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Weak Lensing Trispectrum and Kurt-Spectra

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arxiv 2112.05155 v2 pith:IS3COROA submitted 2021-12-09 astro-ph.CO hep-ph

Weak Lensing Trispectrum and Kurt-Spectra

classification astro-ph.CO hep-ph
keywords kurt-spectranumericalresultsconvergencefourth-orderlensingmapsnonlinear
verification ladder T0 review T1 audit T2 compute T3 formal T4 reserved
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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-$C_{\ell}$ 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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