A Lower Growth Rate from Recent Redshift Space Distortion Measurements than Expected from Planck
arXiv:1303.6583 · doi:10.1103/PhysRevLett.111.161301
Abstract
We perform a meta-study of recently published Redshift Space Distortion (RSD) measurements of the cosmological growth rate, f(z) σ_8(z). We analyse the latest results from the 6dFGS, BOSS, LRG, WiggleZ and VIPERS galaxy redshift surveys, and compare the measurements to expectations from Planck. In this Letter we point out that the RSD measurements are consistently lower than the values expected from Planck, and the relative scatter between the RSD measurements is lower than expected. A full resolution of this issue may require a more robust treatment of non-linear effects in RSD models, although the trend for a low σ_8 agrees with recent constraints on σ_8 and Ω_m from Sunyaev-Zeldovich cluster counts identified in Planck.
4 pages, 1 figure, updated to match version accepted in PRL
References in corpus (10)
- A test of the nature of cosmic acceleration using galaxy redshift distortions
- Confirmation of general relativity on large scales from weak lensing and galaxy velocities
- Testing cosmological structure formation using redshift-space distortions
- The WiggleZ Dark Energy Survey: Final data release and cosmological results
- The 2dF-SDSS LRG and QSO Survey: QSO clustering and the L-z degeneracy
- The 2dF-SDSS LRG and QSO Survey: The LRG 2-Point Correlation Function and Redshift-Space Distortions
- Redshift space distortions in f(R) gravity
- Modelling redshift space distortions in hierarchical cosmologies
- The Atacama Cosmology Telescope: Cross-Correlation of CMB Lensing and Quasars
- How Baryonic Processes affect Strong Lensing properties of Simulated Galaxy Clusters
Cited by in corpus (224)
- Beyond the Cosmological Standard Model
- Challenges for CDM: An update
- Dark Matter and Dark Energy Interactions: Theoretical Challenges, Cosmological Implications and Observational Signatures
- Beyond CDM: Problems, solutions, and the road ahead
- Planck 2015 results. XIV. Dark energy and modified gravity
- The clustering of galaxies in the SDSS-III Baryon Oscillation Spectroscopic Survey: RSD measurement from the power spectrum and bispectrum of the DR12 BOSS galaxies
- First evidence that non-metricity f(Q) gravity could challenge CDM
- Cosmology with Phase 1 of the Square Kilometre Array; Red Book 2018: Technical specifications and performance forecasts
- The Clustering of Galaxies in the SDSS-III Baryon Oscillation Spectroscopic Survey (BOSS): measuring growth rate and geometry with anisotropic clustering
- Small scale problems of the CDM model: a short review
- First Cosmological Results using Type Ia Supernovae from the Dark Energy Survey: Measurement of the Hubble Constant
- Constraints on the sum of the neutrino masses in dynamical dark energy models with are tighter than those obtained in CDM
- Evolution of the tension with the Planck15/CDM determination and implications for modified gravity theories
- Tension and constraints on modified gravity parametrizations of from growth rate and Planck data
- Modified theories of Gravity: Why, How and What?
- Reconciling CMB and structure growth measurements with dark energy interactions
- Testing gravity with redshift space distortions
- Signatures of -gravity in cosmology
- A non-linear solution to the tension?
- Tension, Phantom Dark Energy and Cosmological Parameter Degeneracies
- Cosmological Tests of Gravity
- Update on Coupled Dark Energy and the tension
- Possible signals of vacuum dynamics in the Universe
- Precision cosmology with Padé rational approximations: theoretical predictions versus observational limits
- Holographic dark energy from nonadditive entropy: cosmological perturbations and observational constraints
- A rapid transition of at as a solution of the Hubble and growth tensions
- Stable and unstable cosmological models in bimetric massive gravity
- Exploring Cosmic Origins with CORE: Cosmological Parameters
- Effective gravitational couplings for cosmological perturbations in generalized Proca theories
- Cosmological constraints on interacting dark energy with redshift-space distortion after Planck data
- Constraints on the interacting vacuum -- geodesic CDM scenario
- The clustering of galaxies in the completed SDSS-III Baryon Oscillation Spectroscopic Survey: On the measurement of growth rate using galaxy correlation functions
- Growth rate of cosmological perturbations at z ~ 0.1 from a new observational test
- A phantom transition at as a resolution of the Hubble tension
- Dynamical dark energy versus const. in light of observations
- Density perturbations for running vacuum: a successful approach to structure formation and to the -tension
- Bayesian analysis of gravity using data
- Extending cosmological tests of General Relativity with the Square Kilometre Array
- Dark compact objects: an extensive overview
- Internal Robustness of Growth Rate data
- Cosmology with the EFTofLSS and BOSS: dark energy constraints and a note on priors
- Hints of a Local Matter Underdensity or Modified Gravity in the Low Pantheon data
- The impact of the cosmic variance on on cosmological analyses
- Testing coupled dark energy with large scale structure observation
- What are and diagnostics telling us in light of data?
