The Lensing Counter Narrative: An Effective Description of Small-Scale Clustering in Weak Lensing Power Spectra

TL;DR

The paper introduces a new formalism using lensing counterterms inspired by EFT to separate large- and small-scale contributions in weak lensing, improving constraints without hard scale cuts.

Contribution

A novel EFT-inspired formalism that isolates large-scale signals in weak lensing, reducing reliance on scale cuts and enhancing constraining power.

Findings

Improved constraints on $S_8$ from DES Y3 data.

No evidence of deviations from $ m extit{ extbf{Λ}}$CDM at small scales.

Public release of the gholax pipeline for weak lensing analysis.

Abstract

We present a new formalism to separate large- and small-scale contributions to cosmic shear through \textit{lensing counterterms} (LCT) inspired by effective field theory (EFT). Marginalizing over these LCTs isolates the large-scale cosmological signal in weak lensing power spectra while simultaneously constraining the impact of baryonic feedback or new physics (e.g. axion dark matter) at small scales. Our formalism removes the need for hard scale cuts in standard analyses, even when theoretical predictions are limited to below a physical cutoff $\Lambda$, resulting in significant improvements in constraining power -- up to $5\times$ smaller in the case of a LSST-Y10-like analysis without marginalizing over baryons when the analysis cutoff is set to $\Lambda = 1.0h$ Mpc$^{-1}$. We conduct a proof-of-principle analysis on the publicly available DES Y3 data, finding $S_8= 0.783\pm 0.029$ and $S_8 = 0.798\pm 0.026$ for analyses with cutoffs of $\Lambda = 0.5h$ Mpc$^{-1}$ and $1.0 h$ Mpc$^{-1}$, respectively, with no detection of modifications to small-scale clustering at $k > \Lambda$ beyond the predictions of collisionless dark matter in a $\Lambda$CDM universe. We make our \texttt{JAX}-based pipeline, \texttt{gholax}, integrated with intrinsic alignment predictions from the EFT of large-scale structure at 1-loop, publicly available.