Cosmological Probes of Structure Growth and Tests of Gravity

Abstract

The current standard cosmological model is constructed within the framework of general relativity with a cosmological constant $\Lambda$, which is often associated with dark energy, and phenomenologically explains the accelerated cosmic expansion. Understanding the nature of dark energy is one of the most appealing questions in achieving a self-consistent physical model at cosmological scales. Modification of general relativity could potentially provide a more natural and physical solution to the accelerated expansion. The growth of the cosmic structure is sensitive in constraining gravity models. In this paper, we aim to provide a concise introductory review of modified gravity models from an observational point of view. We will discuss various mainstream cosmological observables, and their potential advantages and limitations as probes of gravity models.

arXiv comment72 pages, 19 figures, Invited review for Universe, Special Issue "Cosmological Constant"

References in corpus (500)

• Observational Evidence from Supernovae for an Accelerating Universe and a Cosmological Constant
• Measurements of Omega and Lambda from 42 High-Redshift Supernovae
• Observation of Gravitational Waves from a Binary Black Hole Merger
• Planck 2015 results. XIII. Cosmological parameters
• GW170817: Observation of Gravitational Waves from a Binary Neutron Star Inspiral
• The Structure of Cold Dark Matter Halos
• The Wide-field Infrared Survey Explorer (WISE): Mission Description and Initial On-orbit Performance
• The cosmological simulation code GADGET-2
• f(R) Theories Of Gravity
• f(R) theories
• 4D Gravity on a Brane in 5D Minkowski Space
• The clustering of galaxies in the completed SDSS-III Baryon Oscillation Spectroscopic Survey: cosmological analysis of the DR12 galaxy sample
• Populating a cluster of galaxies - I. Results at z=0
• LOFAR: The LOw-Frequency ARray
• E pur si muove: Galiliean-invariant cosmological hydrodynamical simulations on a moving mesh
• Nine-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Final Maps and Results
• Is Cosmic Speed-Up Due to New Gravitational Physics?
• SDSS-III: Massive Spectroscopic Surveys of the Distant Universe, the Milky Way Galaxy, and Extra-Solar Planetary Systems
• Cosmological Hydrodynamics with Adaptive Mesh Refinement: a new high resolution code called RAMSES
• The Baryon Oscillation Spectroscopic Survey of SDSS-III
• Halo Models of Large Scale Structure
• Simulating Galaxy Formation with the IllustrisTNG Model
• A Dynamical Solution to the Problem of a Small Cosmological Constant and Late-time Cosmic Acceleration
• Large Magellanic Cloud Cepheid Standards Provide a 1% Foundation for the Determination of the Hubble Constant and Stronger Evidence for Physics Beyond LambdaCDM
• Dark Energy and the Accelerating Universe
• Large-Scale Structure of the Universe and Cosmological Perturbation Theory
• The galileon as a local modification of gravity
• Essentials of k-essence
• Models of f(R) Cosmic Acceleration that Evade Solar-System Tests
• Accurate photometric redshifts for the CFHT Legacy Survey calibrated using the VIMOS VLT Deep Survey
• Chameleon Fields: Awaiting Surprises for Tests of Gravity in Space
• Chameleon Cosmology
• Sloan Digital Sky Survey IV: Mapping the Milky Way, Nearby Galaxies, and the Distant Universe
• The Simons Observatory: Science goals and forecasts
• Cosmology at Low Frequencies: The 21 cm Transition and the High-Redshift Universe
• The Rockstar Phase-Space Temporal Halo Finder and the Velocity Offsets of Cluster Cores
• The Completed SDSS-IV extended Baryon Oscillation Spectroscopic Survey: Cosmological Implications from two Decades of Spectroscopic Surveys at the Apache Point observatory
• Chandra sample of nearby relaxed galaxy clusters: mass, gas fraction, and mass-temperature relation
• Observational Probes of Cosmic Acceleration
• Curvature Quintessence
• Simulating galaxy formation with black hole driven thermal and kinetic feedback
• The DESI Experiment Part I: Science,Targeting, and Survey Design
• Generalized G-inflation: Inflation with the most general second-order field equations
• Dark Energy Survey Year 3 Results: Cosmological Constraints from Galaxy Clustering and Weak Lensing
• Cosmological Parameters from Observations of Galaxy Clusters
• The Effective Field Theory of Inflation
• From k-essence to generalised Galileons
• Weak Gravitational Lensing of the CMB
• The Hyper Suprime-Cam SSP Survey: Overview and Survey Design
• Massive neutrinos and cosmology
• The Dark Energy Survey: more than dark energy - an overview
• Tests of the Gravitational Inverse-Square Law below the Dark-Energy Length Scale
• 21-cm cosmology
• The Halo Occupation Distribution: Towards an Empirical Determination of the Relation Between Galaxies and Mass