- Late-transition vs smooth deformation models for the resolution of the Hubble crisis
- Late time approaches to the Hubble tension deforming , worsen the growth tension
- Cosmological Hints of Modified Gravity ?
- Reconciling tension in a six parameter space?
- Chasing the phantom: A closer look at Type Ia supernovae and the dark energy equation of state
- Is cosmic acceleration proven by local cosmological probes?
- Brans-Dicke cosmology with a - term: a possible solution to CDM tensions
- Coupled quintessence with a CDM background: removing the tension
- Tension of the statistic and RSD data with Planck/CDM and implications for weakening gravity
- Observational constraints on the deceleration parameter in a tilted universe
- Effects of modified gravity on B-mode polarization
- Running vacuum in the Universe: phenomenological status in light of the latest observations, and its impact on the and tensions
- Stringent constraints from small-scale galaxy clustering using a hybrid MCMC+emulator framework
- Instability in a minimal bimetric gravity model
- Can dark energy be expressed as a power series of the Hubble parameter?
- Cosmological constraints on late-universe decaying dark matter as a solution to the tension
- Scalar-field dark energy nonminimally and kinetically coupled to dark matter
- Relaxing the -tension through running vacuum in the Universe
- Post- constraints on interacting vacuum energy
- Coupled and uncoupled early dark energy, massive neutrinos and the cosmological tensions
- Linear growth of structure in massive bigravity
- Coupled dark energy with perturbed Hubble expansion rate
- Banana Split: Testing the Dark Energy Consistency with Geometry and Growth
- Can gravity resolve the tension?
- The clustering of galaxies in the completed SDSS-III Baryon Oscillation Spectroscopic Survey: constraining modified gravity
- Cosmic viscosity as a remedy for tension between PLANCK and LSS data
- Galaxy and Mass Assembly (GAMA): Redshift Space Distortions from the Clipped Galaxy Field
- Probing elastic interactions in the dark sector and the role of
- Planck intermediate results. XXXVII. Evidence of unbound gas from the kinetic Sunyaev-Zeldovich effect
- Cosmography approach to dark energy cosmologies: new constrains using the Hubble diagrams of supernovae, quasars and gamma-ray bursts
- The Linear Growth of Structure in the R_h=ct Universe
- Peculiar Velocity Decomposition, Redshift Space Distortion and Velocity Reconstruction in Redshift Surveys. II. Dark Matter Velocity Statistics
- The missing link: a nonlinear post-Friedmann framework for small and large scales
- Cosmographic parameters in model-independent approaches
- Testing the effect of on tension using a Gaussian Process method
- Comparison between different methods of model selection in cosmology
- Searching for Modified Gravity: Scale and Redshift Dependent Constraints from Galaxy Peculiar Velocities
- CDM Tensions: Localising Missing Physics through Consistency Checks
- Reconstructing teleparallel gravity with cosmic structure growth and expansion rate data
- Testing Dark energy models in the light of tension
- Hints of Modified Gravity in Cosmos and in the Lab?
- Constraints on modified gravity from Planck 2015: when the health of your theory makes the difference
- increases with effective redshift in CDM cosmology
- A Bayesian comparison between CDM and phenomenologically emergent dark energy models
- Cosmological constraints from a joint analysis of cosmic growth and expansion
- Weakening Gravity on Redshift-Survey Scales with Kinetic Matter Mixing
- Structure formation simulations with momentum exchange: alleviating tensions between high-redshift and low-redshift cosmological probes
- Possibility of realizing weak gravity in redshift space distortion measurements
- Cosmology in beyond-generalized Proca theories
- Cosmological perturbations in the Tsallis holographic dark energy scenarios
- Parametrizing modified gravity for cosmological surveys
- Revisiting a non-parametric reconstruction of the deceleration parameter from combined background and the growth rate data
- Cosmological perturbations in an effective and genuinely phantom dark energy Universe
- Cosmology Intertwined: A Review of the Particle Physics, Astrophysics, and Cosmology Associated with the Cosmological Tensions and Anomalies
- The Hubble Tension, The Crisis of Late Time Deformation Models and the Reconstruction of Quintessence Lagrangians
- Machine learning constraints on deviations from general relativity from the large scale structure of the Universe
- The radial acceleration relation in galaxy clusters
- Weak cosmic growth in coupled dark energy with a Lagrangian formulation
- Graviton mass might reduce tension between early and late time cosmological data
- Toward a concordance teleparallel Cosmology I: Background Dynamics
- No-go guide for late-time solutions to the Hubble tension: Matter perturbations
- Dynamical systems methods and statefinder diagnostic of interacting vacuum energy models
- Consistency of Modified Gravity with a decreasing in a CDM background
- Constraining spatial curvature with large-scale structure
- Post-Planck Dark Energy Constraints
- Non-linear contributions to angular power spectra
- Measurement of marked correlation functions in SDSS-III Baryon Oscillation Spectroscopic Survey using LOWZ galaxies in Data Release 12
- Velocity-dependent interacting dark energy and dark matter with a Lagrangian description of perfect fluids
- Does Quartessence Ease Tensions?
