Skewness as a probe of non-Gaussian initial conditions
arXiv:astro-ph/0005087 · doi:10.1103/PhysRevD.62.021301
Abstract
We compute the skewness of the matter distribution arising from non-linear evolution and from non-Gaussian initial perturbations. We apply our result to a very generic class of models with non-Gaussian initial conditions and we estimate analytically the ratio between the skewness due to non-linear clustering and the part due to the intrinsic non-Gaussianity of the models. We finally extend our estimates to higher moments.
arXiv comment5 pages, 2 ps-figs., accepted for publication in PRD, rapid comm
References in corpus (11)
- The density and peculiar velocity fields of nearby galaxies
- Skewness Induced by Gravity
- An Isocurvature CDM Cosmogony. II. Observational Tests
- Cosmic Microwave Background Anisotropies from Scaling Seeds: Global Defect Models
- An Isocurvature CDM Cosmogony. I. A Worked Example of Evolution Through Inflation
- The Projected Three-point Correlation Function: Theory and Observations
- Seeds of large-scale anisotropy in string cosmology
- Massless (pseudo-)scalar seeds of CMB anisotropy
- Cosmological Perturbation Theory and the Spherical Collapse Model - II. Non-Gaussian initial conditions
- Cosmic Microwave Background anisotropies and extra dimensions in String Cosmology
- Microwave Background Anisotropies Induced by Global Scalar Fields: The Large N Limit
Cited by in corpus (29)
- Large-Scale Structure of the Universe and Cosmological Perturbation Theory
- How Many Galaxies Fit in a Halo? Constraints on Galaxy Formation Efficiency from Spatial Clustering
- Non-Gaussianity in multi-field inflation
- Effects of Scale-Dependent Non-Gaussianity on Cosmological Structures
- The bispectrum of galaxies from high-redshift galaxy surveys: primordial non-Gaussianity and non-linear galaxy bias
- Cosmic Structure Formation with Topological Defects
- Primordial non-Gaussianity and Bispectrum Measurements in the Cosmic Microwave Background and Large-Scale Structure
- Inflationary models inducing non-Gaussian metric fluctuations
- Constraining Running Non-Gaussianity
- Halo Clustering with Non-Local Non-Gaussianity
- 1-loop Perturbative Corrections to the Matter and Galaxy Bispectrum with non-Gaussian Initial Conditions
- Testing the theory of gravity with DESI: estimators, predictions and simulation requirements
- The Void Abundance with Non-Gaussian Primordial Perturbations
- Cosmic microwave background bispectrum on small angular scales
- Primordial non-Gaussianity in the large scale structure of the Universe
- The Trispectrum of the 4 Year COBE-DMR data
- The Hunt for Primordial Interactions in the Large Scale Structures of the Universe
- Bayesian field-level inference of primordial non-Gaussianity using next-generation galaxy surveys
- Higher Order Moments of the Angular Distribution of Galaxies from Early SDSS Data
- Hunting high and low: Disentangling primordial and late-time non-Gaussianity with cosmic densities in spheres
- Hierarchy of N-point functions in the LCDM and ReBEL cosmologies
- Non-Gaussianity from Self-Ordering Scalar Fields
- Weak Lensing Effects on the Galaxy Three-Point Correlation Function
- Non-Gaussian Halo Mass Function and Non-Spherical Halo Collapse: Theory vs. Simulations
- Finite volume effects for non-Gaussian multi-field inflationary models
- The VIMOS Public Extragalactic Redshift Survey (VIPERS). Hierarchical scaling and biasing
- Real space tests of the statistical isotropy and Gaussianity of the WMAP CMB data
- Skewness as a probe of Baryon Acoustic Oscillations
- Evolution of Power Spectrum in Non-Gaussian Models