Large-Scale Structure of the Universe and Cosmological Perturbation Theory

Abstract

We review the formalism and applications of non-linear perturbation theory (PT) to understanding the large-scale structure of the Universe. We first discuss the dynamics of gravitational instability, from the linear to the non-linear regime. This includes Eulerian and Lagrangian PT, non-linear approximations, and a brief description of numerical simulation techniques. We then cover the basic statistical tools used in cosmology to describe cosmic fields, such as correlations functions in real and Fourier space, probability distribution functions, cumulants and generating functions. In subsequent sections we review the use of PT to make quantitative predictions about these statistics according to initial conditions, including effects of possible non Gaussianity of the primordial fields. Results are illustrated by detailed comparisons of PT predictions with numerical simulations. The last sections deal with applications to observations. First we review in detail practical estimators of statistics in galaxy catalogs and related errors, including traditional approaches and more recent developments. Then, we consider the effects of the bias between the galaxy distribution and the matter distribution, the treatment of redshift distortions in three-dimensional surveys and of projection effects in angular catalogs, and some applications to weak gravitational lensing. We finally review the current observational situation regarding statistics in galaxy catalogs and what the future generation of galaxy surveys promises to deliver.

309 pages, 60 figures. Accepted for publication in Physics Reports. Version with 2 pages in 1 available at http://physics.nyu.edu/scoccima/PT/ptreview_final/mptreview2.ps

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• Evidence for suppression of structure growth in the concordance cosmological model
• Galaxy bispectrum, primordial non-Gaussianity and redshift space distortions
• \textsc{CompaSO}: A new halo finder for competitive assignment to spherical overdensities
• Large-N expansions applied to gravitational clustering
• The VIMOS VLT Deep Survey: Evolution of the non-linear galaxy bias up to z=1.5
• Higher order corrections to the large scale matter power spectrum in the presence of massive neutrinos
• Measurement of Parity-Odd Modes in the Large-Scale 4-Point Correlation Function of SDSS BOSS DR12 CMASS and LOWZ Galaxies
• Effective Theory of Large-Scale Structure with Primordial Non-Gaussianity
• Coarse-Grained Cosmological Perturbation Theory
• Cosmology with the EFTofLSS and BOSS: dark energy constraints and a note on priors
• Recursive Solutions of Lagrangian Perturbation Theory
• Large-Scale Structure and Gravitational Waves III: Tidal Effects
• Adhesive Gravitational Clustering
• Hyper Suprime-Cam Year 3 Results: Cosmology from Galaxy Clustering and Weak Lensing with HSC and SDSS using the Minimal Bias Model
• The Local Theory of the Cosmic Skeleton
• The 3-point function in large scale structure: redshift distortions and galaxy bias
• N-Body Simulations of Alternate Gravity Models
• Fast Large Scale Structure Perturbation Theory using 1D FFTs
• Cosmology with the Galaxy Bispectrum Multipoles: Optimal Estimation and Application to BOSS Data
• An analytical approximation of the scalar spectrum in the ultra-slow-roll inflationary models
• Galaxy Bias and Halo-Occupation Numbers from Large-Scale Clustering
• On Separate Universes
• Effective Theory of Dark Energy at Redshift Survey Scales
• Lagrangian perturbations and the matter bispectrum I: fourth-order model for non-linear clustering
• Bias Loop Corrections to the Galaxy Bispectrum
• The 2dF Galaxy Redshift Survey: higher order galaxy correlation functions
• FAST-PT II: an algorithm to calculate convolution integrals of general tensor quantities in cosmological perturbation theory
• Galaxy Bispectrum from Massive Spinning Particles
• On the IR-Resummation in the EFTofLSS
• Cosmological Analysis of Three-Dimensional BOSS Galaxy Clustering and Planck CMB Lensing Cross Correlations via Lagrangian Perturbation Theory
• Non-Gaussian Covariance of the Matter Power Spectrum in the Effective Field Theory of Large Scale Structure
• Phases of New Physics in the BAO Spectrum
• Covariance of cross-correlations: towards efficient measures for large-scale structure
• Cosmological perturbation theory in 1+1 dimensions
• Near optimal bispectrum estimators for large-scale structure
• Lagrangian perturbation theory at one loop order: successes, failures, and improvements
• Fast and accurate mock catalogue generation for low-mass galaxies
• Constructing Regularized Cosmic Propagators
• An analytic model for the bispectrum of galaxies in redshift space
• The 2dF Galaxy Redshift Survey: voids and hierarchical scaling models
• On the reach of perturbative descriptions for dark matter displacement fields
• Tests of Gravity from Imaging and Spectroscopic Surveys
• Schrödinger method as N-body double and UV completion of dust
• Structure formation with massive neutrinos: going beyond linear theory
• Numerical and Perturbative Computations of the Fuzzy Dark Matter Model
• Cross-Correlation of spectroscopic and photometric galaxy surveys: cosmology from lensing and redshift distortions
• Comparing approximate methods for mock catalogues and covariance matrices III: Bispectrum
• Testing the theory of gravity with DESI: estimators, predictions and simulation requirements
• Primordial Non-Gaussianity from Biased Tracers: Likelihood Analysis of Real-Space Power Spectrum and Bispectrum
• Non-Gaussian Formation of Primordial Black Holes: Effects on the Threshold
• The effect of relative velocity and density perturbations between baryons and dark matter on the clustering of galaxies
• Redshift Space Distortions in the Effective Field Theory of Large Scale Structures
• Measuring the growth of matter fluctuations with third-order galaxy correlations
• Systematic Renormalization of the Effective Theory of Large Scale Structure
• Tension of the $E_G$ statistic and RSD data with Planck/$\Lambda$CDM and implications for weakening gravity
• The angle-averaged squeezed limit of nonlinear matter N-point functions
• On the road to percent accuracy IV: ReACT -- computing the non-linear power spectrum beyond $\Lambda$CDM
• A rigorous EFT-based forward model for large-scale structure
• The Three-point Correlation Function of Galaxies Determined from the 2dF Galaxy Redshift Survey
• A Perturbative Approach to the Redshift Space Power Spectrum: Beyond the Standard Model
• The Local Bias Model in the Large Scale Halo Distribution
• Lattice Simulations of Axion-U(1) Inflation
• Single-Field Consistency Relations of Large Scale Structure. Part II: Resummation and Redshift Space
• Improving fast generation of halo catalogs with higher-order Lagrangian perturbation theory
• Constraining the halo bispectrum in real and redshift space from perturbation theory and non-linear stochastic bias
• Towards a self-consistent halo model for the nonlinear large-scale structure
• Thinking Outside the Box: Effects of Modes Larger than the Survey on Matter Power Spectrum Covariance
• Exploring redshift-space distortions in large-scale structure
• Three-Point Correlation Functions of SDSS Galaxies: Luminosity and Color Dependence in Redshift and Projected Space
• MPTbreeze: A fast renormalized perturbative scheme
• Testing the lognormality of the galaxy and weak lensing convergence distributions from Dark Energy Survey maps
• The Trispectrum in the Effective Field Theory of Large Scale Structure
• On the non-linear scale of cosmological perturbation theory
• The 2dF Galaxy Redshift Survey: Hierarchical galaxy clustering
• Distribution function approach to redshift space distortions. Part IV: perturbation theory applied to dark matter
• Accelerating the 2-point and 3-point galaxy correlation functions using Fourier transforms
• Back in the saddle: Large-deviation statistics of the cosmic log-density field
• From Weak Lensing to non-Gaussianity via Minkowski Functionals
• Perturbation theory approach to predict the covariance matrices of the galaxy power spectrum and bispectrum in redshift space
• Testing one-loop galaxy bias: joint analysis of power spectrum and bispectrum
• Reduced Shear Power Spectrum
• Stochastic Bias from Non-Gaussian Initial Conditions
• The bispectrum of relativistic galaxy number counts
• Complete super-sample lensing covariance in the response approach
• Higher Order Contributions to the 21 cm Power Spectrum
• Precision modeling of redshift-space distortions from multi-point propagator expansion
• The Impact of Box Size on the Properties of Dark Matter Haloes in Cosmological Simulations
• Non-Gaussian Minkowski functionals & extrema counts in redshift space
• Resummed propagators in multi-component cosmic fluids with the eikonal approximation
• A bias to CMB lensing measurements from the bispectrum of large-scale structure
• Higher-order initial conditions for mixed baryon-CDM simulations
• Baryonic Acoustic Oscillations via the Renormalization Group
• Distribution function approach to redshift space distortions. Part II: N-body simulations
• On the impact of galaxy bias uncertainties on primordial non-Gaussianity constraints
• Optimizing large-scale structure data analysis with the theoretical error likelihood
• The 21cm bispectrum as a probe of non-Gaussianities due to X-ray heating
• Cosmological structure formation with clustering quintessence
• How unusual are the Shapley Supercluster and the Sloan Great Wall?
