The constraining power of the Marked Power Spectrum: an analytical study
Marco Marinucci, Gabriel Jung, Michele Liguori, Andrea Ravenni,, Francesco Spezzati, Adam Andrews, Marco Baldi, William R. Coulton, Dionysios, Karagiannis, Francisco Villaescusa-Navarro, Benjamin Wandlet

TL;DR
This paper provides the first comprehensive analytical study of the marked power spectrum's sensitivity to primordial non-Gaussianity, comparing its constraining power to traditional methods and exploring optimal mark parameters.
Contribution
It extends effective field theory to include primordial non-Gaussianity, validating a theoretical model against simulations and analyzing the practical advantages of the marked power spectrum.
Findings
Marked power spectrum constrains primordial non-Gaussianity effectively in certain regimes.
Performance for discrete tracers with BOSS-like densities does not surpass traditional P+B analysis at mildly non-linear scales.
Marked statistics offer practical benefits like simpler estimation and systematic control.
Abstract
The marked power spectrum - a two-point correlation function of a transformed density field - has emerged as a promising tool for extracting cosmological information from the large-scale structure of the Universe. In this work, we present the first comprehensive analytical study of the marked power spectrum's sensitivity to primordial non-Gaussianity (PNG) of the non-local type. We extend previous effective field theory frameworks to incorporate PNG, developing a complete theoretical model that we validate against the Quijote simulation suite. Through a systematic Fisher analysis, we compare the constraining power of the marked power spectrum against traditional approaches combining the power spectrum and bispectrum (P+B). We explore different choices of mark parameters to evaluate their impact on parameter constraints, particularly focusing on equilateral and orthogonal PNG as well as…
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