- Constraining power of cosmological observables: blind redshift spots and optimal ranges
- Gravitational transitions via the explicitly broken symmetron screening mechanism
- Kinetically coupled dark energy
- Torsion in string-inspired cosmologies and the universe dark sector
- Growth Index after the Planck Results
- Redshift space power spectrum beyond Einstein-de Sitter kernels
- Cosmological constraints on non-adiabatic dark energy perturbations
- Testing the warmness of dark matter
- Coupled Multi-Proca Vector Dark Energy
- Constraints on a decomposed dark fluid with constant adiabatic sound speed by jointing the geometry test and growth rate after Planck data
- Hints for possible low redshift oscillation around the best fit CDM model in the expansion history of the Universe
- Power spectrum multipole expansion for HI intensity mapping experiments: unbiased parameter estimation
- Suppressed cosmic growth in coupled vector-tensor theories
- The growth index of matter perturbations using the clustering of dark energy
- Forecasted constraints on modified gravity from Sunyaev Zel'dovich tomography
- Confronting DGP Braneworld Gravity with Cosmic Observations after Planck Data
- Alleviating Cosmological Tensions with a Coupled Scalar Fields Model
- Mass-Temperature relation in CDM and modified gravity
- The Aemulus Project VI: Emulation of beyond-standard galaxy clustering statistics to improve cosmological constraints
- Redshift-space distortions of galaxies, clusters and AGN: testing how the accuracy of growth rate measurements depends on scales and sample selections
- Running vacuum versus Holographic dark energy: a cosmographic comparison
- Spatial Curvature in Gravity
- Extended CDM model
- Alleviating the Hubble-constant tension and the growth tension via a transition of absolute magnitude favored by the Pantheon+ sample
- A cosmological exclusion plot: Towards model-independent constraints on modified gravity from current and future growth rate data
- Can gravity relieve and tensions?
- The Tension in Light of Updated Redshift-Space Distortion Data and PAge Approximation
- Observational Constraints on Growth Index with Cosmography
- Extended CDM model and viscous dark energy: A Bayesian analysis
- Constraining constant and tomographic coupled dark energy with low-redshift and high-redshift probes
- Modelling Non-Linear Effects of Dark Energy
- Cosmological disformal transformations to the Einstein frame and gravitational couplings with matter perturbations
- Linear Perturbation constraints on Multi-coupled Dark Energy
- No evidence for dynamical dark energy in two models
- Bounds on Neutrino Mass in Viscous Cosmology
- Differentiating dark interactions with perturbation
- Model-independent constraints on modified gravity from current data and from the Euclid and SKA future surveys
- Relationship between the CMB, SZ Cluster Counts, and Local Hubble Parameter Measurements in a Simple Void Model
- Growth of structures and redshift-space distortion data in scale-dependent gravity
- On the tension between growth rate and CMB data
- Testing the tensor-vector-scalar Theory with the latest cosmological observations
- Scalar Field Theory Description of the Running Vacuum Model: the Vacuumon
- Kinetically Coupled Scalar Fields Model and Cosmological Tensions
- Horndeski dark matter and beyond
- Holographic energy density, dark energy sound speed, and tensions in cosmological parameters: and
- Is gravity getting weaker at low z? Observational evidence and theoretical implications
- Constraining the growth of perturbations with lensing of supernovae
- Anisotropic Scalar Field Dark Energy with a Disformally Coupled Yang-Mills Field
- Conformally and Disformally Coupled Vector field Models of Dark Energy
- Linear matter density perturbations in the CDM model: Examining growth dynamics and addressing the tension
- Assessing non-linear models for galaxy clustering II: model validation and forecasts for Stage IV surveys
- Assessing non-linear models for galaxy clustering III: Theoretical accuracy for Stage IV surveys
- Observational constraints on interactions between dark energy and dark matter with momentum and energy transfers
- Testing the Universe Jointly with the Redshift-dependent Expansion rate and Angular-diameter and Luminosity Distances
- Weak gravity on a CDM background
- Linear Density Perturbations in Multifield Coupled Quintessence
- Cosmological framework for renormalization group extended gravity at the action level
