New leaves of the tree: percolation analysis for cosmic web with discrete points

TL;DR

This paper introduces a novel percolation analysis method based on discrete galaxy points, utilizing the S-bb relation and PCCET model, to better understand cosmic web connectivity and higher-order correlations.

Contribution

It proposes the S-bb relation and PCCET model for analyzing cosmic web connectivity directly from discrete points, overcoming limitations of density field smoothing.

Findings

S-bb relation is robust against redshift distortion and incompleteness.

Mock galaxy catalogues match two-point correlations but not higher-order correlations.

S-bb relation reveals limitations of HAM in capturing higher-order correlations.

Abstract

Percolation analysis has long been used to quantify the connectivity of the cosmic web. Most of the previous work is based on density fields on grids. By smoothing into fields, we lose information about galaxy properties like shape or luminosity. Lack of mathematical model also limits our understanding of percolation analysis. In order to overcome these difficulties, we have studied percolation analysis based on discrete points. Using a Friends-of-Friends (FoF) algorithm, we generate the S-bb relation, between the fractional mass of the largest connected group (S) and the FoF linking length (bb). We propose a new model, the Probability Cloud Cluster Expansion Theory (PCCET) to relate the S-bb relation with correlation functions. We show that the S-bb relation reflects a combination of all orders of correlation functions. Using N-body simulation, we find that the S-bb relation is robust against redshift distortion and incompleteness in observation. From the Bolshoi simulation, with Halo Abundance Matching (HAM), we have generated a mock galaxy catalogue. Good matching of the projected two-point correlation function with observation is confirmed. However, comparing the mock catalogue with the latest galaxy catalogue from SDSS DR12, we have found significant differences in their S-bb relations. This indicates that the mock galaxy catalogue cannot accurately retain higher order correlation functions than the two-point correlation function, which reveals the limit of HAM method. As a new measurement, S-bb relation is applicable to a wide range of data types, fast to compute, robust against redshift distortion and incompleteness, and it contains information of all orders of correlation function.