• 21cm-line bispectrum as method to probe Cosmic Dawn and Epoch of Reionization
• Three-Point Correlation Functions of SDSS Galaxies: Constraining Galaxy-Mass Bias
• Galaxy redshift-space bispectrum: the Importance of Being Anisotropic
• The Three-point Correlation Function of Galaxies: Comparing Halo Occupation Models with Observations
• Nonlinear Effective Theory of Dark Energy
• Primordial Features from Linear to Nonlinear Scales
• Galaxy bias and primordial non-Gaussianity: insights from galaxy formation simulations with IllustrisTNG
• Cosmological constraints from galaxy-lensing cross correlations using BOSS galaxies with SDSS and CMB lensing
• A new approach to gravitational clustering: a path-integral formalism and large-N expansions
• Consequences of Symmetries and Consistency Relations in the Large-Scale Structure of the Universe for Non-local bias and Modified Gravity
• Generating Log-normal Mock Catalog of Galaxies in Redshift Space
• Statistical properties of paired fixed fields
• Measuring the Integrated Sachs-Wolfe Effect
• The recursion relation in Lagrangian perturbation theory
• Perturbative approach to covariance matrix of the matter power spectrum
• Cosmic microwave background bispectrum on small angular scales
• The intrinsic bispectrum of the Cosmic Microwave Background [PhD thesis]
• The Large-Scale 3-point correlation function of SDSS Luminous Red Galaxies
• Large scale structure in non-standard cosmologies
• Primordial non-Gaussianity in the large scale structure of the Universe
• Toward a robust inference method for the galaxy bispectrum: likelihood function and model selection
• DEMNUni: Massive neutrinos and the bispectrum of large scale structures
• Distribution function approach to redshift space distortions, Part III: halos and galaxies
• Dark Energy and Modified Gravity in the Effective Field Theory of Large-Scale Structure
• Optimal capture of non-Gaussianity in weak lensing surveys: power spectrum, bispectrum and halo counts
• Impact on the power spectrum of Screening in Modified Gravity Scenarios
• Primordial non-Gaussianity without tails -- how to measure fNL with the bulk of the density PDF
• On the signature of the baryon-dark matter relative velocity in the two and three-point galaxy correlation functions
• Bayesian analysis of the dynamic cosmic web in the SDSS galaxy survey
• Generalized Chaplygin Gas in a modified gravity approach
• Joint analysis of anisotropic power spectrum, bispectrum and trispectrum: application to N-body simulations
• CMB lensing reconstruction biases in cross-correlation with large-scale structure probes
• Inverted initial conditions: exploring the growth of cosmic structure and voids
• Cosmological parameters from the likelihood analysis of the galaxy power spectrum and bispectrum in real space
• The Weak Lensing Bispectrum
• Third-order Perturbation Theory With Non-linear Pressure
• An analytic implementation of the IR-resummation for the BAO peak
• Ward identities and consistency relations for the large scale structure with multiple species
• Going Beyond the Galaxy Power Spectrum: an Analysis of BOSS Data with Wavelet Scattering Transforms
• The Weak Lensing Masses of Filaments between Luminous Red Galaxies
• The Benefits of CMB Delensing
• Rapid Separable Analysis of Higher Order Correlators in Large Scale Structure
• Gravitational Lensing Simulations I : Covariance Matrices and Halo Catalogues
• Detecting Bispectral Acoustic Oscillations from Inflation Using a New Flexible Estimator
• ColDICE: a parallel Vlasov-Poisson solver using moving adaptive simplicial tessellation
• The clustering of galaxies in the completed SDSS-III Baryon Oscillation Spectroscopic Survey: a tomographic analysis of structure growth and expansion rate from anisotropic galaxy clustering
• Large scale structure from viscous dark matter
• Modeling the large-scale redshift-space 3-point correlation function of galaxies
• Modeling the three-point correlation function
• Linear perturbative theory of the discrete cosmological N-body problem
• Galaxy bias from forward models: linear and second-order bias of IllustrisTNG galaxies
• An iterative reconstruction of cosmological initial density fields
• Skewness as a test of the equivalence principle
• Bias, redshift space distortions and primordial nongaussianity of nonlinear transformations: application to Lyman alpha forest
• The Monopole Moment of the Three-Point Correlation Function of the 2-degree Field Galaxy Redshift Survey
• Fitting the nonlinear matter bispectrum by the Halofit approach
• Responses in Large-Scale Structure
• Linear response to long wavelength fluctuations using curvature simulations
• Matter bispectrum in cubic Galileon cosmologies
• Accurate emulator for the redshift-space power spectrum of dark matter halos and its application to galaxy power spectrum
• Non-linear hydrodynamics of axion dark matter: relative velocity effects and "quantum forces"
• On the incompleteness of the moment and correlation function hierarchy as probes of the lognormal field
• The BACCO simulation project: biased tracers in real space
• Deriving an Accurate Formula of Scale-dependent Bias with Primordial Non-Gaussianity: An Application of the Integrated Perturbation Theory
• Observable Deviations from Homogeneity in an Inhomogeneous Universe
• Peculiar Velocity Decomposition, Redshift Space Distortion and Velocity Reconstruction in Redshift Surveys. II. Dark Matter Velocity Statistics
• Impact of Scale Dependent Bias and Nonlinear Structure Growth on the ISW Effect: Angular Power Spectra
• Towards Precision Constraints on Gravity with the Effective Field Theory of Large-Scale Structure
• The Halo Bispectrum in N-body Simulations with non-Gaussian Initial Conditions
• Forecasts on Primordial non-Gaussianity from 21 cm Intensity Mapping experiments
• Maximal compression of the redshift space galaxy power spectrum and bispectrum
• Nonlinear clustering in models with primordial non-Gaussianity: the halo model approach
• Time-sliced perturbation theory with primordial non-Gaussianity and effects of large bulk flows on inflationary oscillating features
• The Effective Field Theory of Large Scale Structure at Three Loops
• Cosmological perturbation theory for baryons and dark matter I: one-loop corrections in the RPT framework
• Very Massive Tracers and Higher Derivative Biases
• Peculiar velocities in redshift space: formalism, N-body simulations and perturbation theory
• Streaming velocities and the baryon-acoustic oscillation scale
• Nonlinear Biasing and Redshift-Space Distortions in Lagrangian Resummation Theory and N-body Simulations
• Cosmological constraints from the BOSS DR12 void size function
• An $n$-th order Lagrangian Forward Model for Large-Scale Structure
• Euclid: impact of nonlinear prescriptions on cosmological parameter estimation from weak lensing cosmic shear
• The missing link: a nonlinear post-Friedmann framework for small and large scales
• Scale Dependence of Halo Bispectrum from Non-Gaussian Initial Conditions in Cosmological N-body Simulations
• Predictions for local PNG bias in the galaxy power spectrum and bispectrum and the consequences for $f_{\mathrm{NL}}$ constraints
• Distribution function approach to redshift space distortions. Part V: perturbation theory applied to dark matter halos
• Dark matter and halo bispectrum in redshift space: theory and applications
• The Clustering of Galaxies in the SDSS-III Baryon Oscillation Spectroscopic Survey: Measuring H(z) and D_A(z) at z = 0.57 with Clustering Wedges
• Primordial Gravitational Waves from Galaxy Intrinsic Alignments
• On the inadequacy of N-point correlation functions to describe nonlinear cosmological fields: explicit examples and connection to simulations
• How close can an Inhomogeneous Universe mimic the Concordance Model?
• CARPool: fast, accurate computation of large-scale structure statistics by pairing costly and cheap cosmological simulations
• GridSPT: Grid-based calculation for perturbation theory of large-scale structure
• Lensing Reconstruction in Post-Born Cosmic Microwave Background Weak Lensing
• IR-safe and UV-safe integrands in the EFTofLSS with exact time dependence
• Cosmological constraints on Lorentz violating dark energy
• Lagrangian or Eulerian; Real or Fourier? Not All Approaches to Large-Scale Structure Are Created Equal
• Signatures of Horndeski gravity on the Dark Matter Bispectrum
• Nonlinear Power Spectrum from Resummed Perturbation Theory: a Leap Beyond the BAO Scale
• Approximate Bayesian Computation in Large Scale Structure: constraining the galaxy-halo connection
• Impact of the non-Gaussian covariance of the weak lensing power spectrum and bispectrum on cosmological parameter estimation
• Gravitational Waves from Density Perturbations in an Early Matter Domination Era
• The DEEP2 Galaxy Redshift Survey: The Evolution of Void Statistics from z~1 to z~0
• Baryonic effects on the matter bispectrum
• Response function of the large-scale structure of the universe to the small scale inhomogeneities
• The Persistence of Large Scale Structures I: Primordial non-Gaussianity
• LyaCoLoRe: Synthetic Datasets for Current and Future Lyman-$\alpha$ Forest BAO Surveys
• Inflationary soft theorems revisited: A generalized consistency relation
• Cosmological nonlinear hydrodynamics with post-Newtonian corrections
• Matter bispectrum of large-scale structure: Three-dimensional comparison between theoretical models and numerical simulations
• Baryon Oscillations and Dark-Energy Constraints from Imaging Surveys
• The kinetic SZ tomography with spectroscopic redshift surveys
• Large-scale tidal effect on redshift-space power spectrum in a finite-volume survey
• Cosmic Structure and Dynamics of the Local Universe
• Non-linear Fields in Generalized Cosmologies
• Precision cosmology with redshift-space bispectrum: a perturbation theory based model at one-loop order
• Clipping the Cosmos: The Bias and Bispectrum of Large Scale Structure
• The effect of baryons on the variance and the skewness of the mass distribution in the universe at small scales
• Quantifying distortions of the Lagrangian dark-matter mesh in cosmology
• Probing gravity with a joint analysis of galaxy and CMB lensing and SDSS spectroscopy
• Chasing the non-linear evolution of matter power spectrum with numerical resummation method: solution of closure equations
• New Optimised Estimators for the Primordial Trispectrum
• Modelling The Redshift-Space Three-Point Correlation Function in SDSS-III
• A Lagrangian Perturbation Theory in the presence of massive neutrinos
• Galaxy power-spectrum responses and redshift-space super-sample effect
• The evolution of clustering length, large-scale bias and host halo mass at 2<z<5 in the VIMOS Ultra Deep Survey (VUDS)
• The Hunt for Primordial Interactions in the Large Scale Structures of the Universe
• The Cosmic Microwave Background: The history of its experimental investigation and its significance for cosmology
• Modeling CMB Lensing Cross Correlations with {\sc CLEFT}
• Next-to-leading resummation of cosmological perturbations via the Lagrangian picture: 2-loop correction in real and redshift spaces
• Lagrangian perturbation theory for modified gravity
• Biased Tracers in Redshift Space in the EFTofLSS with exact time dependence
• Peculiar Velocity Decomposition, Redshift Space Distortion and Velocity Reconstruction in Redshift Surveys - I. The Methodology
• Constraints on modified gravity from the BOSS galaxy survey
• Baryon Acoustic Oscillation Theory and Modelling Systematics for the DESI 2024 results
• Power spectrum of halo intrinsic alignments in simulations
• Hierarchical clustering in chameleon $f(R)$ gravity
• Halo Zeldovich model and perturbation theory: dark matter power spectrum and correlation function
• The matter power spectrum in redshift space using effective field theory
• Tests of General Relativity on Astrophysical Scales
• Modified Dust and the Small Scale Crisis in CDM
• Unbiased Cosmology Inference from Biased Tracers using the EFT Likelihood
• FFT-PT: Reducing the two-loop large-scale structure power spectrum to low-dimensional radial integrals
• ENCORE: An $\mathcal{O}(N_{\mathrm{g}}^2)$ Estimator for Galaxy $N$-Point Correlation Functions
• Including beyond-linear halo bias in halo models
• Probing Primordial Chirality with Galaxy Spins
• Game of cones: A nulling strategy for modelling lensing convergence in cones with large deviation theory
• Capturing Non-Gaussianity of the Large-Scale Structure with Weighted Skew-Spectra
• Galaxy power spectrum in redshift space: combining perturbation theory with the halo model
• Regularized cosmological power spectrum and correlation function in modified gravity models
• The Generation of Vorticity in Cosmological N-body Simulations
• Beyond consistency test of gravity with redshift-space distortions at quasi-linear scales
• Exploring galaxies-gravitational waves cross-correlations as an astrophysical probe
• Non-Gaussianities due to Relativistic Corrections to the Observed Galaxy Bispectrum
• Separate Universe Simulations with IllustrisTNG: baryonic effects on power spectrum responses and higher-order statistics
• Towards optimal cosmological parameter recovery from compressed bispectrum statistics
• Testing one-loop galaxy bias: Power spectrum
• Cosmological constraints from the convergence 1-point probability distribution
• Perturbation theory approach for the power spectrum: from dark matter in real space to massive haloes in redshift space
• Large non-Gaussian Halo Bias from Single Field Inflation
• Time evolution of intrinsic alignments of galaxies
• Perturbation theory and excursion set estimates of the probability distribution function of dark matter, and a method for reconstructing the initial distribution function
• Structure Formation in Modified Gravity Scenarios
• Statistics of cosmic density profiles from perturbation theory
• Time drift of cosmological redshifts and its variance
• Modeling Dark Photon Oscillations in Our Inhomogeneous Universe
• Cosmic shear bispectrum from second-order perturbations in General Relativity
• Estimating cosmic velocity fields from density fields and tidal tensors
• Dark matter voids in the SDSS galaxy survey
• Consistent Modified Gravity Analysis of Anisotropic Galaxy Clustering Using BOSS DR11
• Modelling large-scale halo bias using the bispectrum
• Matter power spectrum from a Lagrangian-space regularization of perturbation theory
• Angular averaged consistency relations of large-scale structures
• What does the Marked Power Spectrum Measure? Insights from Perturbation Theory
• Effects of the size of cosmological N-Body simulations on physical quantities -- I: Mass Function
• Simulations of Baryon Acoustic Oscillations I: Growth of Large-Scale Density Fluctuations
• Tree-Level Bispectrum in the Effective Field Theory of Large-Scale Structure extended to Massive Neutrinos
• Higher-order massive neutrino perturbations in large-scale structure
• Precision modelling of the matter power spectrum in a Planck-like Universe
• A new approach to the propagation of light-like signals in perturbed cosmological backgrounds
• Fast Estimation of Gravitational and Primordial Bispectra in Large Scale Structures
• The integrated 3-point correlation function of cosmic shear
• Impact of shell crossing and scope of perturbative approaches in real and redshift space
• Second-order perturbations of cosmological fluids: Relativistic effects of pressure, multi-component, curvature, and rotation
• Cosmological inference from the EFTofLSS: the eBOSS QSO full-shape analysis
• Fast computation of non-linear power spectrum in cosmologies with massive neutrinos
• Improving the modelling of redshift-space distortions - II. A pairwise velocity model covering large and small scales
• The Next Generation Fornax Survey (NGFS): III. Revealing the Spatial Substructure of the Dwarf Galaxy Population inside half of Fornax's Virial Radius
• Linearisation with Cosmological Perturbation Theory
• Correlation between galaxies and QSO in the SDSS:na signal from gravitational lensing magnification?