• Monodromy in the CMB: Gravity Waves and String Inflation
• Dancing in the dark: galactic properties trace spin swings along the cosmic web
• Cosmology on a Brane in Minkowski Bulk
• The GMRT 150 MHz All-sky Radio Survey: First Alternative Data Release TGSS ADR1
• The physics driving the cosmic star formation history
• The SDSS-IV extended Baryon Oscillation Spectroscopic Survey: Overview and Early Data
• The Baryonic Tully-Fisher Relation
• Tests of the Gravitational Inverse-Square Law
• Large-Scale Galaxy Bias
• Gravity Waves and Linear Inflation from Axion Monodromy
• Modeling Luminosity-Dependent Galaxy Clustering Through Cosmic Time
• KiDS-1000 Cosmology: Cosmic shear constraints and comparison between two point statistics
• 21cmFAST: A Fast, Semi-Numerical Simulation of the High-Redshift 21-cm Signal
• Cosmic Growth History and Expansion History
• KiDS-1000 Cosmology: Multi-probe weak gravitational lensing and spectroscopic galaxy clustering constraints
• Braneworld models of dark energy
• Symmetron Fields: Screening Long-Range Forces Through Local Symmetry Restoration
• Extragalactic Science, Cosmology and Galactic Archaeology with the Subaru Prime Focus Spectrograph (PFS)
• 1/R gravity and Scalar-Tensor Gravity
• The Hubble Hunter's Guide
• Strong Interactions and Stability in the DGP Model
• Dark Energy Survey Year 1 Results: Cosmological Constraints from Cosmic Shear
• Cosmological Non-Linearities as an Effective Fluid
• The Effective Field Theory of Cosmological Large Scale Structures
• Mass Reconstruction with CMB Polarization
• The 2dF Galaxy Redshift Survey: The bias of galaxies and the density of the Universe
• The Atacama Cosmology Telescope: DR4 Maps and Cosmological Parameters
• Effective Field Theory for Inflation
• The 6dF Galaxy Survey: Samples, Observational Techniques and the First Data Release
• Scientific Objectives of Einstein Telescope
• Redshift-Space Distortions, Pairwise Velocities and Nonlinearities
• Renormalized Cosmological Perturbation Theory
• Cosmology from cosmic shear power spectra with Subaru Hyper Suprime-Cam first-year data
• Starting the Universe: Stable Violation of the Null Energy Condition and Non-standard Cosmologies
• The WiggleZ Dark Energy Survey: Survey Design and First Data Release
• The 6dF Galaxy Survey: z \approx 0 measurement of the growth rate and sigma_8
• A hierarchy of voids: Much ado about nothing
• The BAHAMAS project: Calibrated hydrodynamical simulations for large-scale structure cosmology
• The WiggleZ Dark Energy Survey: the growth rate of cosmic structure since redshift z=0.9
• Resumming Cosmological Perturbations via the Lagrangian Picture: One-loop Results in Real Space and in Redshift Space
• The LOFAR Two-metre Sky Survey -- V. Second data release
• CMB Lensing Reconstruction on the Full Sky
• The $H_0$ Olympics: A fair ranking of proposed models
• Nonlinear Evolution of Baryon Acoustic Oscillations
• The effects of galaxy formation on the matter power spectrum: A challenge for precision cosmology
• Dark Energy vs. Modified Gravity
• Testing General Relativity in Cosmology
• Dark Energy Survey Year 3 Results: Cosmology from Cosmic Shear and Robustness to Data Calibration
• The COMBO-17 Survey: Evolution of the Galaxy Luminosity Function from 25,000 Galaxies with 0.2<z<1.2
• Gravitational Lensing
• Rotation-Dependent Catastrophic Disruption of Gravitational Aggregates
• Dependence of the outer density profiles of halos on their mass accretion rate
• EMU: Evolutionary Map of the Universe
• Non-minimal dark sector physics and cosmological tensions
• The Kilo-Degree Survey
• Baryon Acoustic Oscillations in 2D: Modeling Redshift-space Power Spectrum from Perturbation Theory
• An accurate halo model for fitting non-linear cosmological power spectra and baryonic feedback models
• A Parameterized Post-Friedmann Framework for Modified Gravity
• Maximal freedom at minimum cost: linear large-scale structure in general modifications of gravity
• The structural and scaling properties of nearby galaxy clusters - II. The M-T relation
• A new measure for cosmic shear
• Dark Energy Survey Year 3 Results: Cosmology from Cosmic Shear and Robustness to Modeling Uncertainty
• Planck intermediate results. XLVI. Reduction of large-scale systematic effects in HFI polarization maps and estimation of the reionization optical depth
• Weak lensing for precision cosmology
• Dark Energy Survey Year 1 Results: Constraints on Extended Cosmological Models from Galaxy Clustering and Weak Lensing
• Baryon Acoustic Oscillation Intensity Mapping as a Test of Dark Energy
• ZOBOV: a parameter-free void-finding algorithm
• Cluster Cosmology Constraints from the 2500 deg${}^2$ SPT-SZ Survey: Inclusion of Weak Gravitational Lensing Data from Magellan and the Hubble Space Telescope
• Quintessence without scalar fields
