Cosmic Growth History and Expansion History

Abstract

The cosmic expansion history tests the dynamics of the global evolution of the universe and its energy density contents, while the cosmic growth history tests the evolution of the inhomogeneous part of the energy density. Precision comparison of the two histories can distinguish the nature of the physics responsible for the accelerating cosmic expansion: an additional smooth component - dark energy - or a modification of the gravitational field equations. With the aid of a new fitting formula for linear perturbation growth accurate to 0.05-0.2%, we separate out the growth dependence on the expansion history and introduce a new growth index parameter γthat quantifies the gravitational modification.

8 pages, 3 figures; minor changes to match version accepted to PRD

References in corpus (5)

• Effect of inhomogeneities on the expansion rate of the Universe
• Looking for an extra dimension with tomographic cosmic shear
• Undulant Universe
• Cosmic microwave background constraints on dark energy dynamics: analysis beyond the power spectrum
• Limits of dark energy measurements from CMB lensing-ISW-galaxy count correlations

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• Uniqueness of Current Cosmic Acceleration
• An extended analysis for a generalized Chaplygin gas model
• Cluster counts III. $\Lambda$CDM extensions and the cluster tension
• A partial inventory of observational anisotropies in single-dish line-intensity mapping
• Observational Constraints on Undulant Cosmologies
• Constraining dark sector perturbations I: cosmic shear and CMB lensing
• The Peculiar Velocity Correlation Function
• Phase Space dynamics of triaxial collapse: Joint density-velocity evolution
• Clustering tomography: measuring cosmological distances through angular clustering in thin redshift shells
• Galaxy Clustering in 3D and Modified Gravity Theories
• Modifying Gravity at Low Redshift
• Hybrid modeling of redshift space distortions
• Extracting the Signal of Cosmic String Wakes from 21-cm Observations
• Vector modes in $\Lambda$CDM: the gravitomagnetic potential in dark matter haloes from relativistic $N$-body simulations
• Geometric and dynamic distortions in anisotropic galaxy clustering
• Probing gravity with redshift-space distortions: effects of tracer bias and sample selection
• Inferring dark energy properties from the scale factor parametrisation
• Constraining dark sector perturbations II: ISW and CMB lensing tomography
• Cluster counts. II. Tensions, massive neutrinos, and modified gravity
• Observational constraints on finite scale factor singularities
• Model-Independent Predictions for Smooth Cosmic Acceleration Scenarios
• ISiTGR: Testing deviations from GR at cosmological scales including dynamical dark energy, massive neutrinos, functional or binned parametrizations, and spatial curvature
• The generalized evolution of linear bias: a tool to test gravity
• Constraining the emergent dark energy models with observational data at intermediate redshift
• Complete density perturbations in the Jordan-Fierz-Brans-Dicke theory
• Calibrating the BAO scale using the CMB: Lifting the degeneracy between geometric and dynamic distortions using the sound horizon from the CMB
• Linear matter density perturbations in the ${\Lambda }_{\mathrm{s}}$CDM model: Examining growth dynamics and addressing the $S_8$ tension
• Forecasting cosmological parameter constraints from near-future space-based galaxy surveys
• An analytic calculation of the growth index for $f(R)$ dark energy model
• Uneven flows: On cosmic bulk flows, local observers, and gravity
• Statistical Determination of Bulk Flow Motions
• Neural network reconstruction of density and velocity fields from the 2MASS Redshift Survey
• Joint analyses of 2D CMB lensing and 3D galaxy clustering in the spherical Fourier-Bessel basis
• Cosmological Tests of Gravity: A Future Perspective
• Combining spectroscopic and photometric surveys using angular cross-correlations III: Galaxy bias and stochastisity
• Testing Standard Cosmology with Large Scale Structure
• Decaying dark matter mimicking time-varying dark energy
• Reconstructing the growth index $\gamma$ with Gaussian Processes
• The WARPS Survey. VIII. Evolution of the Galaxy Cluster X-ray Luminosity Function
• No Run Gravity
• Looking for a twist: probing the cosmological gravitomagnetic effect via weak lensing-kSZ cross correlations
• Configuration entropy in the $\Lambda$CDM and the dynamical dark energy models: Can we distinguish one from the other?
• Non-linear mode coupling and the growth of perturbations in LCDM
• Cosmological tests of gravity with latest observations
• The observational constraints on the flat $\varphi$CDM models
• High resolution tomography for galaxy spectroscopic surveys with angular redshift fluctuations
• Mass Screening in Modified Gravity
