Model selection and constraints from Holographic dark energy scenarios

Abstract

In this study we combine the expansion and the growth data in order to investigate the ability of the three most popular holographic dark energy models, namely event future horizon, Ricci scale and Granda-Oliveros IR cutoffs, to fit the data. Using a standard ${\chi }^2$ minimization method we place tight constraints on the free parameters of the models. Based on the values of the Akaike and Bayesian information criteria we find that two out of three holographic dark energy models are disfavored by the data, because they predict a non-negligible amount of dark energy density at early enough times. Although the growth rate data are relatively consistent with the holographic dark energy models which are based on Ricci scale and Granda-Oliveros IR cutoffs, the combined analysis provides strong indications against these models. Finally, we find that the model for which the holographic dark energy is related with the future horizon is consistent with the combined observational data.

arXiv comment13 Pages, 7 Figures and 9 Tables. Accepted in MNRAS

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
• Dynamics of dark energy
• The Cosmological Constant and Dark Energy
• Nine-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Cosmological Parameter Results
• The World as a Hologram
• Cosmological parameters from SDSS and WMAP
• Cosmological Constant - the Weight of the Vacuum
• The 6dF Galaxy Survey: Baryon Acoustic Oscillations and the Local Hubble Constant
• The Cosmological Constant
• A Dynamical Solution to the Problem of a Small Cosmological Constant and Late-time Cosmic Acceleration
• Dark Energy and the Accelerating Universe
• A Model of Holographic Dark Energy
• k-Inflation
• The clustering of galaxies in the SDSS-III Baryon Oscillation Spectroscopic Survey: Baryon Acoustic Oscillations in the Data Release 10 and 11 galaxy samples
• The Hubble Space Telescope Cluster Supernova Survey: V. Improving the Dark Energy Constraints Above z>1 and Building an Early-Type-Hosted Supernova Sample
• Effective Field Theory, Black Holes, and the Cosmological Constant
• Constraints on the redshift dependence of the dark energy potential
• A 6% measurement of the Hubble parameter at $z\sim 0.45$: direct evidence of the epoch of cosmic re-acceleration
• Cosmic Chronometers: Constraining the Equation of State of Dark Energy. I: H(z) Measurements
• Perturbations in k-inflation
• Raising the bar: new constraints on the Hubble parameter with cosmic chronometers at z$\sim$2
• Information criteria for astrophysical model selection
• Improved constraints on the expansion rate of the Universe up to z~1.1 from the spectroscopic evolution of cosmic chronometers
• The WiggleZ Dark Energy Survey: mapping the distance-redshift relation with baryon acoustic oscillations
• The WiggleZ Dark Energy Survey: Joint measurements of the expansion and growth history at z < 1
• Unifying phantom inflation with late-time acceleration: scalar phantom-non-phantom transition model and generalized holographic dark energy
• The clustering of galaxies in the SDSS-III Baryon Oscillation Spectroscopic Survey: Baryon Acoustic Oscillations in the Data Release 9 Spectroscopic Galaxy Sample
• Entropy Bounds and Dark Energy
• A 2% Distance to z=0.35 by Reconstructing Baryon Acoustic Oscillations - I : Methods and Application to the Sloan Digital Sky Survey
• Holographic dark energy and cosmic coincidence
• Clustering of Luminous Red Galaxies IV: Baryon Acoustic Peak in the Line-of-Sight Direction and a Direct Measurement of H(z)
• Constraints on the equation of state of dark energy and the Hubble constant from stellar ages and the CMB
• The WiggleZ Dark Energy Survey: the growth rate of cosmic structure since redshift z=0.9
• Big-Bang Nucleosynthesis Predictions for Precision Cosmology
• A Holographic Dark Energy Model from Ricci Scalar Curvature
• Probable Values of the Cosmological Constant in a Holographic Theory
• Infrared cut-off proposal for the Holographic density
• Reconstructing the history of structure formation using redshift distortions
• Interpreting large-scale redshift-space distortion measurements
• Probing dark energy perturbations: the dark energy equation of state and speed of sound as measured by WMAP
• Reconstruction of $f(T)$ gravity: Rip cosmology, finite-time future singularities and thermodynamics
• Constraints on the interacting holographic dark energy model
• The Clustering of the SDSS Main Galaxy Sample II: Mock galaxy catalogues and a measurement of the growth of structure from Redshift Space Distortions at $z=0.15$
• Supernova Constraints on a holographic dark energy model
• Cosmic flows in the nearby universe from Type Ia Supernovae
• The Subaru FMOS galaxy redshift survey (FastSound). IV. New constraint on gravity theory from redshift space distortions at $z\sim 1.4$
• Cosmology and Astrophysical Constraints of Gauss-Bonnet Dark Energy
• Large-scale Structure in f(T) Gravity
• Galaxy And Mass Assembly (GAMA): improved cosmic growth measurements using multiple tracers of large-scale structure
• Entropic Accelerating Universe
• Tension and constraints on modified gravity parametrizations of $G_{\text{eff}}(z)$ from growth rate and Planck data
• Hubble expansion & Structure Formation in Time Varying Vacuum Models
• The VIMOS Public Extragalactic Redshift Survey (VIPERS): The growth of structures at $0.5<z<1.2$ from redshift-space distortions in the clustering of the PDR-2 final sample