• Evading Equivalence Principle Violations, Cosmological and other Experimental Constraints in Scalar Field Theories with a Strong Coupling to Matter
• Reconstruction of lensing from the cosmic microwave background polarization
• KiDS+VIKING-450: Cosmic shear tomography with optical+infrared data
• Breaking a Dark Degeneracy with Gravitational Waves
• The VIMOS Public Extragalactic Redshift Survey (VIPERS). An unprecedented view of galaxies and large-scale structure at 0.5<z<1.2
• Solving Large Scale Structure in Ten Easy Steps with COLA
• The Completed SDSS-IV extended Baryon Oscillation Spectroscopic Survey: BAO and RSD measurements from anisotropic clustering analysis of the Quasar Sample in configuration space between redshift 0.8 and 2.2
• Interacting dark energy in the early 2020s: a promising solution to the $H_0$ and cosmic shear tensions
• A semi-empirical simulation of the extragalactic radio continuum sky for next generation radio telescopes
• Detection of (dark) matter concentrations via weak gravitational lensing
• Measurement of 21 cm brightness fluctuations at z ~ 0.8 in cross-correlation
• The Completed SDSS-IV extended Baryon Oscillation Spectroscopic Survey: measurement of the BAO and growth rate of structure of the luminous red galaxy sample from the anisotropic correlation function between redshifts 0.6 and 1
• Late-time cosmology with 21cm intensity mapping experiments
• Correlation of CMB with large-scale structure: I. ISW Tomography and Cosmological Implications
• Confirmation of general relativity on large scales from weak lensing and galaxy velocities
• SPT-3G: A Next-Generation Cosmic Microwave Background Polarization Experiment on the South Pole Telescope
• The fourth data release of the Kilo-Degree Survey: ugri imaging and nine-band optical-IR photometry over 1000 square degrees
• Dark Energy or Modified Gravity? An Effective Field Theory Approach
• The VIMOS Public Extragalactic Redshift Survey (VIPERS). Galaxy clustering and redshift-space distortions at z=0.8 in the first data release
• f(R) Gravity and Chameleon Theories
• The Completed SDSS-IV extended Baryon Oscillation Spectroscopic Survey: measurement of the BAO and growth rate of structure of the luminous red galaxy sample from the anisotropic power spectrum between redshifts 0.6 and 1.0
• The clustering of galaxies in the SDSS-III Baryon Oscillation Spectroscopic Survey: a large sample of mock galaxy catalogues
• 4MOST: Project overview and information for the First Call for Proposals
• Cosmology with Phase 1 of the Square Kilometre Array; Red Book 2018: Technical specifications and performance forecasts
• GLEAM: The GaLactic and Extragalactic All-sky MWA survey
• Looking for $\Lambda$ with the Rees-Sciama Effect
• Combined analysis of the integrated Sachs-Wolfe effect and cosmological implications
• The Rapid ASKAP Continuum Survey I: Design and First Results
• Dark Energy Survey Year 1 Results: Cosmological Constraints from Cluster Abundances and Weak Lensing
• A Cosmic Watershed: the WVF Void Detection Technique
• Cosmological constraints from cosmic shear two-point correlation functions with HSC survey first-year data
• 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 $z=0.15$
• The Completed SDSS-IV extended Baryon Oscillation Spectroscopic Survey: BAO and RSD measurements from the anisotropic power spectrum of the Quasar sample between redshift 0.8 and 2.2
• The galaxy cluster mass scale and its impact on cosmological constraints from the cluster population
• Evidence for massive neutrinos from CMB and lensing observations
• k-Mouflage gravity
• Challenges to Self-Acceleration in Modified Gravity from Gravitational Waves and Large-Scale Structure
• Searching for modified growth patterns with tomographic surveys
• Symmetron Cosmology
• Nonlinear perturbation theory with halo bias and redshift-space distortions via the Lagrangian picture
• Non-linear Evolution of f(R) Cosmologies III: Halo Statistics
• ECOSMOG: An Efficient Code for Simulating Modified Gravity
• Solar System tests DO rule out 1/R gravity
• HI intensity mapping : a single dish approach
• Effective Field Theory of Cosmic Acceleration: an implementation in CAMB
• Cluster Constraints on f(R) Gravity
• The power spectrum and bispectrum of SDSS DR11 BOSS galaxies I: bias and gravity
• Equivalence Principle Implications of Modified Gravity Models
• The third data release of the Kilo-Degree Survey and associated data products
• The Atacama Cosmology Telescope: Two-Season ACTPol Spectra and Parameters
• FastPM: a new scheme for fast simulations of dark matter and halos
• Fast Estimators for Redshift-Space Clustering
• A new method to quantify the effects of baryons on the matter power spectrum
• Dark Energy Survey Year 3 Results: Photometric Data Set for Cosmology
• The Lagrangian-space Effective Field Theory of Large Scale Structures
• Ingredients for 21cm intensity mapping
