The cosmic web connection to the dark matter halo distribution through gravity

Abstract

This work investigates the connection between the cosmic web and the halo distribution through the gravitational potential at the field level. We combine three fields of research, cosmic web classification, perturbation theory expansions of the halo bias, and halo (galaxy) mock catalogue making methods. In particular, we use the invariants of the tidal field and the velocity shear tensor as generating functions to reproduce the halo number counts of a reference catalogue from full gravity calculations, populating the dark matter field on a mesh well into the non-linear regime ($3h^{-1}\mathrm{Mpc}$ scales). Our results show an unprecedented agreement with the reference power spectrum within 1% up to $k=0.72h{\mathrm{Mpc}}^{-1}$. By analysing the three-point statistics on large scales (configurations of up to $k=0.2h{\mathrm{Mpc}}^{-1}$), we find evidence for non-local bias at the 4.8 $\sigma$ confidence level, being compatible with the reference catalogue. In particular, we find that a detailed description of tidal anisotropic clustering on large scales is crucial to achieve this accuracy at the field level. These findings can be particularly important for the analysis of the next generation of galaxy surveys in mock galaxy production.

arXiv comment19 pages, 10 figures and 2 tables, accepted for publication at MNRAS

References in corpus (165)

• Large scale bias and the peak background split
• Populating a cluster of galaxies - I. Results at z=0
• Halo Models of Large Scale Structure
• Large-Scale Structure of the Universe and Cosmological Perturbation Theory
• An analytic model for the spatial clustering of dark matter haloes
• The Environmental Dependence of the Relations between Stellar Mass, Structure, Star Formation and Nuclear Activity in Galaxies
• How Filaments are Woven into the Cosmic Web
• Analytic model for galaxy and dark matter clustering
• The Large Scale Bias of Dark Matter Halos: Numerical Calibration and Model Tests
• An excursion set model of hierarchical clustering: Ellipsoidal collapse and the moving barrier
• Power Spectrum Analysis of Three-Dimensional Redshift Surveys
• Galaxy bimodality versus stellar mass and environment
• Large-Scale Galaxy Bias
• The bimodal galaxy color distribution: dependence on luminosity and environment
• Relationship between environment and the broad-band optical properties of galaxies in the SDSS
• Properties of Dark Matter Haloes in Clusters, Filaments, Sheets and Voids
• A hierarchy of voids: Much ado about nothing
• Resumming Cosmological Perturbations via the Lagrangian Picture: One-loop Results in Real Space and in Redshift Space
• Biasing and Hierarchical Statistics in Large-scale Structure
• Clustering of dark matter tracers: generalizing bias for the coming era of precision LSS
• Assembly bias in the clustering of dark matter haloes
• Stochastic Nonlinear Galaxy Biasing
• Tracing the cosmic web
• The clustering of galaxies in the SDSS-III Baryon Oscillation Spectroscopic Survey: RSD measurement from the power spectrum and bispectrum of the DR12 BOSS galaxies
• The clustering of galaxies in the SDSS-III Baryon Oscillation Spectroscopic Survey: mock galaxy catalogues for the BOSS Final Data Release
• Bayesian physical reconstruction of initial conditions from large scale structure surveys
• 4MOST: Project overview and information for the First Call for Proposals
• Gravity and Large-Scale Non-local Bias
• Detecting filamentary pattern in the cosmic web: a catalogue of filaments for the SDSS
• A Dynamical Classification of the Cosmic Web
• The persistent cosmic web and its filamentary structure II: Illustrations
• Evidence for Quadratic Tidal Tensor Bias from the Halo Bispectrum
• Spin alignment of dark matter haloes in filaments and walls
• The IR-resummed Effective Field Theory of Large Scale Structures
• Cosmic Voids in Sloan Digital Sky Survey Data Release 7
• The Multiscale Morphology Filter: Identifying and Extracting Spatial Patterns in the Galaxy Distribution
• The Scale Dependence of Halo and Galaxy Bias: Effects in Real Space
• The bispectrum of galaxies from high-redshift galaxy surveys: primordial non-Gaussianity and non-linear galaxy bias
• Testing Tidal-Torque Theory: I. Spin Amplitude and Direction
• NEXUS: Tracing the Cosmic Web Connection
• PINOCCHIO: pinpointing orbit-crossing collapsed hierarchical objects in a linear density field
• Evolution of the angular momentum of protogalaxies from tidal torques: Zel'dovich approximation
• Learning to Predict the Cosmological Structure Formation
• Bias in the Effective Field Theory of Large Scale Structures
• Renormalized Halo Bias