• Holographic Ricci dark energy: Current observational constraints, quintom feature, and the reconstruction of scalar-field dark energy
• The clustering of galaxies in the SDSS-III Baryon Oscillation Spectroscopic Survey: single-probe measurements and the strong power of normalized growth rate on constraining dark energy
• Local Gravity versus Local Velocity: Solutions for $\beta$ and nonlinear bias
• 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
• Measuring the Speed of Sound of Quintessence
• The clustering of galaxies in the SDSS-III Baryon Oscillation Spectroscopic Survey: cosmological implications of the full shape of the clustering wedges in the data release 10 and 11 galaxy samples
• The growth rate of cosmic structure from peculiar velocities at low and high redshifts
• Testing $\Lambda$CDM at the lowest redshifts with SN Ia and galaxy velocities
• Structure formation in the presence of dark energy perturbations
• The clustering of galaxies in the SDSS-III Baryon Oscillation Spectroscopic Survey: single-probe measurements from CMASS anisotropic galaxy clustering
• Interacting holographic dark energy
• ISIS: a new N-body cosmological code with scalar fields based on RAMSES. Code presentation and application to the shapes of clusters
• Constraining dark energy with cross-correlated CMB and Large Scale Structure data
• Planck Constraints on Holographic Dark Energy
• Constraining Dark Energy Anisotropic Stress
• Releasing scalar fields: cosmological simulations of scalar-tensor theories for gravity beyond the static approximation
• Measuring the Speed of Dark: Detecting Dark Energy Perturbations
• Measuring Dark Energy Clustering with CMB-Galaxy Correlations
• Growth rate of cosmological perturbations at z ~ 0.1 from a new observational test
• Constraints on holographic dark energy models using the differential ages of passively evolving galaxies
• Features of holographic dark energy under the combined cosmological constraints
• Physical approximations for the nonlinear evolution of perturbations in dark energy scenarios
• Observational constraints on holographic tachyonic dark energy in interaction with dark matter
• Chasing the phantom: A closer look at Type Ia supernovae and the dark energy equation of state
• Structure formation in inhomogeneous Early Dark Energy models
• No Evidence for Dark Energy Dynamics from a Global Analysis of Cosmological Data
• Entropic-force dark energy reconsidered
• Comparison of dark energy models after Planck 2015
• Entropic Inflation
• Chameleon dark energy models with characteristic signatures
• Confronting Dark Energy Models using Galaxy Cluster Number Counts
• A comparison of structure formation in minimally and non-minimally coupled quintessence models
• Effects of shear and rotation on the spherical collapse model for clustering dark energy
• The WiggleZ Dark Energy Survey: measuring the cosmic growth rate with the two-point galaxy correlation function
• Cosmology of the selfaccelerating third order Galileon
• How clustering dark energy affects matter perturbations
• The spherical collapse model and cluster formation beyond the $\Lambda$ cosmology: Indications for a clustered dark energy?
• Neutrinos in the holographic dark energy model: constraints from latest measurements of expansion history and growth of structure
• Structure formation in cosmologies with oscillating dark energy
• Growth Rate of Large Scale Structure as a Powerful Probe of Dark Energy
• Linear growth in power law $f(T)$ gravity
• Holographic principle and the dominant energy condition for Kasner type metrics
• On the Magnitude of Dark Energy Voids and Overdensities
• The growth index of matter perturbations and modified gravity
• Dynamical Mutation of Dark Energy
• Growth of matter perturbations in clustered holographic dark energy cosmologies
• Constraints on the Holographic Dark Energy Model from Type Ia Supernovae, WMAP7, Baryon Acoustic Oscillation and Redshift-Space Distortion
• Fingerprinting Dark Energy III: distinctive marks of viscosity
• The impact of dark energy perturbations on the growth index
• Effects of Dark Energy Perturbations on Cosmological Tests of General Relativity
• Revisiting the holographic dark energy in a non-flat universe: alternative model and cosmological parameter constraints
• Agegraphic dark energy: growth index and cosmological implications
• Gravitational collapse of k-essence
• Evolution of spherical overdensities in holographic dark energy models
• Effects of ghost dark energy perturbations on the evolution of spherical overdensities
• Generalized Holographic Dark Energy and its Observational Constraints
• The WiggleZ Dark Energy Survey: constraining the evolution of Newton's constant using the growth rate of structure
• Growth of spherical overdensities in scalar-tensor cosmologies
• Constraints on a decomposed dark fluid with constant adiabatic sound speed by jointing the geometry test and growth rate after Planck data
• The growth index of matter perturbations using the clustering of dark energy
• Constraints on shear and rotation with massive galaxy clusters
• Discriminating dark energy models by using the statefinder hierarchy and the growth rate of matter perturbations
• Constraints from growth-rate data on some coupled dark energy models mimicking a $\Lambda CDM$ expansion
• Cosmological constraints on holographic dark energy models under the energy conditions