• Model-independent analyses of non-Gaussianity in Planck CMB maps using Minkowski Functionals
• Power spectra in the eikonal approximation with adiabatic and non-adiabatic modes
• The one-loop matter bispectrum as a probe of gravity and dark energy
• On the cross-correlation of sub-mm sources and optically-selected galaxies
• General relativistic weak-field limit and Newtonian N-body simulations
• Relativistic wide-angle galaxy bispectrum on the light-cone
• Joint likelihood function of cluster counts and $n$-point correlation functions: Improving their power through including halo sample variance
• An Improved Calculation of the Non-Gaussian Halo Mass Function
• A general relativistic signature in the galaxy bispectrum: the local effects of observing on the lightcone
• Inflationary signatures of single-field models beyond slow-roll
• Non-linear evolution of the BAO scale in alternative theories of gravity
• How to generate a significant effective temperature for cold dark matter, from first principles
• Epoch of reionization parameter estimation with the 21-cm bispectrum
• The Bacco Simulation Project: Bacco Hybrid Lagrangian Bias Expansion Model in Redshift Space
• Post-collapse perturbation theory in 1D cosmology -- beyond shell-crossing
• Non-linear Matter Spectra in Coupled Quintessence
• Testing standard perturbation theory and the Eulerian local biasing scheme against N-body simulations
• Strategies to Detect Dark-Matter Decays with Line-Intensity Mapping
• On the reach of perturbative methods for dark matter density fields
• CMB-lensing beyond the leading order: temperature and polarization anisotropies
• Clustering in Massive Neutrino Cosmologies via Eulerian Perturbation Theory
• Voronoi volume function: A new probe of cosmology and galaxy evolution
• Bispectrum Supersample Covariance
• The Full-Sky Angular Bispectrum in Redshift Space
• Biasing and the search for primordial non-Gaussianity beyond the local type
• Optimal Weighting in Galaxy Surveys: Application to Redshift-Space Distortions
• Multi-Point Propagators for Non-Gaussian Initial Conditions
• Fractal Dimensions of a Weakly Clustered Distribution and the Scale of Homogeneity
• Edgeworth streaming model for redshift space distortions
• How smooth are particle trajectories in a $\Lambda$CDM Universe?
• Perturbation theory for modeling galaxy bias: validation with simulations of the Dark Energy Survey
• Signatures of Primordial non-Gaussianities in the Matter Power-Spectrum and Bispectrum: the Time-RG Approach
• Spherical collapse, formation hysteresis and the deeply non-linear cosmological power spectrum
• The Reconstructed Power Spectrum in the Zeldovich Approximation
• On the Bispectra of Very Massive Tracers in the Effective Field Theory of Large-Scale Structure
• Galactic angular momenta and angular momentum couplings in the large-scale structure
• Hunting high and low: Disentangling primordial and late-time non-Gaussianity with cosmic densities in spheres
• Lensing reconstruction from line intensity maps: the impact of gravitational nonlinearity
• Position-dependent correlation function from the SDSS-III Baryon Oscillation Spectroscopic Survey Data Release 10 CMASS Sample
• Constructing perturbation theory kernels for large-scale structure in generalized cosmologies
• Lyman-$\alpha$ forest constraints on interacting dark sectors
• Cosmic propagators at two-loop order
• Response Approach to the Matter Power Spectrum Covariance
• Cosmological constraints from galaxy clustering in the presence of massive neutrinos
• Bispectrum of cosmological density perturbations in the most general second-order scalar-tensor theory
• The Halo Bispectrum Multipoles in Redshift Space
• Third order perturbations of a zero-pressure cosmological medium: Pure general relativistic nonlinear effects
• Integrated Perturbation Theory and One-loop Power Spectra of Biased Tracers
• Information Content of Higher-Order Galaxy Correlation Functions
• Using the Zeldovich dynamics to test expansion schemes
• The two-mode puzzle: Confronting self-interacting neutrinos with the full shape of the galaxy power spectrum
• Combining perturbation theories with halo models for the matter bispectrum
• Biased Tracers of Two Fluids in the Lagrangian Picture
• Consistency tests of field level inference with the EFT likelihood
• Validating a minimal galaxy bias method for cosmological parameter inference using HSC-SDSS mock catalogs
• Extragalactic gamma-ray signal from Dark Matter annihilation: a power spectrum based computation
• Towards a self-consistent analysis of the anisotropic galaxy two- and three-point correlation functions on large scales: application to mock galaxy catalogues
• Perturbative description of bias tracers using consistency relations of LSS
• Effective perfect fluids in cosmology
• Propagators in Lagrangian space
• Einstein's signature in cosmological large-scale structure
• Fast and accurate predictions of the nonlinear matter power spectrum for general models of Dark Energy and Modified Gravity
• Statistical Cosmology with Quadratic Density Fields
• A Large Deviation Principle at play in Large-Scale Structure cosmology
• The effect of early radiation in N-body simulations of cosmic structure formation
• Kinematic consistency relations of large-scale structures
• Precision Tests of CO and [CII] Power Spectra Models against Simulated Intensity Maps
• Non-Gaussianity in Large Scale Structure and Minkowski Functionals
• Higher-order initial conditions with massive neutrinos
• Modified gravity and massive neutrinos: constraints from the full shape analysis of BOSS galaxies and forecasts for Stage IV surveys
• The impact of large-scale tides on cosmological distortions via redshift-space power spectrum
• Optimal non-linear transformations for large scale structure statistics
• Phase-space structure of protohalos: Vlasov versus Particle-Mesh
• Baryon acoustic oscillations signature in the three-point angular correlation function from the SDSS-DR12 quasar survey
• Contributions to the Dark Matter 3-Pt Function from the Radiation Era
• An accurate perturbative approach to redshift space clustering of biased tracers in modified gravity
• Theoretical Accuracy in Cosmological Growth Estimation
• A Robust Measure of Cosmic Structure beyond the Power-Spectrum: Cosmic Filaments and the Temperature of Dark Matter
• Precise Cosmological Constraints from BOSS Galaxy Clustering with a Simulation-Based Emulator of the Wavelet Scattering Transform
• Non-perturbative probability distribution function for cosmological counts in cells
• The intergalactic medium temperature and Compton y parameter
• Detecting the relativistic galaxy bispectrum
• Skewness as a test for Quartessence
• Euclid: Reconstruction of Weak Lensing mass maps for non-Gaussianity studies
• Bispectrum covariance in the flat-sky limit
• Loop corrections to the power spectrum for massive neutrino cosmologies with full time- and scale-dependence
• The VIMOS VLT Deep Survey: Computing the two point correlation statistics and associated uncertainties
• Testing Modified Gravity with Cosmic Shear
• Estimating the power spectrum covariance matrix with fewer mock samples
• Galaxy Clustering Analysis with SimBIG and the Wavelet Scattering Transform
• CoLoRe: fast cosmological realisations over large volumes with multiple tracers
• The Effective Halo Model: Creating a Physical and Accurate Model of the Matter Power Spectrum and Cluster Counts
• The Matter Bispectrum in N-body Simulations with non-Gaussian Initial Conditions
• Precise Calibration of the One-Loop Bispectrum in the Effective Field Theory of Large Scale Structure
• Effect of lensing non-Gaussianity on the CMB power spectra
• Bispectrum-window convolution via Hankel transform
• Moving around the cosmological parameter space: a nonlinear power spectrum reconstruction based on high-resolution cosmic responses
• Statistical analysis of galaxy surveys - III: The non-linear clustering of red and blue galaxies in the 2dFGRS
• Renormalized Newtonian Cosmic Evolution with Primordial Non-Gaussianity
• Self-calibration of weak lensing systematic effects using combined two- and three-point statistics
• Large-scale structure perturbation theory without losing stream crossing
• Estimating Covariance Matrices for Two- and Three-Point Correlation Function Moments in Arbitrary Survey Geometries
• Expansion schemes for gravitational clustering: computing two-point and three-point functions
• $\mathrm{S}\mathrm{IM}\mathrm{BIG}$: Mock Challenge for a Forward Modeling Approach to Galaxy Clustering
• Light propagation in inhomogeneous and anisotropic cosmologies
• Primordial Non-Gaussianity and Extreme-Value Statistics of Galaxy Clusters
• Intrinsic alignment statistics of density and velocity fields at large scales: Formulation, modeling, and baryon acoustic oscillation features
• Projected-Field Kinetic Sunyaev-Zel'dovich Cross-Correlations: Halo Model and Forecasts
• The two-loop bispectrum of large-scale structure
• Consistency relations for large-scale structure in modified gravity and the matter bispectrum
• Missing one-loop contributions in secondary gravitational waves
• Next-to-leading resummations in cosmological perturbation theory
• A new model to predict weak-lensing peak counts III. Filtering technique comparisons
• One-point remapping of Lagrangian perturbation theory in the mildly non-linear regime of cosmic structure formation
• Reconstruction of a Nonminimal Coupling Theory with Scale-invariant Power Spectrum
• Perturbation theory challenge for cosmological parameters estimation: Matter power spectrum in real space
• Cosmic Structure Formation with Kinetic Field Theory
• The squeezed matter bispectrum covariance with responses
• Non-Gaussianity of the Cosmic Infrared Background anisotropies I : Diagrammatic formalism and application to the angular bispectrum
• Why Newton's gravity is practically reliable in the large-scale cosmological simulations
• Proper-Time Hypersurface of Non-Relativistic Matter Flows: Galaxy Bias in General Relativity
• The initial shear field in models with primordial local non-Gaussianity and implications for halo and void abundances
• Separating the Universe into the Real and Fake
• Non-linear contributions to angular power spectra
• Non-local bias in the halo bispectrum with primordial non-Gaussianity
• Accurate predictions from small boxes: variance suppression via the Zel'dovich approximation
• Vlasov-Poisson in 1D for initially cold systems: post-collapse Lagrangian perturbation theory
• Redshift-space streaming velocity effects on the Lyman-$\alpha$ forest baryon acoustic oscillation scale
• Baryon-CDM isocurvature galaxy bias with IllustrisTNG
• Principal Shapes and Squeezed Limits in the Effective Field Theory of Large Scale Structure
• The ALHAMBRA survey: evolution of galaxy clustering since $z\sim 1$
• The phase-space structure of nearby dark matter as constrained by the SDSS
• Non-linear matter power spectrum from Time Renormalisation Group: efficient computation and comparison with one-loop
• Power Spectrum of Cosmic Momentum Field Measured from the SFI Galaxy Sample
• DEMNUni: comparing nonlinear power spectra prescriptions in the presence of massive neutrinos and dynamical dark energy
• The Intrinsic Matter Bispectrum in $\Lambda$CDM
• Testing signatures of phantom crossing through full-shape galaxy clustering analysis
• Sampling Artifact in Volume Weighted Velocity Measurement.--- I. Theoretical Modelling
• Extragalactic gamma-ray signal from dark matter annihilation: an appraisal
• Lagrangian cosmological perturbation theory at shell-crossing
• Precise and Accurate Cosmology with CMBxLSS Power Spectra and Bispectra
• The observed galaxy bispectrum from single-field inflation in the squeezed limit
• A coarse grained perturbation theory for the Large Scale Structure, with cosmology and time independence in the UV
• Statistical properties of the Burgers equation with Brownian initial velocity
• Structure formation beyond shell-crossing: nonperturbative expansions and late-time attractors
• Phase Correlations in Non-Gaussian Fields
• Galaxy Clustering and Dark Energy
• Power spectrum for the small-scale Universe
• How does non-linear dynamics affect the baryon acoustic oscillation?
