Higher N-point function data analysis techniques for heavy particle production and WMAP results
Moritz M\"unchmeyer, Kendrick M. Smith

TL;DR
This paper develops methods for analyzing higher-order N-point correlation functions in cosmological data to detect signatures of heavy particle production during inflation, extending beyond traditional bispectrum and trispectrum analyses.
Contribution
It introduces estimators for arbitrary N-point functions, explores their properties, and demonstrates their application to WMAP data, highlighting new discovery potential in non-Gaussianity analysis.
Findings
Derived estimators for arbitrary N-point functions.
Showed heavy particle production reduces to a Poisson process.
Initial WMAP data analysis illustrates higher N-point function search complexities.
Abstract
We explore data analysis techniques for signatures from heavy particle production during inflation. Heavy particules can be produced by time dependent masses and couplings, which are ubiquitous in string theory. These localized excitations induce curvature perturbations with non-zero correlation functions at all orders. In particular, Flauger et. al. 2016 has shown that the signal-to-noise as a function of the order of the correlation function can peak for of order to for an interesting space of models. As previous non-Gaussianity analyses have focused on , in principle this provides an unexplored data analysis window with new discovery potential. We derive estimators for arbitrary -point functions in this model and discuss their properties and covariances. To lowest order, the heavy particle production phenomenology reduces to a…
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