• Scaling laws in X-ray Galaxy Clusters at redshift between 0.4 and 1.3
• Effective Field Theory of Dark Energy: a Review
• Measurements of the Temperature and E-Mode Polarization of the CMB from 500 Square Degrees of SPTpol Data
• The Completed SDSS-IV extended Baryon Oscillation Spectroscopic Survey: Large-scale Structure Catalogs for Cosmological Analysis
• Intensity Mapping with Carbon Monoxide Emission Lines and the Redshifted 21 cm Line
• Photometric redshifts in the SWIRE Survey
• Quantifying baryon effects on the matter power spectrum and the weak lensing shear correlation
• The Completed SDSS-IV extended Baryon Oscillation Spectroscopic Survey: measurement of the BAO and growth rate of structure of the emission line galaxy sample from the anisotropic power spectrum between redshift 0.6 and 1.1
• CFHTLenS: Testing the Laws of Gravity with Tomographic Weak Lensing and Redshift Space Distortions
• Constraints on Cosmology and Gravity from the Dynamics of Voids
• Testing Gravity using Cosmic Voids
• Modified Gravity-GADGET: A new code for cosmological hydrodynamical simulations of modified gravity models
• Dark Energy Survey Year 3 Results: Weak Lensing Shape Catalogue
• Galileon Gravity in Light of ISW, CMB, BAO and $H_0$ data
• Lack of clustering in low-redshift 21-cm intensity maps cross-correlated with 2dF galaxy densities
• Cosmology from large-scale structure: Constraining $\Lambda$CDM with BOSS
• Dark Energy Survey Year 3 Results: Redshift Calibration of the Weak Lensing Source Galaxies
• Multi-Point Propagators in Cosmological Gravitational Instability
• The Bispectrum of IRAS Galaxies
• Effective Field Theory of Cosmic Acceleration: constraining dark energy with CMB data
• hi_class: Horndeski in the Cosmic Linear Anisotropy Solving System
• Large-scale dark matter simulations
• Testing General Relativity with 21 cm intensity mapping
• KiDS-1000 catalogue: Redshift distributions and their calibration
• Voids in Modified Gravity: Excursion Set Predictions
• Rejuvenating the matter power spectrum: restoring information with a logarithmic density mapping
• Line-Intensity Mapping: 2017 Status Report
• KiDS-1000 catalogue: Weak gravitational lensing shear measurements
• CLASS: The Cosmology Large Angular Scale Surveyor
• Cosmological Constraints on f(R) Acceleration Models
• Is there proof that backreaction of inhomogeneities is irrelevant in cosmology?
• The X-Ray Luminosity--Mass Relation for Local Clusters of Galaxies
• Baryonic Acoustic Oscillations in 21cm Emission: A Probe of Dark Energy out to High Redshifts
• Limits on the number of spacetime dimensions from GW170817
• Challenges to the DGP Model from Horizon-Scale Growth and Geometry
• The Completed SDSS-IV extended Baryon Oscillation Spectroscopic Survey: Growth rate of structure measurement from anisotropic clustering analysis in configuration space between redshift 0.6 and 1.1 for the Emission Line Galaxy sample
• Photometric Redshifts of Galaxies in COSMOS
• Probing modifications of General Relativity using current cosmological observations
• Constraints on f(R) gravity from probing the large-scale structure
• Modified Gravity N-body Code Comparison Project
• Density profile of dark matter haloes and galaxies in the Horizon-AGN simulation: the impact of AGN feedback
• A new approach to observational cosmology using the scattering transform
• Non-linear Evolution of Matter Power Spectrum in Modified Theory of Gravity
• Ultra large-scale cosmology in next-generation experiments with single tracers
• Spatial and Dynamical Properties of Voids in a LCDM Universe
• The Tiered Radio Extragalactic Continuum Simulation (T-RECS)
• The Aemulus Project III: Emulation of the Galaxy Correlation Function
• ISIS: a new N-body cosmological code with scalar fields based on RAMSES. Code presentation and application to the shapes of clusters
• Connecting CO Intensity Mapping to Molecular Gas and Star Formation in the Epoch of Galaxy Assembly
• Constraints on Galaxy Bias, Matter Density, and Primordial Non--Gausianity from the PSCz Galaxy Redshift Survey
• Redshift space distortions in f(R) gravity
• Parameter constraints from cross-correlation of CMB lensing with galaxy clustering
• Probing the Cosmological Principle in the counts of radio galaxies at different frequencies
• Probing cosmology and gravity with redshift-space distortions around voids
• Cosmological Simulations of Normal-Branch Braneworld Gravity
• COSEBIs: Extracting the full E-/B-mode information from cosmic shear correlation functions
• Brans-Dicke gravity with a cosmological constant smoothes out $\Lambda$CDM tensions
• The Santiago-Harvard-Edinburgh-Durham void comparison I: SHEDding light on chameleon gravity tests
• On the road to percent accuracy: nonlinear reaction of the matter power spectrum to dark energy and modified gravity