• Dark-energy dependent test of general relativity at cosmological scales
• Data-driven and Almost Model-independent Reconstruction of Modified Gravity
• Late Time Modification of Structure Growth and the S8 Tension
• ${\Lambda }_{\mathrm{s}}$CDM cosmology from a type-II minimally modified gravity
• Testing the Homogeneity of Type Ia Supernovae in the Near-Infrared for Accurate Distance Estimations
• One-point probability distribution function from spherical collapse: Early Dark Energy (EDE) vs. $\Lambda$CDM
• Primordial non-Gaussianity with Angular correlation function: Integral constraint and validation for DES
• Biasing relation, environmental dependencies and estimation of the growth rate from star forming galaxies
• Parametrizing growth in dark energy and modified gravity models
• Bouncing cosmological models in a functional form of F(R) gravity
• Improved parametrization of the growth index for dark energy and DGP models
• Bound Dark Energy: towards understanding the nature of the Dark Energy
• A Model for Cosmic Self-Acceleration
• Cosmological Acceleration: Dark Energy or Modified Gravity?
• Euclid preparation. LII. Forecast impact of super-sample covariance on 3x2pt analysis with Euclid
• Constraints on scalar-tensor theories of gravity from observations
• Relativistic effects in the large-scale structure with effective dark energy fluids
• The Distinguishability of Interacting Dark Energy from Modified Gravity
• Simultaneous constraints on bias, normalization and growth index through power spectrum measurements
• Hybrid Chaplygin gas and phantom divide crossing
• Can we distinguish early dark energy from a cosmological constant?
• Ellipsoidal universe in the brane world
• Testing modified gravity scenarios with direct peculiar velocities
• Growth and Geometry Split in Light of the DES-Y3 Survey
• Scalar field descriptions of two dark energy models
• Constraining modified gravity scenarios with the 6dFGS and SDSS galaxy peculiar velocity datasets
• The exact analytical solution of the linear structure growth rate in LCDM cosmology and its cosmological applications
• Constraining the growth rate of structure with phase correlations
• Precise peculiar velocities from gravitational waves accompanied by electromagnetic signals and cosmological applications
• Singling out modified gravity parameters and datasets reveals a dichotomy between Planck and lensing
• Fast Calculation of Nonlinear Redshift-space Galaxy Power Spectrum Including Selection Bias
• Power Spectrum Precision for Redshift Space Distortions
• Non-linear density-velocity divergence relation from phase space dynamics
• Improving Constraints on Fundamental Physics Parameters with the Clustering of Sunyaev-Zeldovich Selected Galaxy Clusters
• Expansion and Growth of Structure Observables in a Macroscopic Gravity Averaged Universe
• Unveiling the Universe with Emerging Cosmological Probes
• Constraining dark energy using observational growth rate data
• By Dawn's Early Light: CMB Polarization Impact on Cosmological Constraints
• Galactos: Computing the Anisotropic 3-Point Correlation Function for 2 Billion Galaxies
• Massive Gravity wrapped in the Cosmic Web
• Gravitational Slip parameter and Gravitational Waves in Einstein-Cartan theory
• Halo/Galaxy Bispectrum with Equilateral-type Primordial Trispectrum
• Cosmic Growth Signatures of Modified Gravitational Strength
• A study of holographic dark energy models using configuration entropy
• Trace Anomaly Inflation in Brane Induced Gravity
• Deep learning insights into non-universality in the halo mass function
• An Analytic Formula for the Supercluster Mass Function
• Structure formation and CMBR anisotropy spectrum in the inflessence model
• Teleparallel dark energy in a nonflat universe
• Constraining Dynamical Dark Energy Models through the Abundance of High-Redshift Supermassive Black Holes
• Measuring the Hubble constant through the galaxy pairwise peculiar velocity
• Growth rate of matter perturbations as a probe of large-scale magnetism
• Second order invariants and holography
• The Cosmic Mach Number: Comparison from Observations, Numerical Simulations and Nonlinear Predictions
• Tomographic cross correlations between galaxy surveys and the CMB gravitational lensing potential. Effect of the redshift bin mismatch
• The first direct measurement of gravitational potential decay rate at cosmological scales and improved dark energy constraint
• Non-linear density-velocity dynamics in $f(R)$ gravity from spherical collapse
• Expressing the equation of state parameter in terms of the three dimensional cosmic shear
• Fitting functions on the cheap: the relative nonlinear matter power spectrum
• Measuring the growth of structure by matching dark matter haloes to galaxies with VIPERS and SDSS
• Detection of the Intrinsic Spin Alignments in Isolated Spiral Pairs
• Seeing Darkness: the New Cosmology
