Large-scale structure perturbation theory without losing stream crossing
arXiv:1709.02834 · doi:10.1103/PhysRevD.97.023508
Abstract
We suggest an approach to perturbative calculations of large-scale clustering in the Universe that includes from the start the stream crossing (multiple velocities for mass elements at a single position) that is lost in traditional calculations. Starting from a functional integral over displacement, the perturbative series expansion is in deviations from (truncated) Zel'dovich evolution, with terms that can be computed exactly even for stream-crossed displacements. We evaluate the one-loop formulas for displacement and density power spectra numerically in 1D, finding dramatic improvement in agreement with N-body simulations compared to the Zel'dovich power spectrum (which is exact in 1D up to stream crossing). Beyond 1D, our approach could represent an improvement over previous expansions even aside from the inclusion of stream crossing, but we have not investigated this numerically. In the process we show how to achieve effective-theory-like regulation of small-scale fluctuations without free parameters.
added pedagogical explanation of key math trick in appendix
References in corpus (140)
- A Line of Sight Approach to Cosmic Microwave Background Anisotropies
- Large-Scale Structure of the Universe and Cosmological Perturbation Theory
- Cosmological Perturbation Theory in the Synchronous vs. Conformal Newtonian Gauge
- Cosmological Perturbation Theory in the Synchronous and Conformal Newtonian Gauges
- The DESI Experiment Part I: Science,Targeting, and Survey Design
- Enzo: An Adaptive Mesh Refinement Code for Astrophysics
- Large-Scale Galaxy Bias
- Cosmological Non-Linearities as an Effective Fluid
- The Effective Field Theory of Cosmological Large Scale Structures
- Renormalized Cosmological Perturbation Theory
- Resumming Cosmological Perturbations via the Lagrangian Picture: One-loop Results in Real Space and in Redshift Space
- Nonlinear Evolution of Baryon Acoustic Oscillations
- Anisotropies in the Cosmic Microwave Background: An Analytic Approach
- Relative velocity of dark matter and baryonic fluids and the formation of the first structures
- The Lyman-alpha Forest Power Spectrum from the Sloan Digital Sky Survey
- Baryon Acoustic Oscillations in 2D: Modeling Redshift-space Power Spectrum from Perturbation Theory
- Clustering of dark matter tracers: generalizing bias for the coming era of precision LSS
- The Linear Theory Power Spectrum from the Lyman-alpha Forest in the Sloan Digital Sky Survey
- The Observed Probability Distribution Function, Power Spectrum, and Correlation Function of the Transmitted Flux in the Lyman-alpha Forest
- Memory of Initial Conditions in Gravitational Clustering
- DESI and other dark energy experiments in the era of neutrino mass measurements
- The clustering of galaxies in the completed SDSS-III Baryon Oscillation Spectroscopic Survey: Baryon Acoustic Oscillations in Fourier-space
- Evidence for Quadratic Tidal Tensor Bias from the Halo Bispectrum
- How to measure redshift-space distortions without sample variance
- Nonlinear perturbation theory with halo bias and redshift-space distortions via the Lagrangian picture
- Primordial Black Holes as Dark Matter: The Power Spectrum and Evaporation of Early Structures
- 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
- Toward a Measurement of the Cosmological Geometry at z~2: Predicting Lyman-alpha Forest Correlation in Three Dimensions, and the Potential of Future Data Sets
- A critical look at cosmological perturbation theory techniques
- Beyond linear galaxy alignments
- FastPM: a new scheme for fast simulations of dark matter and halos
- Generation of Vorticity and Velocity Dispersion by Orbit Crossing
- Understanding higher-order nonlocal halo bias at large scales by combining the power spectrum with the bispectrum
- RegPT: Direct and fast calculation of regularized cosmological power spectrum at two-loop order
- Resumming Cosmic Perturbations
- Clustering of dark matter tracers: renormalizing the bias parameters
- Multi-Point Propagators in Cosmological Gravitational Instability
- A Measurement of the Temperature-Density Relation in the Intergalactic Medium Using a New Lyman-alpha Absorption Line Fitting Method
- A Closure Theory for Non-linear Evolution of Cosmological Power Spectra
- Primordial non-Gaussianity: large-scale structure signature in the perturbative bias model
- Dark energy and curvature from a future baryonic acoustic oscillation survey using the Lyman-alpha forest
- Nonlinear Perturbation Theory Integrated with Nonlocal Bias, Redshift-space Distortions, and Primordial Non-Gaussianity
- Nonlinear Cosmological Power Spectra in Real and Redshift--Space
- Structure formation from non-Gaussian initial conditions: multivariate biasing, statistics, and comparison with N-body simulations
- FAST-PT: a novel algorithm to calculate convolution integrals in cosmological perturbation theory
- Non-linear Evolution of Baryon Acoustic Oscillations from Improved Perturbation Theory in Real and Redshift Spaces
- The impact of intrinsic alignment on current and future cosmic shear surveys
- Dark matter clustering: a simple renormalization group approach
- Modeling Nonlinear Evolution of Baryon Acoustic Oscillations: Convergence Regime of N-body Simulations and Analytic Models
- Simulations of Baryon Acoustic Oscillations II: Covariance matrix of the matter power spectrum
- Accounting for baryonic effects in cosmic shear tomography: Determining a minimal set of nuisance parameters using PCA
- Non-linear Power Spectrum including Massive Neutrinos: the Time-RG Flow Approach
