
TL;DR
This paper derives model-independent consistency relations for non-Gaussianity in the early universe, applicable to various inflationary models, and extends these relations to higher-order correlation functions and loop corrections.
Contribution
It provides a dynamical proof of the consistency relation for 3-point functions and generalizes it to n-point functions and higher-order perturbations.
Findings
Consistency relation for 3-point correlation functions established.
Relations applicable to single and multi-field inflation, as well as curvaton scenarios.
Generalization to n-point functions and arbitrary loop orders achieved.
Abstract
We investigate consistency relations for non-Gaussianity. We provide a model-independent dynamical proof for the consistency relation of 3-point correlation functions from the Hamiltonian and field redefinition. This relation can be applied to single field inflation, multi-field inflation and the curvaton scenario. This relation can also be generalized to -point correlation functions up to arbitrary order in perturbation theory and with arbitrary number of loops.
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