- On the uniqueness of CDM-like evolution for homogeneous and isotropic cosmology in General Relativity
- Cosmological constraints with the Effective Fluid approach for Modified Gravity
- Cosmological Fisher forecasts for next-generation spectroscopic surveys
- Data-driven and Almost Model-independent Reconstruction of Modified Gravity
- Coupled Dark Sector Models and Cosmological Tensions
- The interacting vacuum and tensions: a comparison of theoretical models
- CDM as a Noether Symmetry in Cosmology
- Lagrangian formulation for an extended cosmological equation-of-state
- First and second order cosmological perturbations in light mass Galileon models
- Interacting dark energy axions in light of the Hubble tension
- Consistency of Cubic Galileon Cosmology: Model-Independent Bounds from Background Expansion and Perturbative Analyses
- Spherical collapse in coupled quintessence with a CDM background
- Clustering GCG: a viable option for unified dark matter-dark energy?
- Tracking the validity of the quasi-static and sub-horizon approximations in modified gravity
- Interacting parametrized post-Friedmann method
- The CIDER simulations: Nonlinear structure formation in the Constrained Interacting Dark Energy Scenario
- Difficulties in reconciling non-negligible differences between the local and cosmological values of the gravitational coupling in extended Brans-Dicke theories
- Is there evidence for CIDER in the Universe?
- Precise peculiar velocities from gravitational waves accompanied by electromagnetic signals and cosmological applications
- Non-linear Structure Formation for Dark Energy Models with a Steep Equation of State
- Limit on the dark matter mass from its interaction with photons
- Reconstructing the parameter space of non-analytical cosmological fixed points
- Endowing with a dynamic nature: constraints in a spatially curved Universe
- Cosmological Evolution in Bimetric Gravity: Observational Constraints and LSS Signatures
- Can the cosmological dark sector be modeled by a single scalar field?
- Non-linear density-velocity dynamics in gravity from spherical collapse
- Non-Linearity-Free prediction of the growth-rate using Convolutional Neural Networks
- Implications of Dynamical Dark Energy in the expansion of the Universe and the Structure Formation
- Effective field theory of coupled dark energy and dark matter
- Linear growth of structure in projected massive gravity
- Early dark energy in the pre- and post-recombination epochs
- Confronting dark energy in Harada's Conformal Killing Gravity with observational data
- ParamANN: A Neural Network to Estimate Cosmological Parameters for CDM Universe Using Hubble Measurements
- Vainshtein screening in Horndeski theories nonminimally and kinetically coupled to ordinary matter
- The RSD Sorting Hat: Unmixing Radial Scales in Projection
- Cluster density slopes from Dark Matter-Baryons Energy Transfer
- Effect of redshift bin mismatch on cross correlation between DESI Legacy Imaging Survey and Planck CMB lensing potential
- The Effect of Primordial Anti-Biasing on the Local Measurement of the Key Cosmological Parameters
- On Direct Estimation of Density Parameters and Hubble Constant for CDM Universe using Hubble Measurements
- Towards a Composite Framework for Simultaneous Exploration of New Physics in Background and Perturbed Universe
- Exploring Late-Time Cosmic Acceleration in VCDM Cosmology
- Evolution of linear matter perturbations with error-bounded bundle physics-informed neural networks
- Assessing the potential of cluster edges as a standard ruler
- The and tensions necessitate early and late time changes to CDM
- On the absence of a universal surface density, and a maximum Newtonian acceleration in dark matter haloes: consequences for MOND
- Perturbations In Some Dark Energy Models
- Interacting dark energy from redshift-space galaxy clustering
- Dynamical friction shear and rotation in Chaplygin cosmology
- Observational Constraints and Geometric Diagnostics of Barboza-Alcaniz and Logarithmic Dark Energy Parametrizations
- Does Holographic equipartition demand a pure cosmological constant?
- An effective fluid description of scalar-vector-tensor theories under the sub-horizon and quasi-static approximations
- Evolution of matter perturbations in the context of cosmic slowing down
- The Covariance of Photometric and Spectroscopic Two-Point Statistics: Implications for Cosmological Parameter Inference