holographic energy density, dark energy sound speed, and tensions in cosmological parameters: $H_0$ and $S_8$
• Constraints on $\Lambda (t)$CDM models as holographic and agegraphic dark energy with the observational Hubble parameter data
• No evidence for the evolution of mass density power-law index $\gamma$ from strong gravitational lensing observation
• Holographic Λ(t)CDM model in a non-flat universe
• Polytropic gas scalar field models of dark energy
• Interacting viscous entropy-corrected holographic scalar field models of dark energy with time-varying G in modified FRW cosmology
• Real-time cosmology with SKA
• Modified holographic Ricci dark energy coupled to interacting relativistic and non-relativistic dark matter in the nonflat universe
• Qualitative analysis and characterization of two cosmologies including scalar fields
• Bayesian Comparison of Interacting Modified Holographic Ricci Dark Energy Scenarios
• Holographic Dark Energy from Acceleration of Particle Horizon
• Barrow Holographic Dark Energy in Brane World Cosmology
• Revisiting the phenomenologically emergent dark energy model: is non-zero equation of state of dark matter favored by DESI DR2?
• Probing Ricci dark energy model with perturbations by using WMAP seven-year cosmic microwave background measurements, BAO and Type Ia supernovae
• Generalized Ricci dark energy in Horava-Lifshitz gravity
• Reconstructing quintom from WMAP 5-year observations: Generalized ghost condensate
• Revisiting holographic dark energy from the perspective of multi-messenger gravitational wave astronomy: future joint observations with short gamma-ray bursts
• New perspectives on future rip scenarios with holographic dark energy
• Quantum Entropy-Driven Modifications to Holographic Dark Energy in $f(G,T)$ Gravity
• Time Variable Cosmological Constant from Renormalization Group Equations
• Measuring neutrino mass in light of ACT DR6 and DESI DR2
• Role of generalized Ricci dark energy on Chameleon field in the emergent universe
• Second order invariants and holography
• Implementation of cosmological bounce inflation with Nojiri-Odintsov generalized holographic dark fluid
• $f(T)$ gravity from holographic Ricci dark energy model with new boundary conditions
• Current observational constraints on holographic dark energy model
• Revisiting Holographic Dark Energy in Cyclic Cosmology
• Entropy Bounds and Holographic Dark Energy: Conflicts and Consensus
• Fomin's conception of quantum cosmogenesis
• "Microscopic" approach to the Ricci dark energy
• Kaniadakis holographic dark energy: observational constraints and global dynamics
• The holographic origin of future singularities and the role of spatial curvature in cosmic expansion
• Power-law holographic dark energy and cosmology
• Resolving the Hubble Tension in the Early Dark Energy Framework with JWST and DESI Data
• Holographic dark energy models with Interactions and entropy corrections for different cutoffs in the Brans-Dicke cosmology
• Modelling the current accelerated expansion of the Universe with Holographic Dark Energy
• Conditional variational autoencoders for cosmological model discrimination and anomaly detection in cosmic microwave background power spectra