• The Lagrangian-space Effective Field Theory of Large Scale Structures
• Warm-hot baryons comprise 5-10 per cent of filaments in the cosmic web
• EZmocks: extending the Zel'dovich approximation to generate mock galaxy catalogues with accurate clustering statistics
• Understanding higher-order nonlocal halo bias at large scales by combining the power spectrum with the bispectrum
• Biased Tracers and Time Evolution
• PTHalos: A fast method for generating mock galaxy distributions
• A kinematic classification of the cosmic web
• Large-scale bias in the Universe: bispectrum method
• Mock galaxy catalogs using the quick particle mesh method
• Halo Stochasticity from Exclusion and non-linear Clustering
• Modelling Baryon Acoustic Oscillations with Perturbation Theory and Stochastic Halo Biasing
• Large-scale Bias and Efficient Generation of Initial Conditions for Non-Local Primordial Non-Gaussianity
• Tracing the Dark Matter Sheet in Phase Space
• Clustering of dark matter tracers: renormalizing the bias parameters
• On the Renormalization of the Effective Field Theory of Large Scale Structures
• Counting voids to probe dark energy
• Testing Tidal-Torque Theory: II. Alignment of Inertia and Shear and the Characteristics of Proto-haloes
• The Spine of the Cosmic Web
• Non-linear Stochastic Galaxy Biasing in Cosmological Simulations
• The darkness that shaped the void: dark energy and cosmic voids
• The Bispectrum in the Effective Field Theory of Large Scale Structure
• Probing the missing baryons with the Sunyaev-Zel'dovich effect from filaments
• A reconstruction of the initial conditions of the Universe by optimal mass transportation
• Precision cosmology with voids: definition, methods, dynamics
• Lagrangian theory of gravitational instability of Friedman-Lemaitre cosmologies - generic third-order model for non-linear clustering
• Origin and evolution of halo bias in linear and non-linear regimes
• Gaussian covariance matrices for anisotropic galaxy clustering measurements
• Modeling scale-dependent bias on the baryonic acoustic scale with the statistics of peaks of Gaussian random fields
• The Cosmic Web: Geometric Analysis
• Biasing and the distribution of dark matter haloes
• The Cosmic Web, Multi-Stream Flows, and Tessellations
• The three dimensional skeleton: tracing the filamentary structure of the universe
• The Nonlinear Evolution of Rare Events
• Modeling Biased Tracers at the Field Level
• Halo assembly bias and the tidal anisotropy of the local halo environment
• The Properties of Cosmic Velocity Fields
• The fine-grained phase-space structure of Cold Dark Matter halos
• ORIGAMI: Delineating Halos using Phase-Space Folds
• The cosmic web and the orientation of angular momenta
• The Initial Conditions of the Universe from Constrained Simulations
• The One-Loop Matter Bispectrum in the Effective Field Theory of Large Scale Structures
• Streams and caustics: the fine-grained structure of LCDM haloes
• The Cosmic Ballet II: Spin alignment of galaxies and haloes with large-scale filaments in the EAGLE simulation
• Non-linear evolution of the angular momentum of protostructures from tidal torques
• Non-local Lagrangian bias
• ICE-COLA: Towards fast and accurate synthetic galaxy catalogues optimizing a quasi $N$-body method
• Galaxy Colour, Morphology, and Environment in the Sloan Digital Sky Survey
• The mass-Peak Patch algorithm for fast generation of deep all-sky dark matter halo catalogues and its N-Body validation
• The assembly bias of dark matter haloes to higher orders
• Peak-Background Split, Renormalization, and Galaxy Clustering
• Lagrangian Dynamics in Non-Flat Universes and Non-Linear Gravitational Evolution
• The Environmental Dependence of the Infrared Luminosity and Stellar Mass Functions
• Predicting the number, spatial distribution and merging history of dark matter haloes
• Cubic Halo Bias in Eulerian and Lagrangian Space
• The cosmology dependence of galaxy clustering and lensing from a hybrid $N$-body-perturbation theory model
• Stochasticity of Bias and Nonlocality of Galaxy Formation: Linear Scales
• Reconstructing the Initial Density Field of the Local Universe: Method and Test with Mock Catalogs
• On the Distribution of Haloes, Galaxies and Mass
• Comparing approximate methods for mock catalogues and covariance matrices II: Power spectrum multipoles
• Comparing approximate methods for mock catalogues and covariance matrices I: correlation function
• Bias Loop Corrections to the Galaxy Bispectrum
• Beyond LIMD bias: a measurement of the complete set of third-order halo bias parameters
• Fast and accurate mock catalogue generation for low-mass galaxies
• The Zeldovich approximation: key to understanding Cosmic Web complexity
• Void Ellipticity Distribution as a Probe of Cosmology
