Higher Order Statistics for Three-dimensional Shear and Flexion

TL;DR

This paper develops higher-order statistical tools for analyzing three-dimensional spinorial fields in weak gravitational lensing, enabling efficient extraction of cosmological information from noisy, high-frequency data.

Contribution

It introduces new power spectrum-based statistics for 3D spinorial fields, optimized for weak lensing studies, and demonstrates their robustness against noise and masking effects.

Findings

Statistics effectively compress noisy modes

Confrontation with theory is efficient using Limber's approximation

Applicable to scalar and spinorial fields in 3D weak lensing

Abstract

We introduce a collection of statistics appropriate for the study of spinorial quantities defined in three dimensions, focussing on applications to cosmological weak gravitational lensing studies in 3D. In particular, we concentrate on power spectra associated with three- and four-point statistics, which have the advantage of compressing a large number of typically very noisy modes into a convenient data set. It has been shown previously by \cite{MuHe09} that, for non--Gaussianity studies in the microwave background, such compression can be lossless for certain purposes, so we expect the statistics we define here to capture the bulk of the cosmological information available in these higher-order statistics. We consider the effects of a sky mask and noise, and use Limber's approximation to show how, for high-frequency angular modes, confrontation of the statistics with theory can be achieved efficiently and accurately. We focus on scalar and spinorial fields including convergence, shear and flexion of 3D weak lensing, but many of the results apply for general spin fields.