• Exploring KSZ velocity reconstruction with $N$-body simulations and the halo model
• Mass functions and bias of dark matter halos
• Precision cosmology in muddy waters: Cosmological constraints and N-body codes
• Cosmological perturbations for two cold fluids in $\Lambda$CDM
• Cosmological inference from emulator based halo model I: Validation tests with HSC and SDSS mock catalogs
• Remapping dark matter halo catalogues between cosmological simulations
• A fitting formula for the non-Gaussian contribution to the lensing power spectrum covariance
• Three-Point Correlations in f(R) Models of Gravity
• NECOLA: Towards a Universal Field-level Cosmological Emulator
• Linear and non-linear bias: predictions vs. measurements
• The Power of Locality: Primordial Non-Gaussianity at the Map Level
• Cosmic Purity Lost: Perturbative and Resummed Late-Time Inflationary Decoherence
• Gravitational Binding, Virialization and the Peculiar Velocity Distribution of the Galaxies
• Simulations and cosmological inference: A statistical model for power spectra means and covariances
• Testing tidal alignment models for anisotropic correlations of halo ellipticities with N-body simulations
• The cosmic web for density perturbations of various scales
• Wide-angle and relativistic effects in Fourier-space clustering statistics
• Semiclassical path to cosmic large-scale structure
• Nonlinear evolution of initially biased tracers in modified gravity
• Perturbation Theory for BAO reconstructed fields: one-loop results in real-space matter density field
• Clipping the Cosmos II: Cosmological information from non-linear scales
• What Can We Learn by Combining the Skew Spectrum and the Power Spectrum?
• Interacting dark energy from the joint analysis of the power spectrum and bispectrum multipoles with the EFTofLSS
• Extracting bias using the cross-bispectrum: An EoR and 21 cm-[CII]-[CII] case study
• ${\Lambda }_{\mathrm{s}}$CDM cosmology: Alleviating major cosmological tensions by predicting standard neutrino properties
• Constraining Primordial Non-Gaussianity with Post-reconstructed Galaxy Bispectrum in Redshift Space
• Gaussianizing the non-Gaussian lensing convergence field I: the performance of the Gaussianization
• Halo Sampling, Local Bias and Loop Corrections
• Nonlinear cosmological consistency relations and effective matter stresses
• Cosmological gravity on all scales II: Model independent modified gravity $N$-body simulations
• Measuring nonlocal Lagrangian peak bias
• How the Big Bang Ends up Inside a Black Hole
• How Density Environment Changes the Influence of the Dark Matter-Baryon Streaming Velocity on the Cosmological Structure Formation
• Covariance of the galaxy angular power spectrum with the halo model
• Euclid: The search for primordial features
• Cosmological Perturbation Theory Using the Schrödinger Equation
• Higher-Order Angular Galaxy Correlations in the SDSS: Redshift and Color Dependence of non-Linear Bias
• New constraints on cosmological modified gravity theories from anisotropic three-point correlation functions of BOSS DR12 galaxies
• Cosmological information content in redshift-space power spectrum of SDSS-like galaxies in the quasi-nonlinear regime up to $k=0.3h$Mpc${}^{-1}$
• Precision Measurements of Higher-Order Angular Galaxy Correlations Using 11 Million SDSS Galaxies
• Equal-time Consistency Relations in the Large-Scale Structure of the Universe
• Vorticity generation in the Universe: A perturbative approach
• Responses of Halo Occupation Distributions: a new ingredient in the halo model & the impact on galaxy bias
• Fast Generation of Covariance Matrices for Weak Lensing
• The structure of correlation functions in single field inflation
• Characteristic Scales of Baryon Acoustic Oscillations from Perturbation Theory: Non-linearity and Redshift-Space Distortion Effects
• Dynamical flows through Dark Matter Haloes: Inner perturbative dynamics, secular evolution, and applications
• Non-local bias contribution to third-order galaxy correlations
• Statistical Analysis of Galaxy Surveys-IV: An objective way to quantify the impact of superstructures on galaxy clustering statistics
• Global view of neutrino interactions in cosmology: The freestreaming window as seen by Planck
• Revealing modified gravity signal in matter and halo hierarchical clustering
• A new method to measure galaxy bias
• Trajectories of point particles in cosmology and the Zel'dovich approximation
• Going Nonlinear with Dark Energy Cosmologies
• The Halo Void (Dust) Model of Large Scale Structure
• Kinematic Morphology of Large-scale Structure: Evolution from Potential to Rotational Flow
• Non-linear dark energy clustering
• Three-point phase correlations: A new measure of non-linear large-scale structure
• Tidal alignments as a contaminant of the galaxy bispectrum
• Renormalization-group flow of the effective action of cosmological large-scale structures
• Second order perturbations of a zero-pressure cosmological medium: Proofs of the relativistic-Newtonian correspondence
• Imprints of local lightcone projection effects on the galaxy bispectrum. II
• An improved model of redshift-space distortions around voids: application to quintessence dark energy
• Primordial non-Gaussianity in the bispectra of large-scale structure
• Radiation-induced large-scale structure during the reionization epoch: the autocorrelation function
• Redshift space power spectrum beyond Einstein-de Sitter kernels
• Higher order relativistic galaxy number counts: dominating terms
• General relativistic 'screening' in cosmological simulations
• Bayesian weak lensing tomography: Reconstructing the 3D large-scale distribution of matter with a lognormal prior
• The halo light cone catalogues of \Abacus{AbacusSummit}
• A direct measure of free electron gas via the Kinematic Sunyaev-Zel'dovich effect in Fourier-space analysis
• Probability distribution function of the aperture mass field with large deviation theory
• Covariance matrices for halo number counts and correlation functions
• The Weak Lensing Bispectrum Induced By Gravity
• The Effective Field Theory of Large-Scale Structure and Multi-tracer
• Unveiling dark forces with measurements of the Large Scale Structure of the Universe
• Helmholtz Decomposition of the Lagrangian Displacement
• Pair Correlations and Merger Bias
• Cosmological Large-scale Structures beyond Linear Theory in Modified Gravity
• A First Detection of the Connected 4-Point Correlation Function of Galaxies Using the BOSS CMASS Sample
• Second-order matter density perturbations and skewness in scalar-tensor modified gravity models
• Cosmological constraints from the power spectrum and bispectrum of 21cm intensity maps
• BOSS full-shape analysis from the EFTofLSS with exact time dependence
• Convolution Lagrangian perturbation theory for biased tracers beyond general relativity
• New fitting formula for cosmic non-linear density distribution
• The Ly$\alpha$ forest flux correlation function: a perturbation theory perspective
• Precise Calibration of the One-Loop Trispectrum in the Effective Field Theory of Large Scale Structure
• Weakly non-Gaussian formula for the Minkowski functionals in general dimensions
• One line to run them all: SuperEasy massive neutrino linear response in $N$-body simulations
• Covariance of the matter power spectrum including the survey window function effect: N-body simulations vs. fifth-order perturbation theory on grid
• Relativistic-Newtonian correspondence of the zero-pressure but weakly nonlinear cosmology
• Accurate initial conditions in mixed Dark Matter--Baryon simulations
• Cylinders out of a top hat: counts-in-cells for projected densities
• Imprints of local lightcone projection effects on the galaxy bispectrum. III Relativistic corrections from nonlinear dynamical evolution on large-scales
• Growth of structure in interacting vacuum cosmologies
• Non-Spherical Szekeres models in the language of Cosmological Perturbations
• The effect of non-Gaussian curvature perturbations on the formation of primordial black holes
• Hierarchy of N-point functions in the LCDM and ReBEL cosmologies
• Unveiling the nonlinear dynamics of a rolling axion during inflation
• The Impact of Nonlinear Structure Formation on the Power Spectrum of Transverse Momentum Fluctuations and the Kinetic Sunyaev-Zel'dovich Effect
• Non-Gaussianity from Self-Ordering Scalar Fields
• The large-scale correlations of multi-cell densities and profiles, implications for cosmic variance estimates
• Light Fields during Inflation from BOSS and Future Galaxy Surveys
• The HI intensity mapping bispectrum including observational effects
• A new model for the full shape of the large-scale power spectrum
• The two and three-loop matter bispectrum in perturbation theories
• Unveiling the singular dynamics in the cosmic large-scale structure
• Disentangling interacting dark energy cosmologies with the three-point correlation function
• Violation of the consistency relations for large-scale structure with dark energy
• Probing primordial non-Gaussianity with the power spectrum and bispectrum of future 21cm intensity maps
• How well can (renormalized) perturbation theory predict dark matter clustering properties?
• A Bayesian method for combining theoretical and simulated covariance matrices for large-scale structure surveys
• Testing the equal-time angular-averaged consistency relation of the gravitational dynamics in N-body simulations
• Neutrino mass bounds from confronting an effective model with BOSS Lyman-alpha data
• Relativistic Lagrangian displacement field and tensor perturbations
• Impact of bias and redshift-space modelling for the halo power spectrum: Testing the effective field theory of large-scale structure
• General relativistic effects on non-linear power spectra
• Higher-order Convergence Statistics for Three-dimensional Weak Gravitational Lensing
• The Effect of Local non-Gaussianity on the Matter Bispectrum at Small Scales
• Unbiased Cosmological Parameter Estimation from Emission Line Surveys with Interlopers
• Evolution of hierarchical clustering in the CFHTLS-Wide since z~1
• The Integrated Bispectrum and Beyond
• Primordial non-Gaussianity and non-Gaussian Covariance
• The joint statistics of mildly non-linear cosmological densities and slopes in count-in-cells
• Fisher Forecasts for Primordial non-Gaussianity from Persistent Homology
• Why is the Zel'dovich Approximation so Accurate?