• Density split statistics: Cosmological constraints from counts and lensing in cells in DES Y1 and SDSS data
• Probing Parity-Violation with the Four-Point Correlation Function of BOSS Galaxies
• Constraints on dark matter scenarios from measurements of the galaxy luminosity function at high redshifts
• Cosmological constraints from unWISE and Planck CMB lensing tomography
• Towards an Optimal Estimation of Cosmological Parameters with the Wavelet Scattering Transform
• An Improved Measurement of the Secondary Cosmic Microwave Background Anisotropies from the SPT-SZ + SPTpol Surveys
• Fisher for complements: Extracting cosmology and neutrino mass from the counts-in-cells PDF
• Cosmology with Void-Galaxy Correlations
• Cluster Density Profiles as a Test of Modified Gravity
• Weak lensing by voids in modified lensing potentials
• What can Cosmology tell us about Gravity? Constraining Horndeski with Sigma and Mu
• Testing chameleon gravity with the Coma cluster
• Cosmological Constraints on DGP Braneworld Gravity with Brane Tension
• The Atacama Cosmology Telescope: A CMB lensing mass map over 2100 square degrees of sky and its cross-correlation with BOSS-CMASS galaxies
• Nearest Neighbor distributions: new statistical measures for cosmological clustering
• Deconstructing the kinetic SZ Power Spectrum
• Exploring Vainshtein mechanism on adaptively refined meshes
• Photometric Redshifts for Next-Generation Surveys
• Redshift-space distortions around voids
• Computing the Three-Point Correlation Function of Galaxies in $\mathcal{O}(N^2)$ Time
• Systematic simulations of modified gravity: symmetron and dilaton models
• Non-linear interactions in a cosmological background in the DGP braneworld
• HI intensity mapping with MeerKAT: power spectrum detection in cross-correlation with WiggleZ galaxies
• Cosmological constraints from the tomographic cross-correlation of DESI Luminous Red Galaxies and Planck CMB lensing
• Cosmological Tests of General Relativity with Future Tomographic Surveys
• HI constraints from the cross-correlation of eBOSS galaxies and Green Bank Telescope intensity maps
• Weak lensing of the CMB
• HI as a Probe of the Large Scale Structure in the Post-Reionization Universe
• First results from the 2dF galaxy redshift survey
• COPSS II: The Molecular Gas Content of Ten Million Cubic Megaparsecs at $z\sim 3$
• The VIMOS Public Extragalactic Redshift Survey (VIPERS). Gravity test from the combination of redshift-space distortions and galaxy-galaxy lensing at $0.5<z<1.2$
• Cluster Abundance in f(R) Gravity Models
• The LOFAR LBA Sky Survey I. survey description and preliminary data release
• Intensity Mapping of Lyman-alpha Emission During the Epoch of Reionization
• Re-Ionization and its Imprint on the Cosmic Microwave Background
• Density split statistics: joint model of counts and lensing in cells
• New Interpretable Statistics for Large Scale Structure Analysis and Generation
• BOSS Correlation Function Analysis from the Effective Field Theory of Large-Scale Structure
• COLA with scale-dependent growth: applications to screened modified gravity models
• A marked correlation function for constraining modified gravity models
• On the EFT of Large Scale Structures in Redshift Space
• The Effect of Large-Scale Structure on the SDSS Galaxy Three-Point Correlation Function
• The Novel Probes Project -- Tests of Gravity on Astrophysical Scales
• LRP 2020 Whitepaper: The Canadian Hydrogen Observatory and Radio-transient Detector (CHORD)
• Testing Screened Modified Gravity
• Detection of Cosmological 21 cm Emission with the Canadian Hydrogen Intensity Mapping Experiment
• Reconstructing Gravity on Cosmological Scales
• A complete FFT-based decomposition formalism for the redshift-space bispectrum
• Intensity Mapping across Cosmic Times with the Lyman-Alpha Line
• Wide-Field InfraRed Survey Telescope-Astrophysics Focused Telescope Assets WFIRST-AFTA Final Report
• Measurement of Parity-Odd Modes in the Large-Scale 4-Point Correlation Function of SDSS BOSS DR12 CMASS and LOWZ Galaxies
• HI 21-centimetre emission from an ensemble of galaxies at an average redshift of one
• Nonlinear Kinetic Sunyaev-Zeldovich Effect
• Joint constraints on cosmology and the impact of baryon feedback: combining KiDS-1000 lensing with the thermal Sunyaev-Zeldovich effect from Planck and ACT
• New constraints on parametrised modified gravity from correlations of the CMB with large scale structure
• Galaxy clustering in the DESI Legacy Survey and its imprint on the CMB
• Testing Gravity Using Galaxy Clusters: New Constraints on Beyond Horndeski Theories
• Precision cosmology with voids in the final BOSS data
• Cosmological tests of General Relativity: a principal component analysis
• Arguments against using $h^{-1}\mathrm{Mpc}$ units in observational cosmology
• Cosmological Hints of Modified Gravity ?
