
TL;DR
This paper employs an Effective Field Theory framework to compute and analyze the correlation functions of primordial fluctuations in a quasi de Sitter universe, connecting theoretical predictions with CMB observations.
Contribution
It introduces a systematic EFT approach to calculate scalar and tensor correlations for arbitrary initial vacua, linking EFT coefficients to inflationary parameters and observational data.
Findings
Computed two-point and three-point correlations in EFT framework.
Constrained EFT operator coefficients using Planck CMB data.
Validated EFT predictions against canonical single-field models.
Abstract
In this work, we study the key role of generic Effective Field Theory (EFT) framework to quantify the correlation functions in a quasi de Sitter background for an arbitrary initial choice of the quantum vacuum state. We perform the computation in unitary gauge, in which we apply the Stckelberg trick in lowest dimensional EFT operators which are broken under time diffeomorphism. In particular, using this non-linear realization of broken time diffeomorphism and truncating the action by considering the contribution from two derivative terms in the metric, we compute the two-point and three-point correlations from scalar perturbations and two-point correlation from tensor perturbations to quantify the quantum fluctuations observed in the Cosmic Microwave Background (CMB) map. We also use equilateral limit and squeezed limit configurations for the scalar three-point…
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