Halo abundances and counts-in-cells: The excursion set approach with correlated steps
Aseem Paranjape, Tsz Yan Lam, Ravi K. Sheth

TL;DR
This paper refines the excursion set approach for predicting halo properties by incorporating correlated steps in random walks, extending previous models to include moving barriers and constraints, with validation against Monte Carlo simulations.
Contribution
It introduces an improved approximation for correlated steps in the excursion set approach, extending it to moving barriers and constrained walks, enhancing predictive accuracy.
Findings
The approximation aligns well with Monte Carlo solutions.
Extension to moving barriers improves modeling flexibility.
Conditional distributions are accurately described by a simple rescaling.
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…
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