Trans-Planckian enhancements of the primordial non-Gaussianities
Hael Collins (Niels Bohr International Academy), R. Holman, (Carnegie Mellon University)

TL;DR
This paper investigates how breaking Lorentz invariance at tiny scales can significantly enhance primordial non-Gaussianities, providing stronger constraints on trans-Planckian physics during inflation.
Contribution
It introduces a set of irrelevant operators preserving spatial symmetries that can amplify non-Gaussian signals beyond standard inflationary predictions.
Findings
Non-Gaussianities can be substantially larger than usual.
Enhanced non-Gaussianities lead to tighter constraints on trans-Planckian physics.
Study of irrelevant operators affecting primordial perturbations.
Abstract
This article examines how breaking a Lorentz-invariant description of nature at tiny space-time intervals would affect the non-Gaussian character of the pattern of primordial perturbations left by inflation. We specifically study a set of irrelevant operators that preserve the spatial symmetries of the usual inflationary background. The non-Gaussian component in the primordial fluctuations can be much larger than the usual, small, inflationary prediction and can thus lead to much stronger constraints on the role of "trans-Planckian" physics in inflation than those from the measurements of the primordial power spectrum.
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