Cited by in corpus (21)

• Can dark energy be expressed as a power series of the Hubble parameter?
• Dynamical analysis and statefinder of Barrow holographic dark energy
• Cosmological perturbations in the Tsallis holographic dark energy scenarios
• Can Holographic dark energy models fit the observational data?
• A forecast of using fast radio burst observations to constrain holographic dark energy
• Modeling holographic dark energy with particle and future horizons
• Corrected holographic dark energy with power-law entropy and Hubble Horizon cut-off in FRW Universe
• RHDE models in FRW Universe with two IR cut-offs with redshift parametrization
• Differentiating dark interactions with perturbation
• Forecast Analysis on Interacting Dark Energy Models from Future Generation PICO and DESI Missions
• Barrow entropic Quintessence and Dilation dark energy Models with Generalized HDE cut-off
• Holographic energy density, dark energy sound speed, and tensions in cosmological parameters: $H_0$ and $S_8$
• Renyi Holographic Dark Energy models in Teleparallel gravity
• Bayesian Comparison of Interacting Modified Holographic Ricci Dark Energy Scenarios
• Holographic inflation and holographic dark energy from entropy of the anti-de Sitter black hole
• Dynamics of holographic dark energy with apparent-horizon cutoff and non-minimal derivative coupling gravity in non-flat FLRW universe
• Cosmology in holographic non-minimal derivative coupling theory: constraints from inflation and variation of gravitational constant
• Observational constraints on thawing quintessence scalar field model
• Agegraphic dark energy from entropy of the anti-de Sitter black hole
• Perturbations In Some Dark Energy Models
• Primordial gravitational waves: Model effects on time evolution and spectrum