Halo abundances and counts-in-cells: The excursion set approach with correlated steps
arXiv:1105.1990 · doi:10.1111/j.1365-2966.2011.20128.x
Abstract
The Excursion Set approach has been used to make predictions for a number of interesting quantities in studies of nonlinear hierarchical clustering. These include the halo mass function, halo merger rates, halo formation times and masses, halo clustering, analogous quantities for voids, and the distribution of dark matter counts in randomly placed cells. The approach assumes that all these quantities can be mapped to problems involving the first crossing distribution of a suitably chosen barrier by random walks. Most analytic expressions for these distributions ignore the fact that, although different k-modes in the initial Gaussian field are uncorrelated, this is not true in real space: the values of the density field at a given spatial position, when smoothed on different real-space scales, are correlated in a nontrivial way. As a result, the problem is to estimate first crossing distribution by random walks having correlated rather than uncorrelated steps. In 1990, Peacock & Heavens presented a simple approximation for the first crossing distribution of a single barrier of constant height by walks with correlated steps. We show that their approximation can be thought of as a correction to the distribution associated with what we call smooth completely correlated walks. We then use this insight to extend their approach to treat moving barriers, as well as walks that are constrained to pass through a certain point before crossing the barrier. For the latter, we show that a simple rescaling, inspired by bivariate Gaussian statistics, of the unconditional first crossing distribution, accurately describes the conditional distribution, independently of the choice of analytical prescription for the former. In all cases, comparison with Monte-Carlo solutions of the problem shows reasonably good agreement. (Abridged)
14 pages, 9 figures; v2 -- revised version with explicit demonstration that the original conclusions hold for LCDM, expanded discussion on stochasticity of barrier. Accepted in MNRAS
References in corpus (7)
- Toward a Universal Formulation of the Halo Mass Function
- Excursion Set Halo Mass Function and Bias in a Stochastic Barrier Model of Ellipsoidal Collapse
- The Bias and Mass Function of Dark Matter Halos in Non-Markovian Extension of the Excursion Set Theory
- Perturbation theory and excursion set estimates of the probability distribution function of dark matter, and a method for reconstructing the initial distribution function
- Spherical Collapse and Cluster Counts in Modified Gravity Models
- Excursion Set Theory for generic moving barriers and non-Gaussian initial conditions
- Dark matter halo creation in moving barrier models
Cited by in corpus (43)
- Large-Scale Galaxy Bias
- Large-scale Bias and Efficient Generation of Initial Conditions for Non-Local Primordial Non-Gaussianity
- Non-local Lagrangian bias
- Peaks theory and the excursion set approach
- One step beyond: The excursion set approach with correlated steps
- Excursion set peaks: a self-consistent model of dark halo abundances and clustering
- Scale dependent halo bias in the excursion set approach
- The Hunt for Primordial Interactions in the Large Scale Structures of the Universe
- Voids in Modified Gravity Reloaded: Eulerian Void Assignment
- Excursion set theory for modified gravity: correlated steps, mass functions and halo bias
- An improved model of HII bubbles during the epoch of reionization
- Excursion set theory for modified gravity: Eulerian versus Lagrangian environments
- The importance of stepping up in the excursion set approach
- Large Scale Anisotropic Bias from Primordial non-Gaussianity
- The locations of halo formation and the peaks formalism
- Statistics of Dark Matter Halos from the Excursion Set Approach
- The Excursion set approach: Stratonovich approximation and Cholesky decomposition
- The universal multiplicity function: counting halos and voids
- The Effect of Local non-Gaussianity on the Matter Bispectrum at Small Scales
- The excursion set approach in non-Gaussian random fields
- Stochastic bias in multi-dimensional excursion set approaches
- The scale-dependent signature of primordial non-Gaussianity in the large-scale structure of cosmic reionization
- Impacts of biasing schemes in the one-loop integrated perturbation theory
- On the Markovian assumption in the excursion set approach: the approximation of Markov Velocities
- Halo statistics in non-Gaussian cosmologies: the collapsed fraction, conditional mass function, and halo bias from the path-integral excursion set method
- Halo Mass Definition and Multiplicity Function
- An analytical model of the large neutral regions during the late stage of reionization
- A Stochastic Theory of the Hierarchical Clustering I. Halo Mass Function
- Cosmology with Galaxy Clusters: Systematic Effects in the Halo Mass Function
- Using large scale structure data and a halo model to constrain Generalised Dark Matter
- Excursion Set Theory for Correlated Random Walks
- Statistics of Dark Matter Halos in the Excursion Set Peak Framework
- An Extended Zel'dovich Model for the Halo Mass Function
- A Stochastic Theory of the Hierarchical Clustering II. Halo progenitor mass function and large-scale bias
- Scale-dependent bias from an inflationary bispectrum: the effect of a stochastic moving barrier
- A spherical hydrodynamical model of cosmic voids in ΛCDM and beyond
- Accurate halo mass functions from the simplest excursion set theory
- Mass accretion rates and multi-scale halo environment in cold and warm dark matter cosmologies
- The Effect of Primordial Anti-Biasing on the Local Measurement of the Key Cosmological Parameters
- Mass function and assembly of dark halos: an approach to inventory isolated overdense regions in random fields
- The Extended Zel'dovich Mass Functions of Clusters and Isolated Clusters in the Presence of Primordial Non-Gaussianity
- Excursion-set for Primordial Black Holes I: white noise and moving barrier
- Addressing the too-big-to-fail problem and the void phenomenon through a modified initial power spectrum