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December 5, 2025Journal of High Energy Physics2 citationsOpen Access

On pre-inflationary non Gaussianities

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MMM. MeoASA. Sagnotti

Key Points

  • Initial singularity may be replaced by a bounce, indicating a significant shift in understanding early universe cosmology.
  • Identified through three-point amplitudes, the analysis of curvature perturbations highlights implications for the angular power spectrum of the CMB.
  • The approach uses assumptions from String Theory to evaluate contributions to non-Gaussian signals, providing insights into inflation dynamics.
  • Findings may align with Planck constraints, suggesting observable effects tied to the turning point during inflation.

Abstract

A bstract We explore the three-point amplitude of curvature perturbations in scenarios suggested by high-scale supersymmetry breaking in String Theory, where the inflaton is forced to climb a steep exponential potential. We can do it at the price of some simplifications, and more importantly with some assumptions on the softening effects of String Theory. These suggest a scenario proposed long ago by Gasperini and Veneziano, where the initial singularity is replaced by a bounce, and the resulting analysis rests on a scale ∆ that leaves some signs in the angular power spectrum of the CMB. The amplitude comprises two types of contribution: the first oscillates around the original result of Maldacena and gives no further prospects to detect a non-Gaussian signal, but the second, which is subtly tied to the turning point at the end of the climbing phase, within the window 62 < N < 66 for the inflationary e -folds could be compatible with Planck constraints and potentially observable. The amplitudes involving the tensor modes contain only the first type of contribution.

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Cite This Study

Meo et al. (2025) studied this question.

synapsesocial.com/papers/6932311e8e51979591dce3ffhttps://doi.org/10.1007/jhep12(2025)016
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