- Nonlinear power spectrum in the presence of massive neutrinos: perturbation theory approach, galaxy bias and parameter forecasts
- The Gaussian streaming model and Lagrangian effective field theory
- The WiggleZ Dark Energy Survey: the selection function and z=0.6 galaxy power spectrum
- Gravitational redshift and other redshift-space distortions of the imaginary part of the power spectrum
- Distribution function approach to redshift space distortions
- The Effective Field Theory of Dark Matter and Structure Formation: Semi-Analytical Results
- Perturbation Theory Reloaded II: Non-linear Bias, Baryon Acoustic Oscillations and Millennium Simulation In Real Space
- Cosmological Information in the Intrinsic Alignments of Luminous Red Galaxies
- Massive Neutrinos in Cosmology: Analytic Solutions and Fluid Approximation
- Bispectrum and Nonlinear Biasing of Galaxies: Perturbation Analysis, Numerical Simulation and SDSS Galaxy Clustering
- Large-N expansions applied to gravitational clustering
- Coarse-Grained Cosmological Perturbation Theory
- Fast Large Scale Structure Perturbation Theory using 1D FFTs
- Lagrangian perturbations and the matter bispectrum I: fourth-order model for non-linear clustering
- Non-Gaussian Covariance of the Matter Power Spectrum in the Effective Field Theory of Large Scale Structure
- FAST-PT II: an algorithm to calculate convolution integrals of general tensor quantities in cosmological perturbation theory
- Constructing Regularized Cosmic Propagators
- Cosmological perturbation theory in 1+1 dimensions
- Lagrangian perturbation theory at one loop order: successes, failures, and improvements
- Third-Order Density Perturbation and One-Loop Power Spectrum in Dark-Energy-Dominated Universe
- Dynamics of gravitational clustering II. Steepest-descent method for the quasi-linear regime
- The Mildly Non-Linear Regime of Structure Formation
- An accurate and practical method for inference of weak gravitational lensing from galaxy images
- Distribution function approach to redshift space distortions. Part IV: perturbation theory applied to dark matter
- Linear redshift space distortions for cosmic voids based on galaxies in redshift space
- Extracting Angular Diameter Distance and Expansion Rate of the Universe from Two-dimensional Galaxy Power Spectrum at High Redshifts: Baryon Acoustic Oscillation Fitting versus Full Modeling
- Distribution function approach to redshift space distortions. Part II: N-body simulations
- Baryonic Acoustic Oscillations via the Renormalization Group
- Precision Cosmology from the Lyman-alpha Forest: Power Spectrum and Bispectrum
- A new approach to gravitational clustering: a path-integral formalism and large-N expansions
- The recursion relation in Lagrangian perturbation theory
- Distribution function approach to redshift space distortions, Part III: halos and galaxies
- Non-Gaussian Error Contribution to Likelihood Analysis of the Matter Power Spectrum
- Extending the modeling of the anisotropic galaxy power spectrum to
- Large scale structure from viscous dark matter
- Peculiar velocities in redshift space: formalism, N-body simulations and perturbation theory
- Scale-Dependent Galaxy Bias from Massive Particles with Spin during Inflation
- Non-linear Fields in Generalized Cosmologies
- Matter bispectrum of large-scale structure: Three-dimensional comparison between theoretical models and numerical simulations
- Next-to-leading resummation of cosmological perturbations via the Lagrangian picture: 2-loop correction in real and redshift spaces
- Regularized cosmological power spectrum and correlation function in modified gravity models
- FFT-PT: Reducing the two-loop large-scale structure power spectrum to low-dimensional radial integrals
- The Evolution of Baryon Density Fluctuations in Multi-Component Cosmological Simulations
- Higher-order massive neutrino perturbations in large-scale structure
- Simulations of Baryon Acoustic Oscillations I: Growth of Large-Scale Density Fluctuations
- A microscopic, non-equilibrium, statistical field theory for cosmic structure formation
- Impact of shell crossing and scope of perturbative approaches in real and redshift space
- Power spectra in the eikonal approximation with adiabatic and non-adiabatic modes
- How to generate a significant effective temperature for cold dark matter, from first principles
- Post-collapse perturbation theory in 1D cosmology -- beyond shell-crossing
- Signatures of Primordial non-Gaussianities in the Matter Power-Spectrum and Bispectrum: the Time-RG Approach
- Lagrangian perturbations and the matter bispectrum II: the resummed one-loop correction to the matter bispectrum
- Using the Zeldovich dynamics to test expansion schemes
- Propagators in Lagrangian space
- Dynamics of gravitational clustering I. Building perturbative expansions
- Renormalized Newtonian Cosmic Evolution with Primordial Non-Gaussianity
- Next-to-leading resummations in cosmological perturbation theory
- Expansion schemes for gravitational clustering: computing two-point and three-point functions
- Modeling the clustering of dark-matter haloes in resummed perturbation theories
- Halo Sampling, Local Bias and Loop Corrections
- Characteristic Scales of Baryon Acoustic Oscillations from Perturbation Theory: Non-linearity and Redshift-Space Distortion Effects
- Renormalization-group flow of the effective action of cosmological large-scale structures
- Cosmological implications from the full shape of the large-scale power spectrum of the SDSS DR7 luminous red galaxies
- How well can (renormalized) perturbation theory predict dark matter clustering properties?
