A robust determination of halo environment in the cosmic field
Peng Wang (PMO/AIP), Xi Kang (PMO/ZJU), Noam I. Libeskind (AIP/Lyon),, Quan Guo (SHAO), Stefan Gottl\'ober (AIP), Wei Wang (PMO/USTC)

TL;DR
This paper introduces an adaptive interpolation method to determine halo environments in the cosmic web, improving robustness against grid resolution limitations compared to traditional fixed-grid Hessian matrix approaches.
Contribution
The authors propose a novel adaptive interpolation technique that computes the Hessian matrix per halo, enhancing convergence and resolution independence over the standard NGP method.
Findings
The new method converges faster with respect to grid resolution.
It shows smaller changes in eigenvalues and eigenvectors when resolution varies.
The approach is recommended for future large-scale structure studies.
Abstract
A number of methods for studying the large-scale cosmic matter distribution exist in the literature. One particularly common method employed to define the cosmic web is to examine the density, velocity or potential field. Such methods are advantageous since a Hessian matrix can be constructed whose eigenvectors (and eigenvalues) indicate the principal directions (and strength) of local collapse or expansion. Technically this is achieved by diagonalizing the Hessian matrix using a fixed finite grid. The resultant large-scale structure quantification is thus inherently limited by the grid's finite resolution. Here, we overcome the obstacle of finite grid resolution by introducing a new method to determine halo environment using an adaptive interpolation which is more robust to resolution than the typical "Nearest Grid Point" (NGP) method. Essentially instead of computing and diagonalizing…
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