• The BINGO Project V: Further steps in Component Separation and Bispectrum Analysis
• The cosmic neutrino background as a collection of fluids in large-scale structure simulations
• Third order solutions of the cosmological density perturbations in the Horndeski's most general scalar-tensor theory with the Vainshtein mechanism
• Perturbation theory with dispersion and higher cumulants: non-linear regime
• Bayesian cosmic density field inference from redshift space dark matter maps
• Projected Three-Point Correlation Functions and Galaxy Bias
• Dark acoustic oscillations: Imprints on the matter power spectrum and the halo mass function
• Gravitational wave fossils in nonlinear regime: halo tidal bias and intrinsic alignments from gravitational wave separate universe simulations
• Non-Gaussian gravitational clustering field statistics
• Non-Gaussian Error in Galaxy Survey (Part 1)
• Cosmological Vlasov-Poisson equations for dark matter: Recent developments and connections to selected plasma problems
• An Effective Bias Expansion for 21 cm Cosmology in Redshift Space
• Gravitational instability via the Schrodinger equation
• Controlling intrinsic-shear alignment in three-point weak lensing statistics
• On spherical dust fluctuations: the exact vs. the perturbative approach
• Kinetic Field Theory: Effects of momentum correlations on the cosmic density-fluctuation power spectrum
• The Dark Ages' 21-cm Trispectrum
• N-point Statistics of Large-Scale Structure in the Zel'dovich Approximation
• Relativistic cosmological large scale structures at one-loop
• Neutrino Lump Fluid in Growing Neutrino Quintessence
• Euclid preparation. XLI. Galaxy power spectrum modelling in real space
• Cosmological Inference from Galaxy-Clustering Power Spectrum: Gaussianization and Covariance Decomposition
• The Anisotropic Line Correlation Function as a Probe of Anisotropies in Galaxy Surveys
• Multi-tracer power spectra and bispectra: Formalism
• Nonlinear modulation of the HI power spectrum on ultra-large scales. I
• Testing one-loop galaxy bias: cosmological constraints from the power spectrum
• The excursion set approach in non-Gaussian random fields
• A scale dependent bias on linear scales: the case for HI intensity mapping at z=1
• The Schrödinger-Poisson method for Large-Scale Structure
• A non-perturbative test of consistency relations and their violation
• Unequal time correlators and the Zeldovich approximation
• Toward Accurate Modeling of the Nonlinear Matter Bispectrum: Standard Perturbation Theory and Transients from Initial Conditions
• Cosmology with Phase Statistics: Parameter Forecasts and Detectability of BAO
• Quintessential Scale Dependence from Separate Universe Simulations
• Modelling non-dust fluids in cosmology
• C${}^3$-Cluster Clustering Cosmology II. First detection of the BAO peak in the three-point correlation function of galaxy clusters
• An Analytic Hybrid Halo + Perturbation Theory Model for Small-scale Correlators: Baryons, Halos, and Galaxies
• Divergence of Perturbation Theory in Large Scale Structures
• The nonlinear power spectrum in clustering quintessence cosmologies
• Vacuum Condensate Picture of Quantum Gravity
• A measurement of the mean central optical depth of galaxy clusters via the pairwise kinematic Sunyaev-Zel'dovich effect with SPT-3G and DES
• Frame dragging and Eulerian frames in General Relativity
• Initial conditions for cold dark matter particles and General Relativity
• A determination of dark matter bispectrum with a large set of N-body simulations
• Cosmology from clustering of Lyman-alpha galaxies: breaking non-gravitational Lyman-alpha radiative transfer degeneracies using the bispectrum
• Quadratic shape biases in three-dimensional halo intrinsic alignments
• Cosmology in Poincare gauge gravity with a pseudoscalar torsion
• HYMALAIA: A Hybrid Lagrangian Model for Intrinsic Alignments
• Determine the galaxy bias factors on large scales using bispectrum method
• Comparing cosmic web classifiers using information theory
• Modelling the matter bispectrum at small scales in modified gravity
• Fast and Accurate Non-Linear Predictions of Universes with Deep Learning
• Effects of the size of cosmological N-Body simulations on physical quantities - III: Skewness
• Renormalization of Lagrangian bias via spectral parameters
• On the equivalence between the effective cosmology and excursion set treatments of environment
• Higher-order Statistics of Weak Lensing Shear and Flexion
• The CMB lensing bi-spectrum as a probe of modified gravity theories
• Full-sky bispectrum in redshift space for 21cm intensity maps
• Perturbation theory with dispersion and higher cumulants: framework and linear theory
• Screening in perturbative approaches to LSS
• Imprints of Reionization in Galaxy Clustering
• Modal compression of the redshift-space galaxy bispectrum
• Cosmic Microwave Background--Weak Lensing Correlation: Analytical and Numerical Study of Non-linearity and Implications for Dark Energy
• Perturbation theory for the redshift-space matter power spectra after reconstruction
• Weak Lensing Effects on the Galaxy Three-Point Correlation Function
• The matter density PDF for modified gravity and dark energy with Large Deviations Theory
• A new method to measure galaxy bias by combining the density and weak lensing fields
• Modelling Non-Linear Effects of Dark Energy
• Impacts of biasing schemes in the one-loop integrated perturbation theory
• Multipoles of the relativistic galaxy bispectrum
• Oscillating Bispectra and Galaxy Clustering: A Novel Probe of Inflationary Physics with Large-Scale Structure
• Lifting Primordial Non-Gaussianity Above the Noise
• Optimal Transport Reconstruction of Baryon Acoustic Oscillations
• Perturbation theory for nonlinear halo power spectrum: the renormalized bias and halo bias
• The cosmic web connection to the dark matter halo distribution through gravity
• Finding closure: approximating Vlasov-Poisson using finitely generated cumulants
• Newton to Einstein - dust to dust
• Accurate Baryon Acoustic Oscillations reconstruction via semi-discrete optimal transport
• Lagrangian theory for cosmic structure formation with vorticity: Newtonian and post-Friedmann approximations
• The non-perturbative regime of cosmic structure formation
• Self-Similar Bumps and Wiggles: Isolating the Evolution of the BAO Peak with Power-law Initial Conditions
• Using Lagrangian perturbation theory for precision cosmology
• Statistics of biased tracers in variance-suppressed simulations
• Modeling of weak lensing statistics. I. Power spectrum and bispectrum
• The VIMOS Public Extragalactic Redshift Survey (VIPERS). Hierarchical scaling and biasing
• Resummed Kinetic Field Theory: general formalism and linear structure growth from Newtonian particle dynamics
• On the importance of nonlinear couplings in large-scale neutrino streams
• Squeezing $f_{\mathrm{NL}}$ out of the matter bispectrum with consistency relations
• The dark matter dispersion tensor in perturbation theory
• Constraints on ultra-slow-roll inflation from the third LIGO-Virgo observing run
• Cosmological Angular Trispectra and Non-Gaussian Covariance
• Renormalisation of linear halo bias in N-body simulations
• Lenses in the forest: cross-correlation of the Lyman-alpha flux with CMB lensing
• Cosmic Variance of the 21-cm Global Signal
• Finite volume effects for non-Gaussian multi-field inflationary models
• Beyond Kaiser bias: mildly non-linear two-point statistics of densities in distant spheres
• General relativistic effects in the galaxy bias at second order
• BAO scale inference from biased tracers using the EFT likelihood
• Lagrangian approach to super-sample effects on biased tracers at field level: galaxy density fields and intrinsic alignments
• Modeling the Marked Spectrum of Matter and Biased Tracers in Real- and Redshift-Space
• The Adaptive TreePM: An Adaptive Resolution Code for Cosmological N-body Simulations
• The VIMOS Public Extragalactic Redshift Survey (VIPERS): On the correct recovery of the count-in-cell probability distribution function
• Accuracy of analytical models of the large-scale matter distribution
• Optimal computation of anisotropic galaxy three point correlation function multipoles using 2DFFTLOG formalism
• Evolution of skewness and kurtosis of cosmic density fields
• Cosmological perturbations in f(G) gravity
• Marked correlation functions in perturbation theory
• Clustering of Local Extrema in Planck CMB maps
• The Poisson equation at second order in relativistic cosmology
• Two-loop power spectrum with full time- and scale-dependence and EFT corrections: impact of massive neutrinos and going beyond EdS
• Galilean invariant resummation schemes of cosmological perturbations
• Neutrino Mass Signatures in the Galaxy Bispectrum
• Evolution Equation for Non-linear Cosmological Perturbations
• Exploring the Redshift-Space Peculiar Velocity Field and its Power Spectrum
• Cross-correlation of CFHTLenS galaxy catalogue and Planck CMB lensing using the halo model prescription
• Large-Scale Tides in General Relativity
• Dynamical flows through Dark Matter Haloes II: one and two points statistics at the virial radius
• Weak lensing probe of cubic Galileon model
• The position-dependent matter density probability distribution function
• Transients from initial conditions based on Lagrangian perturbation theory in N-body simulations
• Cubic Derivative Interactions and Asymptotic Dynamics of the Galileon Vacuum
• Source-lens clustering and intrinsic-alignment bias of weak-lensing estimators
• Application of the iterative reconstruction to simulated galaxy fields
• Improving constraints on primordial non-Gaussianity using neural network based reconstruction
• Normalization of the Matter Power Spectrum via Higher-Order Angular Correlations of Luminous Red Galaxies
• Cosmological Probes of Structure Growth and Tests of Gravity
• Intensity mapping of the 21cm emission: lensing
• Reconstruction of f(R) models with Scale-invariant Power Spectrum
• The unequal-time matter power spectrum: impact on weak lensing observables
• Eulerian and Lagrangian propagators for the adhesion model (Burgers dynamics)
• fkPT: Constraining scale-dependent modified gravity with the full-shape galaxy power spectrum
• Redshift-space correlation functions in large galaxy cluster surveys
• Degeneracy between CCDM and $\Lambda$CDM cosmologies
• Robustness of the covariance matrix for galaxy clustering measurements
• The VIMOS Public Extragalactic Redshift Survey (VIPERS). The matter density and baryon fraction from the galaxy power spectrum at redshift $0.6<z<1.1$
• On Soft Limits of Large-Scale Structure Correlation Functions
• Lagrangian space consistency relation for large scale structure
• Tomography and Weak lensing Statistics
• Neutrino mass tension or suppressed growth rate of matter perturbations?
• Volume Statistics as a Probe of Large-Scale Structure
• A Simple Analytic Treatment of Linear Growth of Structure with Baryon Acoustic Oscillations
• Evolution of dark matter velocity dispersion
• Variations of cosmic large-scale structure covariance matrices across parameter space
• The clustering of baryonic matter. II: halo model and hydrodynamic simulations
• The Lyman-$\alpha$ power spectrum - CMB lensing convergence cross-correlation
• The Integrated Bispectrum in Modified Gravity Theories
• The VIMOS VLT Deep Survey: Testing the gravitational instability paradigm at z ~ 1
• Determination of the abundance of cosmic matter via the cell count moments of the galaxy distribution (1)
• Duel of cosmological screening lengths
• From 100 kpc to 10 Gpc: Dark Matter self-interactions before and after DESI
• Simple expressions for second order density perturbations in standard cosmology
• Cosmic Web Dissection in Fuzzy Dark Matter Cosmologies
• Perturbation theory of LSS in the $\Lambda$CDM Universe: exact time evolution and the two-loop power spectrum
• Matter bispectrum of large-scale structure with Gaussian and non-Gaussian initial conditions: Halo models, perturbation theory, and a three-shape model
• Reconstruction of halo power spectrum from redshift-space galaxy distribution: cylinder-grouping method and halo exclusion effect
• Constraining Primordial Non-Gaussianity with Moments of the Large Scale Density Field
• Galaxy Three-Point Correlation Functions and Halo/Subhalo Models
