A local bias approach to the clustering of discrete density peaks
Vincent Desjacques

TL;DR
This paper introduces a local bias approach to model the clustering of density peaks in Gaussian random fields, simplifying calculations and capturing higher-order effects related to peak asphericity.
Contribution
It presents a novel local bias expansion based on rotational invariants that avoids complex joint probability computations for density peak clustering.
Findings
Bias factors can be computed using peak-background split.
The approach captures asphericity effects with generalized Laguerre polynomials.
The method is potentially extendable to all orders and other point processes.
Abstract
Maxima of the linear density field form a point process that can be used to understand the spatial distribution of virialized halos that collapsed from initially overdense regions. However, owing to the peak constraint, clustering statistics of discrete density peaks are difficult to evaluate. For this reason, local bias schemes have received considerably more attention in the literature thus far. In this paper, we show that the 2-point correlation function of maxima of a homogeneous and isotropic Gaussian random field can be thought of, up to second order at least, as arising from a local bias expansion formulated in terms of rotationally invariant variables. This expansion relies on a unique smoothing scale, which is the Lagrangian radius of dark matter halos. The great advantage of this local bias approach is that it circumvents the difficult computation of joint probability…
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