• Scaling of the 1-halo terms with bias
• Modified gravity with disappearing cosmological constant
• What Drives Our Accelerating Universe?
• Re-examination of Large Scale Structure and Cosmic Flows
• Dynamical dark energy models with singularities in the view of the forthcoming results of the growth observations
• Measuring neutrino mass and asymmetry with matter pairwise velocities
• A method to extract the redshift distortions beta parameter in configuration space from minimal cosmological assumptions
• New measures to test modified gravity cosmologies
• Cosmology with voids from the Nancy Grace Roman Space Telescope
• Configurational Entropy in Chaplygin Gas Models
• Galaxy and Mass Assembly (GAMA): Probing galaxy-group correlations in redshift space with the halo streaming model
• Testing for gravitational preferred directions with galaxy and lensing surveys
• Effect of redshift bin mismatch on cross correlation between DESI Legacy Imaging Survey and Planck CMB lensing potential
• Cross-correlating radial peculiar velocities and CMB lensing convergence
• Growth of matter perturbations for realistic $F(R)$ models
• Post-Newtonian Gravity in Cosmology
• Late Time Phenomena in $f(T,\mathcal{T})$ Gravity Framework: Role of $H_0$ Priors
• Can we constrain the dark energy equation of state parameters using configuration entropy?
• Euclid preparation. Improving cosmological constraints using a new multi-tracer method with the spectroscopic and photometric samples
• The Cosmic Mach Number as an Environment Measure for the Underlying Dark Matter Density Field
• Probing the time variation of the effective Newton's constant with optimal redshift weights
• Catalog-level blinding on the bispectrum for DESI-like galaxy surveys
• Probing the independence within the dark sector in the fluid approximation
• The RSD Sorting Hat: Unmixing Radial Scales in Projection
• The Direction of Gravity
• Observational constraints and differential diagnosis for cosmic evolutionary models
• Redshift Sensitivity of the Kaiser Effect
• Towards a Composite Framework for Simultaneous Exploration of New Physics in Background and Perturbed Universe
• A density-responsive scalar-field framework for singularity regularization and dynamical dark energy
• Influence of the Local Void on measurements of the clustering dipole
• A new consistency test for $\Lambda$CDM cosmology using galaxy surveys
• Perspectives for studying the dark energy at z>2 with galaxy surveys
• Evolution of axis ratios from phase space dynamics of triaxial collapse
• Prospects for constraining quasar ages with fiber spectrographs: quasar-induced Ly$\alpha$ emission from the intergalactic medium
• Constraining the expansion history of the universe from the red shift evolution of cosmic shear
• Spatial Dependence of the Growth Factor in Scalar-Tensor Cosmology
• Cosmology with Gravitational Lensing
• Motion of the Local Group as a cosmological probe
• Modeling and measuring the anisotropic halo 3-point correlation function: a coordinated study
• Can dark energy explain a high growth index?
• Improving cosmological constraints via galaxy intrinsic alignment in full-shape analysis
• $\Lambda$CDM without cosmological constant
• Fullshape power spectrum for the Symmetron modified gravity model
• Angular correlation functions of bright Lyman-break galaxies at $3\lesssim \mathbf{z}\lesssim 5$
• Probing the Type 3 interacting dark-energy model using matter pairwise velocity
• Theory Challenges of the Accelerating Universe
• Dark Energy After DESI DR2: Observational Status, Reconstructions, and Physical Models
• Coupling dark-baryonic matter density profile for vacuum decay scenarios
• Biased Cosmology: Pivots, Parameters, and Figures of Merit
• Joint Curvature and Growth Rate measurements with Supernova Peculiar Velocities and the CMB
• The anisotropic redshift space galaxy correlation function: detection on the BAO Ring
• Structural Limitations on Constraining the Time Evolution of Dark Energy
• Improved Methods for Estimating Peculiar Velocity Correlation Functions Using Volume Weighting
• Probing gravity with non-linear clustering in redshift space
• Inductive rectilinear frame dragging and local coupling to the gravitational field of the universe
• The frame-dragging vector potential on galaxy scales from Dark-Matter-only Newtonian $N$-body simulations
• Diagnostics and future evolution analysis of the two parametric models
• $\Lambda$CDM-like models with future singularities
• Integrated Sachs-Wolfe maps from the Gower Street $w$CDM simulations
• Constraining the growth rate on linear scales by combining SKAO and DESI surveys
• Bayesian evidence and model selection approach for time-dependent dark energy
• Implications of a high growth index on the variation of $G$
• Determining the expansion history of the universe with the three dimensional cosmic shear