Cosmic inflation in a landscape of heavy-fields
Sebastian Cespedes, Gonzalo A. Palma

TL;DR
This paper investigates how multiple heavy-fields in a multi-dimensional inflation landscape influence curvature perturbations, extending previous single-field analyses, and derives an effective field theory revealing new self-interactions.
Contribution
It generalizes the effective field theory of curvature perturbations to include two heavy-fields, showing their significant impact on inflationary dynamics and potential observational constraints.
Findings
Two heavy-fields can significantly alter curvature perturbation evolution.
Additional self-interactions arise from the second heavy-field.
Future observations can constrain the number of interacting heavy-fields.
Abstract
Heavy isocurvature fields may have a strong influence on the low energy dynamics of curvature perturbations during inflation, as long as the inflationary trajectory becomes non-geodesic in the multi-field target space (the landscape). If fields orthogonal to the inflationary trajectory are sufficiently heavy, one expects a reliable effective field theory describing the low energy dynamics of curvature perturbations, with self-interactions determined by the shape of the inflationary trajectory. Previous work analyzing the role of heavy-fields during inflation have mostly focused in the effects on curvature perturbations due to a single heavy-field. In this article we extend the results of these works by studying models of inflation in which curvature perturbations interact with two heavy-fields. We show that the second heavy-field (orthogonal to both tangent and normal directions of the…
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