• RCSLenS: Testing gravitational physics through the cross-correlation of weak lensing and large-scale structure
• HI intensity mapping with MeerKAT: Calibration pipeline for multi-dish autocorrelation observations
• Calculation of the Ostriker-Vishniac Effect in Cold Dark Matter Models
• A User's Guide to Extracting Cosmological Information from Line-Intensity Maps
• The BOSS bispectrum analysis at one loop from the Effective Field Theory of Large-Scale Structure
• Testing the theory of gravity with DESI: estimators, predictions and simulation requirements
• Dark matter statistics for large galaxy catalogs: power spectra and covariance matrices
• Redshift Space Distortions in the Effective Field Theory of Large Scale Structures
• The completed SDSS-IV extended Baryon Oscillation Spectroscopic Survey: geometry and growth from the anisotropic void-galaxy correlation function in the luminous red galaxy sample
• The power spectrum and bispectrum of SDSS DR11 BOSS galaxies II: cosmological interpretation
• On the road to percent accuracy IV: ReACT -- computing the non-linear power spectrum beyond $\Lambda$CDM
• Three-point Correlation Functions of SDSS Galaxies in Redshift Space: Morphology, Color, and Luminosity Dependence
• A Perturbative Approach to the Redshift Space Power Spectrum: Beyond the Standard Model
• K-mouflage Cosmology: the Background Evolution
• Cross-correlating Planck CMB lensing with SDSS: Lensing-lensing and galaxy-lensing cross-correlations
• SKAO HI Intensity Mapping: Blind Foreground Subtraction Challenge
• Three-Point Correlation Functions of SDSS Galaxies: Luminosity and Color Dependence in Redshift and Projected Space
• Carbon Monoxide Intensity Mapping at Moderate Redshifts
• The Santiago-Harvard-Edinburgh-Durham void comparison II: unveiling the Vainshtein screening using weak lensing
• Breaking degeneracies in modified gravity with higher (than 2nd) order weak-lensing statistics
• Back in the saddle: Large-deviation statistics of the cosmic log-density field
• A WISE measurement of the ISW effect
• Quadratic estimators for CMB weak lensing
• Phenomenology of the generalized cubic covariant Galileon model and cosmological bounds
• Systematic simulations of modified gravity: chameleon models
• Validating estimates of the growth rate of structure with modified gravity simulations
• hi_class: Background Evolution, Initial Conditions and Approximation Schemes
• Cosmological structure formation with clustering quintessence
• Three-Point Correlation Functions of SDSS Galaxies: Constraining Galaxy-Mass Bias
• Recovery of 21 cm intensity maps with sparse component separation
• Large-scale clustering of Lyman-alpha emission intensity from SDSS/BOSS
• Cosmological constraints from galaxy-lensing cross correlations using BOSS galaxies with SDSS and CMB lensing
• Search for CII Emission on Cosmological Scales at Redshift Z~2.6
• Measuring the Integrated Sachs-Wolfe Effect
• KiDS+2dFLenS+GAMA: Testing the cosmological model with the $E_{\mathrm{G}}$ statistic
• Concordance cosmology without dark energy
• Modelling Void Abundance in Modified Gravity
• Cosmological Constraints from Galaxy Clusters and Groups in the eROSITA Final Equatorial Depth Survey
• Weak lensing scattering transform: dark energy and neutrino mass sensitivity
• The Bispectrum of f(R) Cosmologies
• Modeling the nonlinear clustering in modified gravity models I: A fitting formula for matter power spectrum of f(R) gravity
• Prospects for Constraining Interacting Dark Energy Models with 21 cm Intensity Mapping Experiments
• Void Lensing as a Test of Gravity
• Finding cosmic voids and filament loops using topological data analysis
• Redshift-space distortions with split densities
• Source-lens clustering effects on the skewness of the lensing convergence
• Cosmological Measurements with Forthcoming Radio Continuum Surveys
• The Atacama Cosmology Telescope: Detection of the Pairwise Kinematic Sunyaev-Zel'dovich Effect with SDSS DR15 Galaxies
• Large-Scale Structure of the Universe as a Cosmic Standard Ruler
• Intensity mapping with SDSS/BOSS Lyman-alpha emission, quasars and their Lyman-alpha forest
• LOFAR and APERTIF surveys of the radio sky: probing shocks and magnetic fields in galaxy clusters
• Impact of Baryonic Processes on Weak Lensing Cosmology: Power Spectrum, Non-Local Statistics, and Parameter Bias
• Warm dark matter signatures on the 21cm power spectrum: Intensity mapping forecasts for SKA
• BICEP3 performance overview and planned Keck Array upgrade
• Efficient simulations of large scale structure in modified gravity cosmologies with comoving Lagrangian acceleration
• HICOSMO - Cosmology with a complete sample of galaxy clusters: II. Cosmological results
• Inflation and Early Dark Energy with a Stage II Hydrogen Intensity Mapping Experiment
• Statistics of dark matter haloes expected from weak lensing surveys
• Cluster abundance in chameleon $f(R)$ gravity I: toward an accurate halo mass function prediction
• Accurate emulator for the redshift-space power spectrum of dark matter halos and its application to galaxy power spectrum
• Hi intensity mapping with MeerKAT: Primary beam effects on foreground cleaning
• The Tianlai Dish Pathfinder Array: design, operation and performance of a prototype transit radio interferometer
• Realistic simulations of galaxy formation in f(R) modified gravity
• K-mouflage Cosmology: Formation of Large-Scale Structures
• The nature of voids: II. Tracing underdensities with biased galaxies
• The missing link: a nonlinear post-Friedmann framework for small and large scales
• Speeding up $N$-body simulations of modified gravity: Chameleon screening models
• Intensity mapping of H-alpha, H-beta, [OII] and [OIII] lines at z<5
• Dark Energy Survey Year 1 Results: tomographic cross-correlations between DES galaxies and CMB lensing from SPT+Planck