• Extending the domain of validity of the Lagrangian approximation
• Optical depth to reionization from perturbative 21cm clustering
• Simulated evolution of the dark matter large-scale structure
• Phenomenology of BAO evolution from Lagrangian to Eulerian Space
• CMB lensing bi-spectrum: assessing analytical predictions against full-sky lensing simulations
• Using kinetic theory to examine a self-gravitating system composed of baryons and cold dark matter
• Modelling the next-to-leading order matter three-point correlation function using FFTLog
• Fisher matrix for the one-loop galaxy power spectrum: measuring expansion and growth rates without assuming a cosmological model
• Field-Based Physical Inference From Peculiar Velocity Tracers
• Differentiable Predictions for Large Scale Structure with SHAMNet
• Grid-based calculations of redshift-space matter fluctuations from perturbation theory: UV sensitivity and convergence at the field level
• Indra: a Public Computationally Accessible Suite of Cosmological $N$-body Simulations
• Post-Born corrections to the one-point statistics of (CMB) lensing convergence obtained via large deviation theory
• Kinetic Field Theory: Exact free evolution of Gaussian phase-space correlations
• Using galaxy pairs to investigate the three-point correlation function in the squeezed limit
• Imprint of non-linear effects on HI intensity mapping on large scales
• Galaxy Clustering in 3D and Modified Gravity Theories
• Phase Space dynamics of triaxial collapse: Joint density-velocity evolution
• Nonlinear effects of dark energy clustering beyond the acoustic scales
• Simulating the Anisotropic Clustering of Luminous Red Galaxies with Subhalos: A Direct Confrontation with Observation and Cosmological Implications
• Cosmic Microwave Background Bispectrum from the Lensing--Rees-Sciama Correlation Reexamined: Effects of Non-linear Matter Clustering
• Field Theory of the Correlation Function of Mass Density Fluctuations for Self-Gravitating Systems
• A revised density split statistic model for general filters
• Testing the equivalence principle on cosmological scales using the odd multipoles of galaxy cross-power spectrum and bispectrum
• Scalar field dark matter in hybrid approach
• A Robust BAO Extractor
• Suppressing variance in 21-cm signal simulations during reionization
• A Coarse-Grained Field Theory for Density Fluctuations and Correlation Functions of Galactic Objects
• A gauge-invariant approach to interactions in the dark sector
• A new framework for numerical simulations of structure formation
• The Morphology of the Thermal Sunyaev-Zel'dovich Sky
• Euclid preparation. Modelling spectroscopic clustering on mildly nonlinear scales in beyond-$\Lambda$CDM models
• Planting a Lyman alpha forest on AbacusSummit
• The ACCEL2 Project: Precision Measurements of EFT Parameters and BAO Peak Shifts for the Lyman-$\alpha$ Forest
• Density fields and halo mass functions in the Geometrical Adhesion toy Model
• Conditional Cumulants in Weakly Non-linear Regime
• A theoretical estimate of intrinsic ellipticity bispectra induced by angular momenta alignments
• Cosmological Density Perturbations with a Scale-Dependent Newton's G
• Merging and fragmentation in the Burgers dynamics
• Second-order matter fluctuations via higher-order galaxy correlators
• The Monge-Ampère-Kantorovich approach to reconstruction in cosmology
• Perfectly parallel cosmological simulations using spatial comoving Lagrangian acceleration
• Kriging Interpolating Cosmic Velocity Field
• Toward an Improved Analytical Description of Lagrangian Bias
• A joint 2- and 3-point clustering analysis of the VIPERS PDR2 catalogue at z~1: breaking the degeneracy of cosmological parameters
• An analytic halo approach to the bispectrum of galaxies in redshift space
• Baryon oscillations in galaxy and matter power-spectrum covariance matrices
• Statistical Properties of Thermal Sunyaev-Zel'dovich Maps
• Wide-angle effects in the galaxy bispectrum
• KiDS+VIKING+GAMA: Halo occupation distributions and correlations of satellite numbers with a new halo model of the galaxy-matter bispectrum for galaxy-galaxy-galaxy lensing
• Consistency Relations in Effective Field Theory
• Tackling non-linearities with the effective field theory of dark energy and modified gravity
• The Shape Dependence of Vainshtein Screening in the Cosmic Matter Bispectrum
• Assessing non-linear models for galaxy clustering II: model validation and forecasts for Stage IV surveys
• A Relativistic view on large scale N-body simulations
• Structure formation in an anisotropic universe: Eulerian perturbation theory
• Cosmic topology. Part IIa. Eigenmodes, correlation matrices, and detectability of orientable Euclidean manifolds
• Higher multipoles of the galaxy bispectrum in redshift space
• Non-Gaussian CMB and LSS statistics beyond polyspectra
• Super-sample tidal modes on the celestial sphere
• DISCO-DJ I: a differentiable Einstein-Boltzmann solver for cosmology
• The role of shell crossing on the existence and stability of trapped matter shells in spherical inhomogeneous Λ-CDM models
• The Gravity of the Classical Klein-Gordon field
• Integrated perturbation theory for cosmological tensor fields. I. Basic formulation
• Quasi-spherical collapse of matter in $\Lambda$CDM
• Ellipsoidal collapse and the redshift space probability distribution function of dark matter
• Validating the methodology for constraining the linear growth rate from clustering anisotropies
• The statistics of peaks of weakly non-Gaussian random fields: Effects of bispectrum in two- and three-dimensions
• The halo squeezed-limit bispectrum with primordial non-Gaussianity: a power spectrum response approach
• Exact Analytic Solution for Non-Linear Density Fluctuation in a LCDM Universe
• Weak Lensing Skew-Spectrum
• Nonlinear Density Fluctuation Field Theory for Large Scale Structure
• Astrophysical Bose-Einstein Condensates and Superradiance
• Large scale structures in the Early SDSS: Comparison of the North and South Galactic strips
• Interferometric HI intensity mapping: perturbation theory predictions and foreground removal effects
• The adhesion model as a field theory for cosmological clustering
• Consistency relations for large scale structures with primordial non-Gaussianities
• Bayesian Control Variates for optimal covariance estimation with pairs of simulations and surrogates
• Revisiting Vainshtein Screening for fast N-body simulations
• Three-point intrinsic alignments of dark matter halos in the IllustrisTNG simulation
• Detecting baryon acoustic oscillations by 3d weak lensing
• Constraints on dark matter self-interaction from galactic core size
• Large Scale Structure Reconstruction with Short-Wavelength Modes
• Estimating the Integrated Bispectrum from Weak Lensing Maps
• Asymptotic expansions for the Large Scale Structure
• Fast Correlation Function Calculator -- A high-performance pair counting toolkit
• Eye of the Tyger: early-time resonances and singularities in the inviscid Burgers equation
• On the primordial information available to galaxy redshift surveys
• Relativistic Effects on Galaxy Redshift Samples due to Target Selection
• Imitating intrinsic alignments: A bias to the CMB lensing-galaxy shape cross-correlation power spectrum induced by the large-scale structure bispectrum
• Two is better than one: joint statistics of density and velocity in concentric spheres as a cosmological probe
• Modeling iterative reconstruction and displacement field in the large scale structure
• Impact of tidal environment on galaxy clustering in GAMA
• Cosmological Tests of Gravity: A Future Perspective
• Generalized statistical models of voids and hierarchical structure in cosmology
• Integrated perturbation theory for cosmological tensor fields. III. Projection effects
• Kinetic theory and classical limit for real scalar quantum field in curved space-time
• Halo Model Analysis of Cluster Statistics
• A constructive approach to regularity of Lagrangian trajectories for incompressible Euler flow in a bounded domain
• Cosmological Perturbation Theory for streams of relativistic particles
• The bispectrum of matter perturbations from cosmic strings
• Towards the physical vacuum of cosmic inflation
• Matrix Formalism of Excursion Set Theory: A new approach to statistics of dark matter halo counting
• On the Fast Random Sampling and Other Properties of the Three Point Correlation Function in Galaxy Surveys
• Morphology of Weak Lensing Convergence Maps
• A first comparison of Kinetic Field Theory with Eulerian Standard Perturbation Theory
• Halo Counts-in-cells for Cosmological Models with Different Dark Energy
• The continuous wavelet derived by smoothing function and its application in cosmology
• Zero average values of cosmological perturbations as an indispensable condition for the theory and simulations
• A Study on the Baryon Acoustic Oscillation with Topological Data Analysis
• Gravitational collapse in an expanding background and the role of substructure II: Excess power at small scales and its effect of collapse of structures at larger scales
• A Modified TreePM Code
• Damping of the baryon acoustic oscillations in the matter power spectrum as a probe of the growth factor
• Neutrino winds on the sky
• Quasi-linear regime and rare-event tails of decaying Burgers turbulence
• The pairwise velocity probability density function in models with local primordial non-Gaussianity
• Non-linear mode coupling and the growth of perturbations in LCDM
• Parameter estimation biases due to contributions from the Rees-Sciama effect to the integrated Sachs-Wolfe spectrum
• An exact Lagrangian integral for the Newtonian gravitational field strength
• A weak lensing view on primordial non-Gaussianities
• Got plenty of nothing: cosmic voids as a probe of particle dark matter
• Exploring neutrino interactions in light of present and upcoming galaxy surveys
• Towards unveiling the large-scale nature of gravity with the wavelet scattering transform
• Cross-correlating Sunyaev-Zel'dovich and Weak Lensing Maps
• Quantifying the redshift space distortion of the bispectrum III : Detection prospects of the multipole moments
• What can the spatial distribution of galaxy clusters tell about their scaling relations?
• Scale Dependence of the Halo Bias in General Local-Type Non-Gaussian Models I: Analytical Predictions and Consistency Relations
• Improving precision and accuracy in cosmology with model-independent spectrum and bispectrum
• Wave-mechanics and the adhesion approximation
• Simple lessons from complex learning: what a neural network model learns about cosmic structure formation
• First and second order cosmological perturbations in light mass Galileon models
• The galaxy bias at second order in general relativity with Non-Gaussian initial conditions
• Cell Count Moments in the Halo Model
• An Application of Wiener Hermite Expansion to Non-linear Evolution of Dark Matter
• Modeling of weak lensing statistics. II. Configuration-space statistics
• Constraints on Running of Non-Gaussianity from Large Scale Structure Probes
• Angular power spectra of anisotropic stochastic gravitational wave background: developing statistical methods and analyzing data from ground-based detectors
• The two-loop power spectrum in redshift space
• KiDS-Legacy: Covariance validation and the unified OneCovariance framework for projected large-scale structure observables
• The Renormalization Group for Large-Scale Structure: Primordial non-Gaussianities
• fNL - gNL mixing in the matter density field at higher orders
• Third-order cosmological perturbations of zero-pressure multi-component fluids: Pure general relativistic nonlinear effects
• Integrated perturbation theory for cosmological tensor fields. II. Loop corrections
• Cosmological constraints from the redshift dependence of the volume effect using the galaxy 2-point correlation function across the line-of-sight
• Relativistic Euler Equations in cosmologies with non-linear structures
• The nonlinear redshift space probability distribution function in models with local primordial non-Gaussianity
• First test of the consistency relation for the large-scale structure using the anisotropic three-point correlation function of BOSS DR12 galaxies (An explanatory video is available at https://youtu.be/Zi36ooLPhss.)
