A non-perturbative framework for N-point functions of locally non-Gaussian fields
arXiv:2602.10151 · doi:10.1088/1475-7516/2026/06/001
Abstract
We present a non-perturbative approach to correlation functions and polyspectra of locally non-Gaussian fields and develop a semi-perturbative framework that does not rely on a local expansion. This enables the computation of -point functions of non-Gaussian fields even when the mapping between the auxiliary Gaussian field and the non-Gaussian field is non-analytic. As an example, we consider non-Gaussian fields with exponentially tailed distributions, which can arise, for instance, in ultra-slow-roll models of inflation, and derive some exact analytic results in the strongly non-Gaussian regime.
26 pages, 6 figures. Figures 5 and 6 updated and section 4 extended. Matches the version published in JCAP
References in corpus (9)
- Primordial Black Holes as Dark Matter
- Primordial Black Holes as Dark Matter: Recent Developments
- Gravitational Wave Spectrum Induced by Primordial Scalar Perturbations
- The cosmological gravitational wave background from primordial density perturbations
- The recent gravitational wave observation by pulsar timing arrays and primordial black holes: the importance of non-gaussianities
- Stochastic constant-roll inflation and primordial black holes
- Ultra-Slow-Roll Inflation on the Lattice I: Backreaction and Nonlinear Effects
- Primordial black holes: constraints, potential evidence and prospects
- Ultra-Slow-Roll Inflation on the Lattice II: Nonperturbative Curvature Perturbation