Published November 10, 2022 | Version v1
Journal article Open

Weak lensing trispectrum and Kurt-spectra

  • 1. University College London
  • 2. University of Chicago
  • 3. Harvard University

Description

We introduce two kurt-spectra to probe fourth-order statistics of weak lensing convergence maps. Using state-of-the-art numerical simulations, we study the shapes of these kurt-spectra as a function of source redshifts and smoothing angular scales. We employ a pseudo-C approach to estimate the spectra from realistic convergence maps in the presence of an observational mask and noise for stage-IV large-scale structure surveys. We compare these results against theoretical predictions calculated using the FFTLog formalism, and find that a simple nonlinear clustering model — the hierarchical ansatz — can reproduce the numerical trends for the kurt-spectra in the nonlinear regime. In addition, we provide estimators for beyond fourth-order spectra where no definitive analytical results are available, and present corresponding results from numerical simulations.

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Munshi_2022_J._Cosmol._Astropart._Phys._2022_020.pdf

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Additional details

Identifiers

DOI
10.1088/1475-7516/2022/11/020
Other
oai:uchicago.tind.io:13777

Funding

Leverhulme Trust
U.S. Department of Energy
DE-SC0020223
Kavli Foundation

UChicago Information

Division(s)
Physical Sciences Division
Center(s) or Institute(s)
Kavli Institute for Cosmological Physics