• Lagrangian theory of structure formation in relativistic cosmology. V. Irrotational fluids
• Power spectrum in the presence of large-scale overdensity and tidal fields: breaking azimuthal symmetry
• Constraining primordial and gravitational mode coupling with the position-dependent bispectrum of the large-scale structure
• Non-Gaussian error bars in galaxy surveys -- II
• One-point statistics of the Lagrangian displacement field
• Non-linear matter bispectrum in general relativity
• Coarse-grained cosmological perturbation theory: stirring up the dust model
• One-point probability distribution function from spherical collapse: Early Dark Energy (EDE) vs. $\Lambda$CDM
• Exact Third-Order Density Perturbation and One-Loop Power Spectrum in General Dark Energy Models
• Constraining primordial non-Gaussianity with cosmological weak lensing: shear and flexion
• Void Probability Function of Simulated Surveys of high-redshift Lyman-Alpha Emitters
• Redshift-space equal-time angular-averaged consistency relations of the gravitational dynamics
• CMB power spectrum in the emergent universe with k-essence
• The Effective Field Theory and Perturbative Analysis for Log-Density Fields
• Imprints of dynamical dark energy on weak-lensing measurements
• The non-linear evolution of bispectrum from the scale-free N-body simulation
• Multi-Scale Perturbation Theory I: Methodology and Leading-Order Bispectrum Corrections in the Matter-Dominated Era
• Large-scale structure in superfluid Chaplygin gas cosmology
• The shape distribution of superclusters in SDSS DR 12
• Weak Lensing Trispectrum and Kurt-Spectra
• A universal bound on the duration of a kination era
• Nonlinear Behavior of Baryon Acoustic Oscillations in Redshift Space from the Zel'dovich Approximation
• Nonlinear cosmological power spectra in Einstein's gravity
• The halo bispectrum as a sensitive probe of massive neutrinos and baryon physics
• Kinetic Field Theory for Cosmic Structure Formation
• Renormalizing a Viscous Fluid Model for Large Scale Structure Formation
• Nonlinear stochastic growth rates and redshift space distortions
• Probing dark energy using convergence power spectrum and bi-spectrum
• Evolution of intrinsic ellipticity correlations due to peculiar motion
• Hitting the mark: Optimising Marked Power Spectra for Cosmology
• The halo 3-point correlation function: a methodological analysis
• Probing redshift-space distortions with phase correlations
• BullFrog: Multi-step perturbation theory as a time integrator for cosmological simulations
• GEO-FPT: a model of the galaxy bispectrum at mildly non-linear scales
• Gravitational collapse in an expanding background and the role of substructure I: Planar collapse
• de Sitter symmetries and inflationary correlators in parity violating scalar-vector models
• Fast estimation of aperture-mass statistics I: aperture mass variance and an application to the CFHTLenS data
• The copula of the cosmological matter density field is non-Gaussian
• Cosmological post-Newtonian equations from nonlinear perturbation theory
• Apparent parity violation in the observed galaxy trispectrum
• Measuring the Galaxy-Galaxy-Mass Three-point Correlation Function with Weak Gravitational Lensing
• Non-linear Structure Formation for Dark Energy Models with a Steep Equation of State
• BAO Extractor: bias and redshift space effects
• The Quest for the Inflationary Spectral Runnings in the Presence of Systematic Errors
• Influence of the local Universe on weak gravitational lensing surveys
• APPLIED COSMOGRAPHY: A Pedagogical Review
• Field-theoretic approach to large-scale structure formation
• Constraining the growth rate of structure with phase correlations
• Second-order peculiar velocity field as a novel probe of scalar-tensor theories
• Perturbation Theory Remixed: Improved Nonlinearity Modeling beyond Standard Perturbation Theory
• Characteristic Functions for Cosmological Cross-Correlations
• Renormalization group and UV completion of cosmological perturbations: Gravitational collapse as a critical phenomenon
• Triumvirate: A Python/C++ package for three-point clustering measurements
• Impact of a Warm Dark Matter late-time velocity dispersion on large-scale structures
• A theoretical view of the T-web statistical description of the cosmic web
• Integrated perturbation theory for cosmological tensor fields. IV. Full-sky formulation
• Keeping It Real: Revisiting a Real-Space Approach to Running Ensembles of Cosmological N-body Simulations
• Probing vector chirality in the early Universe
• Reducing nuisance prior sensitivity via non-linear reparameterization, with application to EFT analyses of large-scale structure
• On general-relativistic Lagrangian perturbation theory and its non-perturbative generalization
• Evidence of Turbulence-like Universality on the Formation of Galaxy-sized Dark Matter Haloes
• Fast Calculation of Nonlinear Redshift-space Galaxy Power Spectrum Including Selection Bias
• Probing inflation with CMB polarization : weak lensing effect on the covariance of CMB spectra
• Three- and two-point spatial correlations of IGM at $z\sim 2$: Cloud based analysis using simulations
• Beyond the Lognormal Approximation: a General Simulation Scheme
• Perturbative Gaussianizing transforms for cosmological fields
• Covariance of Weak Lensing Observables
• The primordial non-Gaussianity of local type (f_NL) in the WMAP 5-year data: the length distribution of CMB skeleton
• Scalar-Induced Gravitational Waves in a $\Lambda$CDM Cosmology
• The dark matter bispectrum from effective viscosity and one-particle irreducible vertices
• Map-level baryonification: unified treatment of weak lensing two-point and higher-order statistics
• Resummed Kinetic Field Theory: Using Mesoscopic Particle Hydrodynamics to Describe Baryonic Matter in a Cosmological Framework
• Triple-Spherical Bessel Function Integrals with Exponential and Gaussian Damping: Towards an Analytic N-Point Correlation Function Covariance Model
• Sensitivity of Cosmological Parameter Estimation to Nonlinear Prescription from Galaxy Clustering
• The effect of finite halo size on the clustering of neutral hydrogen
• A Relativistic Interpretation of Bias in Newtonian Simulations
• Probing the Anisotropy and Non-Gaussianity in the Redshift Space through the Conditional Moments of the First Derivative
• Linear theory and velocity correlations of clusters
• Halo Profile Evolution and Velocity Bias
• Power spectrum response of large-scale structure in 1D and in 3D: tests of prescriptions for post-collapse dynamics
• Non-linear Cosmological Perturbations for Coupled Dark Energy
• Higher moments of primordial non-Gaussianity and N-body simulations
• CMB power spectrum for emergent scenario and slow expansion in scalar-tensor theory of gravity
• On Observables in a Dark Matter-Clustering Quintessence System
• One-loop power spectrum corrections in interacting dark energy cosmologies
• DESIVAST: A Catalog of Low-Redshift Voids using Data from the DESI DR1 Bright Galaxy Survey
• Probing the Neutrino Mass through the Cross Correlation between the Rees-Sciama Effect and Weak Lensing
• Cosmological inference including massive neutrinos from the matter power spectrum: biases induced by uncertainties in the covariance matrix
• DESI Mock Challenge: Constructing DESI galaxy catalogues based on FastPM simulations
• Gravitational Collapse in an Expanding Universe: Scaling Relations for Two-Dimensional Collapse Revisited
• Transverse velocities and matter gradient correlations: a new signal and a new challenge to moving-lens analyses
• Topology of Reionisation times: concepts, measurements and comparisons to gaussian random field predictions
• Probing the cosmic web in Ly$\alpha$ emission over large scales: an Intensity Mapping forecast for DECaLS/BASS and DESI
• Cosmological constraints from the EFT power spectrum and tree-level bispectrum of 21cm intensity maps
• Covariance matrices for variance-suppressed simulations
• A study of relative velocity statistics in Lagrangian perturbation theory with PINOCCHIO
• Nonlinear power spectrum in clustering and smooth dark energy models beyond the BAO scale
• Einasto profile as the halo model solution coupled to the depletion radius
• Impact of our local environment on cosmological statistics
• Assessing theoretical uncertainties for cosmological constraints from weak lensing surveys
• Cosmological Evolution in Bimetric Gravity: Observational Constraints and LSS Signatures
• Exact Results for Propagators in the Geometrical Adhesion Model
• Metal Enrichment and Reionization Constraints on Early Star Formation
• Impact of lensing magnification on the analysis of galaxy clustering in redshift space
• High-order 2MASS galaxy correlation functions: Probing the primordial density field and the linearity of galaxy bias
• COmoving Computer Acceleration (COCA): $N$-body simulations in an emulated frame of reference
• An Analytically Tractable Marked Power Spectrum
• Nonlinear evolution of density and flow perturbations on a Bjorken background
• Kinetic Field Theory: Perturbation theory beyond first order
• Efficient implementation of the Time Renormalization Group
• The Beylkin-Cramer Summation Rule and A New Fast Algorithm of Cosmic Statistics for Large Data Sets
• Kinetic Field Theory applied to Vector-Tensor Gravity
• Impact of cosmological signatures in two-point statistics beyond the linear regime
• Cosmological signatures of a Rapid Diluted Energy Density
• Constraints on primordial non-Gaussianity using multitracer technique for skew spectrum
• Optimizing the Evolution of Perturbations in the $\Lambda$CDM Universe
• The cumulant generating function as a novel observable to cumulate weak lensing information
• The nonlinear field equation of the three-point correlation function of galaxies
• Relativistic perturbations in $\Lambda$CDM: Eulerian & Lagrangian approaches
• Holographic inflation and holographic dark energy from entropy of the anti-de Sitter black hole
• Dynamics of pairwise motions in the fully non-linear regime in LCDM and Modified Gravity cosmologies
• Dark matter vorticity and velocity dispersion from truncated Dyson$\unicode{x2013}$Schwinger equations
• Revisiting coupled CDM-massive neutrino perturbations in diverse cosmological backgrounds
• A Model for the Redshift-Space Galaxy 4-Point Correlation Function
• The galaxy power spectrum on the lightcone: deep, wide-angle redshift surveys and the turnover scale
• Continuous Filament Network of the Local Universe
• Spawning and merging of Fourier modes and phase coupling in cosmological density bispectrum
• Constraining Ultralight Axions with Galaxy Surveys
• A halo model of extragalactic contamination to CMB lensing, delensing, and cross-correlations
• Sample variance in N--body simulations and impact on tomographic shear predictions
• Position-Dependent Correlation Function of Weak Lensing Convergence
• Higher-Order Spectra of Weak Lensing Convergence Maps in Parameterized Theories of Modified Gravity
• Measurement of redshift-space two- and three-point correlation of Ly$\alpha$ absorbers at $1.7<z<3.5$: Implications on evolution of the physical properties of IGM
• Lagrangian perturbations theory : Third-order solution for general dark energy models
• Studying Interstellar Turbulence Driving Scales using the Bispectrum
• Reconstructing the Long-wavelength Matter Density Fluctuation Modes from the Scalar-Type Clustering Fossils
• Transients from initial conditions based on Lagrangian perturbation theory in $N$-body simulations II: the effect of the transverse mode
• Including relativistic and primordial Non-Gaussianity contributions in cosmological simulations by modifying the initial condition
• Cosmological Perturbation Theory as a Tool for Estimating Box-Scale Effects in N-body Simulations
• Non-Linearity-Free prediction of the growth-rate $f{\sigma }_8$ using Convolutional Neural Networks
• Fourth-order perturbative equations in Lagrangian perturbation theory for a cosmological dust fluid
• Numerical study of the cosmological velocity field as a function of density
• Fourier imaging of non-linear structure formation
• Relativistic matter bispectrum of cosmic structures on the light cone
• The gravitational force field of proto-pancakes
• Starting Cosmological Simulations from the Big Bang
• Determining accurate measurements of the growth rate from the galaxy correlation function in simulations
• Perturbative interaction approach to cosmological structure formation
• Galaxy and halo angular clustering in LCDM and Modified Gravity cosmologies
• Fast and accurate collapse-time predictions for collisionless matter
• How do uncertainties in galaxy formation physics impact field-level galaxy bias?