• An accurate linear model for redshift space distortions in the void-galaxy correlation function
• Forecast for FAST: from Galaxies Survey to Intensity Mapping
• Voids in Modified Gravity Reloaded: Eulerian Void Assignment
• Modeling CMB Lensing Cross Correlations with {\sc CLEFT}
• Modelling The Redshift-Space Three-Point Correlation Function in SDSS-III
• Splashback in galaxy clusters as a probe of cosmic expansion and gravity
• Cosmological cross-correlations and nearest neighbor distributions
• Homological Percolation and the Euler Characteristic
• Lagrangian perturbation theory for modified gravity
• ENCORE: An $\mathcal{O}(N_{\mathrm{g}}^2)$ Estimator for Galaxy $N$-Point Correlation Functions
• Constraint on the cosmological f(R) model from the multipole power spectrum of the SDSS luminous red galaxy sample and prospects for a future redshift survey
• Regularized cosmological power spectrum and correlation function in modified gravity models
• Joint halo mass function for modified gravity and massive neutrinos I: simulations and cosmological forecasts
• FORGE -- the f(R) gravity cosmic emulator project I: Introduction and matter power spectrum emulator
• Beyond consistency test of gravity with redshift-space distortions at quasi-linear scales
• Large-scale redshift space distortions in modified gravity theories
• Statistics of cosmic density profiles from perturbation theory
• Constraints on the growth of structure around cosmic voids in eBOSS DR14
• The one-loop matter bispectrum as a probe of gravity and dark energy
• Weak lensing by voids in weak lensing maps
• Speeding up N-body simulations of modified gravity: Vainshtein screening models
• Testing gravity using galaxy-galaxy lensing and clustering amplitudes in KiDS-1000, BOSS and 2dFLenS
• Marked clustering statistics in $f(R)$ gravity cosmologies
• Persistent homology of the cosmic web. I: Hierarchical topology in $\Lambda$CDM cosmologies
• Friction in Gravitational Waves: a test for early-time modified gravity
• A Future Test of Gravitation Using Galaxy Cluster Velocities
• Parametrized modified gravity constraints after Planck
• Intensity Mapping Cross-Correlations: Connecting the Largest Scales to Galaxy Evolution
• Probing gravity at large scales through CMB lensing
• Principal reconstructed modes of dark energy and gravity
• Survey strategy optimization for the Atacama Cosmology Telescope
• Projected Constraints on Modified Gravity Cosmologies from 21 cm Intensity Mapping
• Cosmological test of gravity using weak lensing voids
• Primordial gravitational waves in Horndeski gravity
• Effects of baryons on weak lensing peak statistics
• MUSE: Marginal Unbiased Score Expansion and Application to CMB Lensing
• Fast full N-body simulations of generic modified gravity: conformal coupling models
• Galaxy formation in the brane world I: overview and first results
• Intensity mapping with neutral hydrogen and the Hidden Valley simulations
• Does the Galaxy-Halo Connection Vary with Environment?
• Fast and accurate predictions of the nonlinear matter power spectrum for general models of Dark Energy and Modified Gravity
• Gravitational wave propagation in $f(R)$ models: New parametrizations and observational constraints
• A Zeldovich reconstruction method for measuring redshift space distortions using cosmic voids
• Precision Tests of CO and [CII] Power Spectra Models against Simulated Intensity Maps
• Direct detection of the kinetic Sunyaev-Zel'dovich effect in galaxy clusters
• Dark energy imprints on the kinematic Sunyaev-Zel'dovich signal
• The cross-correlation between 21cm intensity mapping maps and the Lyman-alpha forest in the post-reionization era
• No evidence for modifications of gravity from galaxy motions on cosmological scales
• An accurate perturbative approach to redshift space clustering of biased tracers in modified gravity
• Alleviating the tension at low multipole through Axion Monodromy
• Testing Modified Gravity with Cosmic Shear
• Persistent homology in cosmic shear II: A tomographic analysis of DES-Y1
• The imprint of $f(R)$ gravity on weak gravitational lensing II : Information content in cosmic shear statistics
• Baryonic feedback biases on fundamental physics from lensed CMB power spectra
• Constraining cosmology with a new all-sky Compton parameter map from the Planck PR4 data
• New probe of departures from general relativity using Minkowski functionals
• Impact of systematics on cosmological parameters from future Galaxy Clusters surveys
• The impact of modified gravity on the Sunyaev-Zel'dovich effect
• $\mathrm{S}\mathrm{IM}\mathrm{BIG}$: Mock Challenge for a Forward Modeling Approach to Galaxy Clustering
• The BINGO Project II: Instrument Description
• Tomographic Intensity Mapping versus Galaxy Surveys: Observing the Universe in H-alpha emission with new generation instruments
• A general framework to test gravity using galaxy clusters II: A universal model for the halo concentration in $f(R)$ gravity
• Fast full $N$-body simulations of generic modified gravity: derivative coupling models
• Constraining the Expansion History and Early Dark Energy with Line Intensity Mapping
• Developing the 3-Point Correlation Function For the Turbulent Interstellar Medium
• Isotropic N-Point Basis Functions and Their Properties
• Disentangling dark sector models using weak lensing statistics
• Kinetic Sunyaev-Zeldovich effect in modified gravity
• Lensing power spectrum of the Cosmic Microwave Background with deep polarization experiments
• Constraints on neutrino masses from the study of the nearby large-scale structure and galaxy cluster counts
• DEUS Full Observable ΛCDM Universe Simulation: the numerical challenge
• Modeling Nearest Neighbor distributions of biased tracers using Hybrid Effective Field Theory
• Does Quartessence Ease Tensions?
