The Non-Minimal Ekpyrotic Trispectrum
Angelika Fertig, Jean-Luc Lehners

TL;DR
This paper develops a formalism to predict non-Gaussian features in multi-field ekpyrotic cosmological models, revealing that the conversion process induces detectable non-Gaussianity with distinctive negative trispectrum signatures.
Contribution
It derives third-order evolution equations for multi-field models with non-canonical kinetic terms and applies them to ekpyrotic scenarios, highlighting unique non-Gaussian signatures.
Findings
Entropy perturbations have negligible bi- and trispectra during ekpyrosis.
Conversion to curvature perturbations induces observable non-Gaussianity.
The trispectrum parameter g_{NL} is typically negative and large in magnitude.
Abstract
Employing the covariant formalism, we derive the evolution equations for two scalar fields with non-canonical field space metric up to third order in perturbation theory. These equations can be used to derive predictions for local bi- and trispectra of multi-field cosmological models. Our main application is to ekpyrotic models in which the primordial curvature perturbations are generated via the non-minimal entropic mechanism. In these models, nearly scale-invariant entropy perturbations are generated first due to a non-minimal kinetic coupling between two scalar fields, and subsequently these perturbations are converted into curvature perturbations. Remarkably, the entropy perturbations have vanishing bi- and trispectra during the ekpyrotic phase. However, as we show, the conversion process to curvature perturbations induces local non-Gaussianity parameters and at…
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