• Comparing approximate methods for mock catalogues and covariance matrices III: Bispectrum
• The Evolution of Assembly Bias
• Cosmic web anisotropy is the primary indicator of halo assembly bias
• Constraining the halo bispectrum in real and redshift space from perturbation theory and non-linear stochastic bias
• An Interacting Galaxy System Along a Filament in a Void
• On the Statistics of Biased Tracers in the Effective Field Theory of Large Scale Structures
• More out of less: an excess integrated Sachs-Wolfe signal from supervoids mapped out by the Dark Energy Survey
• A halo bias function measured deeply into voids without stochasticity
• Linear redshift space distortions for cosmic voids based on galaxies in redshift space
• HALOGEN: A tool for fast generation of mock halo catalogues
• Signatures of the Primordial Universe from Its Emptiness: Measurement of Baryon Acoustic Oscillations from Minima of the Density Field
• Testing one-loop galaxy bias: joint analysis of power spectrum and bispectrum
• Large-scale assembly bias of dark matter halos
• On the least action principle in cosmology
• Halo bias in Lagrangian Space: Estimators and theoretical predictions
• The cosmological background of vector modes
• The multidimensional dependence of halo bias in the eye of a machine: a tale of halo structure, assembly and environment
• Cosmic web dependence of galaxy clustering and quenching in SDSS
• The cosmic web of the Local Universe: cosmic variance, matter content and its relation to galaxy morphology
• Galaxy Quenching from Cosmic Web Detachment
• Caustic Skeleton & Cosmic Web
• Estimating cosmic velocity fields from density fields and tidal tensors
• Modelling large-scale halo bias using the bispectrum
• Linearisation with Cosmological Perturbation Theory
• Extremely Metal-Poor Galaxies: The Environment
• Measuring Baryon Acoustic Oscillations from the clustering of voids
• Painting halos from cosmic density fields of dark matter with physically motivated neural networks
• On the Bispectra of Very Massive Tracers in the Effective Field Theory of Large-Scale Structure
• BAM: Bias Assignment Method to generate mock catalogs
• Nonlinear Bias of Cosmological Halo Formation in the Early Universe
• New method for initial density reconstruction
• Perturbative description of bias tracers using consistency relations of LSS
• A Zeldovich reconstruction method for measuring redshift space distortions using cosmic voids
• Dependence of halo bias on mass and environment
• Dark Matter Caustics
• Beyond two-point statistics: using the minimum spanning tree as a tool for cosmology
• Revealing the cosmic web dependent halo bias
• Modeling the clustering of dark-matter haloes in resummed perturbation theories
• Vorticity generation in the Universe: A perturbative approach
• A new method to measure galaxy bias
• Some assembly required: assembly bias in massive dark matter halos
• Cosmic Velocity Field Reconstruction Using AI
• The bias of dark matter tracers: assessing the accuracy of mapping techniques
• The Variation of Galaxy Morphological Type with the Shear of Environment
• The large-scale environment from cosmological simulations II: The redshift evolution and distributions of baryons
• One simulation to have them all: performance of the Bias Assignment Method against N-body simulations
• Improving baryon acoustic oscillation measurement with the combination of cosmic voids and galaxies
• Beta-Skeleton Analysis of the Cosmic Web
• Renormalisation of linear halo bias in N-body simulations
• Accurate halo-galaxy mocks from automatic bias estimation and particle mesh gravity solvers
• Large-scale bias of dark matter halos
• Robustness of the covariance matrix for galaxy clustering measurements
• Constraining the baryon fraction in the Warm Hot Intergalactic Medium at low redshifts with PLANCK data
• Complete Zeldovich approximation
• Symmetries, Invariants and Generating Functions: Higher-order Statistics of Biased Tracers

Cited by in corpus (8)

• The Bacco Simulation Project: Bacco Hybrid Lagrangian Bias Expansion Model in Redshift Space
• $\text{PineTree}$: A generative, fast, and differentiable halo model for wide-field galaxy surveys
• On general-relativistic Lagrangian perturbation theory and its non-perturbative generalization
• Secondary halo bias through cosmic time II: Reconstructing halo properties using clustering information
• Fast simulation mapping: from standard to modified gravity cosmologies using the bias assignment method
• Gaussian Lagrangian Galaxy Bias
• Bye-bye, Local-in-matter-density Bias: The Statistics of the Halo Field Are Poorly Determined by the Local Mass Density
• Differentiable Fuzzy Cosmic-Web for Field Level Inference