- The Clustering of Galaxies in the Completed SDSS-III Baryon Oscillation Spectroscopic Survey: Cosmic Flows and Cosmic Web from Luminous Red Galaxies
- Large-scale Correlation of Mass and Galaxies with the Lyman-alpha Forest Transmitted Flux
- Scale dependent bias from primordial non-Gaussianity with trispectrum
- Self-Similar Bumps and Wiggles: Isolating the Evolution of the BAO Peak with Power-law Initial Conditions
- The dark matter dispersion tensor in perturbation theory
- Scale Transformations, Tree-level Perturbation Theory, and the Cosmological Matter Bispectrum
- Testing the consistency of three-point halo clustering in Fourier and configuration space
- Linear and Second-Order Evolution of Cosmic Baryon Perturbations below 10^6 Solar Masses
- Simulating the Anisotropic Clustering of Luminous Red Galaxies with Subhalos: A Direct Confrontation with Observation and Cosmological Implications
- The Helmholtz Hierarchy: Phase Space Statistics of Cold Dark Matter
- Lensing smoothing of BAO wiggles
- Baryon oscillations in galaxy and matter power-spectrum covariance matrices
- The adhesion model as a field theory for cosmological clustering
- Damping of the baryon acoustic oscillations in the matter power spectrum as a probe of the growth factor
- An Application of Wiener Hermite Expansion to Non-linear Evolution of Dark Matter
- Renormalizing a Viscous Fluid Model for Large Scale Structure Formation
- Higher-Order Gravitational Lensing Reconstruction using Feynman Diagrams
- A Comment on the Path Integral Approach to Cosmological Perturbation Theory
- Perturbative interaction approach to cosmological structure formation
- Building Unbiased Estimators from Non-Gaussian Likelihoods with Application to Shear Estimation
- A model of the anisotropic correlation function xi(rp, pi) in redshift space including redshift errors
- Large-k Limit of Multi-Point Propagators in the RG Formalism
- What the "simple renormalization group" approach to dark matter clustering really was
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- Accurate initial conditions for cosmological N-body simulations: Minimizing truncation and discreteness errors
- GridSPT: Grid-based calculation for perturbation theory of large-scale structure
- The Generation of Vorticity in Cosmological N-body Simulations
- The EFT Likelihood for Large-Scale Structure
- Structure formation beyond shell-crossing: nonperturbative expansions and late-time attractors
- Cosmological perturbations for two cold fluids in CDM
- Cosmological Vlasov-Poisson equations for dark matter: Recent developments and connections to selected plasma problems
- Perturbation theory with dispersion and higher cumulants: non-linear regime
- Divergence of Perturbation Theory in Large Scale Structures
- Perturbation theory with dispersion and higher cumulants: framework and linear theory
- Finding closure: approximating Vlasov-Poisson using finitely generated cumulants
- Evolution of dark matter velocity dispersion
- Perturbation theory of LSS in the CDM Universe: exact time evolution and the two-loop power spectrum
- Kinetic Field Theory: Exact free evolution of Gaussian phase-space correlations
- Asymptotic expansions for the Large Scale Structure
- A first comparison of Kinetic Field Theory with Eulerian Standard Perturbation Theory
- Kinetic Field Theory for Cosmic Structure Formation
- Kinetic Field Theory: Perturbation theory beyond first order
- Dark matter vorticity and velocity dispersion from truncated Dyson$\unicode{x2013}$Schwinger equations
- Resummed Kinetic Field Theory: a model of coupled baryonic and dark matter
- Renormalization group computation of likelihood functions for cosmological data sets
- Cosmological perturbation theory for large scale structure in phase space
- Calculating the EFT likelihood via saddle-point expansion
- Improved renormalization group computation of likelihood functions for cosmological data sets
- Projection of the gravitational dynamics on a subspace of probability distributions: curl-free Gaussian ansatz
- Lagrangian-space Gaussian ansatz for the matter redshift-space power spectrum and correlation function
- Lagrangian Perturbation Theory for Biased Tracers: Significance of the Number Conservation
- Baryon-photon interactions in Resummed Kinetic Field Theory