• Resummed Kinetic Field Theory: a model of coupled baryonic and dark matter
• Infrared divergence of pure Einstein gravity contributions to cosmological density power spectrum
• Massive neutrinos in nonlinear large scale structure: A consistent perturbation theory
• Position-dependent Voronoi probability distribution functions for matter and halos
• Relativistic second-order initial conditions for simulations of large-scale structure
• A spherical hydrodynamical model of cosmic voids in ΛCDM and beyond
• Relativistic and non-Gaussianity contributions to the one-loop power spectrum
• Testing for gravitational preferred directions with galaxy and lensing surveys
• Projected two- and three-point statistics: Forecasts and mitigation of non-linear RSDs
• A model of the anisotropic correlation function xi(rp, pi) in redshift space including redshift errors
• Cosmological perturbation theory for large scale structure in phase space
• Phenomenological power spectrum models for H$\alpha$ emission line galaxies from the Nancy Grace Roman Space Telescope
• The ergodicity bias in the observed galaxy distribution
• Reconstructing HI power spectrum with minimal parameters using the dark matter distribution beyond halos
• Neural style transfer of weak lensing mass maps
• Cosmological Parameters, Dark Energy and Large Scale Structure
• Explicit computation of shear three-point correlation functions: the one-halo model case
• Scale-dependent halo bias and the squeezed limit bispectrum in the presence of radiation
• Cosmological perturbation theory using generalized Einstein de Sitter cosmologies
• A model-independent measurement of the expansion and growth rates from BOSS using the FreePower method
• Testing the assumptions of the Effective Field Theory of Large-Scale Structure
• Analytical Equation of Three-point Correlation Function of Galaxies: to Third Order of Density Perturbation
• Generating Approximate Halo Catalogs for Blind Challenges in Precision Cosmology
• Approximate methods for the generation of dark matter halo catalogs in the age of precision cosmology
• Symmetries, Invariants and Generating Functions: Higher-order Statistics of Biased Tracers
• The Effective Field Theory of Large Scale Structure for Mixed Dark Matter Scenarios
• Clustering of K-band selected local galaxies
• Updated neutrino mass constraints from galaxy clustering and CMB lensing-galaxy cross-correlation measurements
• Skewness consistency relation in large-scale structure and test of gravity theory
• The Compressed 3D Lyman-Alpha Forest Bispectrum
• Numerical investigation of non-Gaussianities in the phase and modulus of density Fourier modes
• The RSD Sorting Hat: Unmixing Radial Scales in Projection
• Neural Network Reconstruction of Non-Gaussian Initial Conditions from Dark Matter Halos
• Influence of baryons on spatial distribution of matter: higher order correlation functions
• Lagrangian Perturbation Theory : Exact One-Loop Power Spectrum in General Dark Energy Models
• Counts-in-Cells of subhaloes in the IllustrisTNG simulations: the role of baryonic physics
• Evolution of the early universe in Einstein-Cartan theory
• On counterterms in cosmological perturbation theory
• Bye-bye, Local-in-matter-density Bias: The Statistics of the Halo Field Are Poorly Determined by the Local Mass Density
• Gaussian Lagrangian Galaxy Bias
• Probabilistic Lagrangian bias estimators and the cumulant bias expansion
• The Statistics of Cosmological Lyman-alpha Absorption
• Squeezing information from radio surveys to probe the primordial Universe
• One-point Statistics in various cosmic environments in the presence of massive neutrinos
• Estimators for the cross-pairwise kSZ effect: forecasts for the dark energy and modified gravity parameters with Simons Observatory and CMB-S4
• Optimal transport by omni-potential flow and cosmological reconstruction
• Large-k Limit of Multi-Point Propagators in the RG Formalism
• Bending the web: exploring the impact of modified gravity on the density field and halo properties within the cosmic web
• Pair Counting without Binning -- A New Approach to Correlation Functions in Clustering Statistics
• Impact of Redshift Space Distortion on Persistent Homology of cosmic matter density field
• Degrees of Freedom of New General Relativity I: Type 2, Type 3, Type 5, and Type 8
• An Optimally Weighted Estimator of the Linear Power Spectrum Disentangling the Growth of Density Perturbations Across Galaxy Surveys
• Fast Generation of Weak Lensing Maps in Modified Gravity with COLA
• Cosmic Strings-induced CMB anisotropies in light of Weighted Morphology
• The frozen vanilla model: Exploring dark sector interactions with delta effective theories
• Redshift-space galaxy bispectrum in presence of massive neutrinos: A multipole expansion approach for Euclid
• Non-Gaussian statistics in galaxy weak lensing: compressed three-point correlations and cosmological forecasts
• Impact of redshift distribution uncertainties on Lyman-break galaxy cosmological parameter inference
• Multiscale Turbulence Synthesis: Validation in 2D Hydrodynamics
• Approximating Density Probability Distribution Functions Across Cosmologies
• The imprints of massive neutrinos on the three-point correlation function of large-scale structures
• Cosmological functional renormalisation group, extended Galilean invariance and the sweeping effect
• The reach of next-to-leading-order perturbation theory for the matter bispectrum
• Evolution of Cosmic Voids in the Schrodinger-Poisson Formalism
• Cosmological Implications of a Neutrino Mass Detection
• Cosmological consequences of intrinsic alignments super-sample covariance
• Statistical Decoupling of Lagrangian Fluid Parcel in Newtonian Cosmology
• Projection of the gravitational dynamics on a subspace of probability distributions: curl-free Gaussian ansatz
• SOMBI: Bayesian identification of parameter relations in unstructured cosmological data
• Estimating power spectrum of discrete cosmic momentum field with fast Fourier transform
• Multi-Scale Perturbation Theory II: Solutions and Leading-Order Bispectrum in the $\Lambda$CDM Universe
• Theory and Experiments for Disordered Elastic Manifolds, Depinning, Avalanches, and Sandpiles
• Probability Density Functionals in Perturbation Theory within the QFT in-in Formalism
• Baryonic effects in the Effective Field Theory of Large-Scale Structure and an analytic recipe for lensing in CMB-S4
• Introduction to Higher Order Spatial Statistics in Cosmology
• Towards a Gravity Dual for the Large Scale Structure of the Universe
• Speeding up the detectability of the harmonic-space galaxy bispectrum
• Lyman-alpha power spectrum as a probe of modified gravity
• Super-horizon second-order perturbations for cosmological random fluctuations and the Hubble-constant problem
• The Effective Field Theory of Large Scale Structures of a Fuzzy Dark Matter Universe
• Perturbation theory challenge for cosmological parameters estimation II.: Matter power spectrum in redshift space
• A theoretical approach to density-split clustering
• Preliminary clustering properties of the DESI BGS bright targets using DR9 Legacy Imaging Surveys
• Kinetic field theory: generic effects of alternative gravity theories on non-linear cosmic density-fluctuations
• Effect of peculiar velocities of inhomogeneities on the shape of gravitational potential in spatially curved universe
• The Odd-Parity Part of the Observed Galaxy Trispectrum
• Induced cosmological anisotropy by a gauge-gravity interaction
• Transients from Initial Conditions Based on Lagrangian Perturbation Theory in $N$-body Simulations III: The Case of GADGET-2 Code
• A semi-analytic estimate for the effective sound speed counterterm in the EFTofLSS
• Cold Collapse and Bounce of an FLRW Cloud
• Lagrangian-space Gaussian ansatz for the matter redshift-space power spectrum and correlation function
• Non-Gaussianity of the density distribution in accelerating universes II:N-body simulations
• Modeling and measuring the anisotropic halo 3-point correlation function: a coordinated study
• Implementing spectra response function approaches for fast calculation of power spectra and bispectra
• Precision calculation of the EFT likelihood with primordial non-Gaussianities
• Perturbation Theory Remixed II: Improved Modeling of Nonlinear Bispectrum
• Multipoles of the galaxy bispectrum on a light cone: wide-separation and relativistic corrections
• Astrophysical and cosmological problems of invisible mass and dark energy in the Universe
• The Effective Fluid Approach to Cosmological Nonlinearities: Applications to Preheating
• The pairwise and cross-pairwise y-type polarised kinetic Sunyaev Zeldovich effect from transverse velocity of galaxy clusters
• Weak lensing deflection of three-point correlation functions
• Quasilinear observables in dark energy cosmologies
• Simulation budgeting for hybrid effective field theories
• Lensing contribution to the 21cm intensity bispectrum
• Parity Violation in Galaxy Shapes: Primordial Non-Gaussianity
• The Large Scale Structure Bootstrap: perturbation theory and bias expansion from symmetries
• Cosmic structure from the path integral of classical mechanics and its comparison to standard perturbation theory
• Using strong gravitational lensing to probe the post reionization \HI power spectrum
• Effective description of dark matter as a viscous fluid
• Informational corrections to the early-Universe radiation sector: CET Omega, WIMP freeze-out, and implications for a possible 20 GeV gamma-ray excess
• A New Estimator for Phase Statistics
• Cross bispectra and trispectra of the non-linear integrated Sachs-Wolfe effect and the tracer galaxy density field
• O-V-S-Z and friends: Non-Gaussianity from inhomogeneous reionization
• On the symmetry properties of the PT kernels and recurrence relations
• Mass density vs. energy density at cosmological scales
• Effects of the size of cosmological N-body simulations on physical quantities II-. Halo formation and destruction rate
• A direct detection method of galaxy intrinsic ellipticity-gravitational shear correlation in non-linear regimes using self-calibration
• Suppression of matter density growth at scales exceeding the cosmic screening length
• Constant-roll inflation and primordial black holes within Barrow entropic framework
• Effects of dynamical friction on perturbations for evolving dark energy
• Dark matter halo dynamics in 2D Vlasov Simulations: a self-similar approach
• Fullshape power spectrum for the Symmetron modified gravity model
• Kinetic field theory: effects of modified gravity theories with screening mechanisms on non-linear cosmic density fluctuations
• Redshift-space distortion from dynamical dark energy with time-dependent Lagrangian perturbation theory
• One-dimensional model of cosmological perturbations: direct integration in the Fourier space
• Constraining effective neutrino species with bispectrum of large scale structures
• Growth rate measurements from a joint analysis of the large-scale galaxy clustering in Fourier and configuration space
• Bridging Simulations and EFT: A Hybrid Model of the Lyman-Alpha Forest Field
• A Non-parametric Method for the Inference of Halo Occupation Distributions
• About One-point Statistics of the Ratio of Two Fourier-transformed Cosmic Fields and an Application
• Optimizing Foreground Modelling for Global 21cm Cosmology with GPU-Accelerated Nested Sampling
• Sound Mode and Scale-Dependent Growth in Two-Fluid Dynamical Dark Energy
• Probing the large-scale structure with 21cm-galaxy cross-bispectrum: Estimates from simulations and forecasts for upcoming cosmological surveys
• Probing gravity beyond general relativity with bispectrum multipoles of cosmological tracers: I. Theoretical Foundations
• Cosmology from LOFAR Two-metre Sky Survey Data Release 2: Counts-in-Cells Statistics
• Phase-space perturbation theory for cosmic large-scale structure
• Skew-spectra: a generalization to spin-$s$
• Impact of scale-dependent bias and nonlinear evolution on the ISW
• On Weak Lensing Response Functions
• Quantifying Weighted Morphological Content of Large-Scale Structures via Simulation-Based Inference
• Explosions in the Empty: A Survey of Transients in Local Void Galaxies
• On the Statistical Evolution of the Large-scale Structure and the Effective Dynamics
• Hybrid $P_{\ell }(k)$: general, unified, non-linear matter power spectrum in redshift space
• $\text{SBi3PCF:}$ Simulation-based inference with the integrated 3PCF
• Interacting dark energy from redshift-space galaxy clustering
• Streaming Velocity Effects on the Post-reionization 21 cm Baryon Acoustic Oscillation Signal
• Post-collapse Lagrangian perturbation theory in three dimensions
• Towards an application of fourth-order shear statistics I. The information content of $⟨M_{\mathrm{ap}}^4⟩$
• The Effects of Gravitational Slip on the Higher-Order Moments of the Matter Distribution
• Analytical Template for the 4-Point Correlation Function Covariance Beyond the Gaussian Random Field $\mathrm{II}$: 1-Loop Corrections with Third-Order Densities
• Analytical Template for the 4-Point Correlation Function Covariance Beyond the Gaussian Random Field $\mathrm{I}$: 1-Loop Corrections involving Second-Order Densities
• Structure of cosmic web in non-linear regime: the nearest neighbour and spherical contact distributions
• Lagrangian Perturbation Theory for Biased Tracers: Significance of the Number Conservation
• Visualising relativistic effects in redshift space distortions of large scale structure
• Stable Clustering Ansatz, Consistency Relations and Gravity Dual of Large-Scale Structure
• Tracing Signatures of Modified Gravity in Redshift-Space Galaxy Bispectrum Multipoles: Prospects for Euclid
• Baryon-photon interactions in Resummed Kinetic Field Theory
• Web-Halo Model (WHM): Accurate non-linear matter power spectrum predictions without free parameters
• Addressing Dipole Tension via Clustering in $\Lambda$CDM and beyond
• An Optimal In-Situ Multipole Algorithm for the Isotropic Three-Point Correlation Functions
• Euclid preparation. Full-shape modelling of 2-point and 3-point correlation functions in real space
• Anisotropic Counts-in-Cells in Redshift Space: A New Route to Cosmological Constraints from Galaxy Surveys
• Differentiable Fuzzy Cosmic-Web for Field Level Inference
• The dynamics of background evolution and structure formation in phase space: a semi-cosmographic reconstruction
• Cosmic curl -- Features and convergence of the vorticity power spectrum in $N$-body simulations
• nuGAN: Generative Adversarial Emulator for Cosmic Web with Neutrinos
• Turning dispersion into signal: density-split analyses of pairwise velocities
• A redshift distortion free correlation function at third order in the nonlinear regime
• Testing growth rate dependence in cosmological perturbation theory using scale-free models
• Sensitivity of Cosmological Parameter Estimation to Nonlinear Prescription from Cosmic Shear
• Fast Baryonic Field Painting for Sunyaev-Zel'dovich Analyses: Transfer Function vs. Hybrid Effective Field Theory
• Skewness as a Probe of Gravity: Real and Redshift Space Counts-In-Cells
• Probing gravity with non-linear clustering in redshift space
• Free Cosmic Density Bispectrum on Small Scales
• The anisotropic redshift space galaxy correlation function: detection on the BAO Ring
• Clustering redshifts with the 21cm-galaxy cross-bispectrum
• Testing the growth of cosmic structures during the Dark Ages
• Response approach to the integrated shear 3-point correlation function: the impact of baryonic effects on small scales
• Non-Gaussian likelihood of weak lensing power spectra
• On the Kinematic Morphology around Halos
• Model-agnostic interpretation of 10 billion years of cosmic evolution traced by BOSS and eBOSS data
• Non-Gaussianity in the Squeezed Three-Point Correlation from the Relativistic Effects
• Cosmology with the Redshift-Space Galaxy Bispectrum Monopole at One-Loop Order