• Minkowski Functionals of SDSS-III BOSS : Hints of Possible Anisotropy in the Density Field?
• KiDS-1000 Cosmology: Constraints from density split statistics
• Cosmological gravity on all scales II: Model independent modified gravity $N$-body simulations
• The BINGO Project VII: Cosmological Forecasts from 21cm Intensity Mapping
• Testing General Relativity on cosmological scales at redshift z ~ 1.5 with quasar and CMB lensing
• Updated constraints from the PLANCK experiment on modified gravity
• The Integrated Sachs Wolfe effect: unWISE and Planck constraints on Dynamical Dark Energy
• Wavelet Moments for Cosmological Parameter Estimation
• Prospects for measuring dark energy with 21 cm intensity mapping experiments: A joint survey strategy
• Parametrising non-linear dark energy perturbations
• Retrieving cosmological information from small-scale CMB foregrounds II. The kinetic Sunyaev Zel'dovich effect
• The impact of baryonic physics and massive neutrinos on weak lensing peak statistics
• Testing gravity at large scales with HI intensity mapping
• Prospects for measuring dark energy with 21 cm intensity mapping experiments
• Galaxy-galaxy weak gravitational lensing in $f(R)$ gravity
• Cosmological constrains on minimally and non-minimally coupled scalar field models
• Cosmological gravity on all scales: simple equations, required conditions, and a framework for modified gravity
• General Modified Gravity With 21cm Intensity Mapping: Simulations and Forecast
• BICEP2 and Keck Array operational overview and status of observations
• Topology of large scale structure as test of modified gravity
• Constraining the interaction between dark sectors with future HI intensity mapping observations
• Baryonic effects on CMB lensing and neutrino mass constraints
• Avoiding baryonic feedback effects on neutrino mass measurements from CMB lensing
• Modelling the matter bispectrum at small scales in modified gravity
• The matter density PDF for modified gravity and dark energy with Large Deviations Theory
• Testing a generalized cubic Galileon gravity model with the Coma Cluster
• Cleaning foregrounds from single-dish 21cm intensity maps with Kernel Principal Component Analysis
• The Void Galaxy Survey
• The Tianlai dish array low-z surveys forecasts
• Marked correlation functions in perturbation theory
• Real-world CMB lensing quadratic estimator power spectrum response
• Building a digital twin of a luminous red galaxy spectroscopic survey: galaxy properties and clustering covariance
• Constraints on Modified Gravity from ACT and SPT
• Imprints of non-standard Dark Energy and Dark Matter Models on the 21cm Intensity Map Power Spectrum
• Testing gravity with gravitational waves $\times$ electromagnetic probes cross-correlations
• Dark energy constraints from the 21~cm intensity mapping surveys with SKA1
• Constraining dark energy using the cross correlations of weak lensing with post-reionization probes of neutral hydrogen
• Opening Reionization: Quantitative Morphology of the Epoch of Reionization and Its Connection to the Cosmic Density Field
• Probing Dark Energy with Alpha Shapes and Betti Numbers
• Marked correlations in galaxy formation models
• Retrieving cosmological information from small-scale CMB foregrounds I. The thermal Sunyaev Zel'dovich effect
• Calibration of systematics in constraining modified gravity models with galaxy cluster mass profiles
• Interferometric HI intensity mapping: perturbation theory predictions and foreground removal effects
• A Study on the Baryon Acoustic Oscillation with Topological Data Analysis
• Weighted density fields as improved probes of modified gravity models
• Searching for dark energy in the matter-dominated era
• A general framework to test gravity using galaxy clusters VI: Realistic galaxy formation simulations to study clusters in modified gravity
• Towards an accurate model of small-scale redshift-space distortions in modified gravity
• Challenges in Constraining Gravity with Cosmic Voids
• High-redshift test of gravity using enhanced growth of small structures probed by the neutral hydrogen distribution
• MGLenS: Modified gravity weak lensing simulations for emulation-based cosmological inference
• On the galaxy 3-point correlation function in Modified Gravity
• The Galaxy Halo Connection in Modified Gravity Cosmologies: Environment Dependence of Galaxy Luminosity function
• A Forecast for Large Scale Structure Constraints on Horndeski Gravity with Line Intensity Mapping
• Model-Independent Test for Gravity using Intensity Mapping and Galaxy Clustering
• Cosmic variance mitigation in measurements of the integrated Sachs-Wolfe effect
• Topological Data Analysis
• Joint analysis of DES Year 3 data and CMB lensing from SPT and Planck III: Combined cosmological constraints
• Testing modified gravity with 21 cm intensity mapping, HI galaxy, cosmic microwave background, optical galaxy, weak lensing, galaxy clustering, type Ia supernovae and gravitational wave surveys

Cited by in corpus (5)

• Sweeping Horndeski Canvas: New Growth-Rate Parameterization for Modified-Gravity Theories
• Constraining gravity with a new precision $E_G$ estimator using Planck + SDSS BOSS
• A Model for the Redshift-Space Galaxy 4-Point Correlation Function
• kSZ Pairwise Velocity Reconstruction with Machine Learning
• Non-Gaussian statistics in galaxy weak lensing: compressed three-point correlations and cosmological forecasts