Cosmological Predictions from the Primordial Universe: Non-Gaussianities

TL;DR

This paper reviews the theoretical basis of non-Gaussianities in the early universe and uses Planck 2015 data to constrain inflationary models, focusing on their non-Gaussian signatures.

Contribution

It provides a comprehensive review of non-Gaussianity from first principles and applies observational constraints to non-standard inflationary models.

Findings

Planck data constrains non-Gaussianity parameters.

Non-Bunch-Davis initial states produce distinct non-Gaussian signatures.

Certain inflationary models are disfavored by the data.

Abstract

Non-Gaussian statistics in the distribution of large scale structure, and in temperature fluctuations of the cosmic microwave background, can be used to constrain inflationary models. Data on the cosmic microwave background from Planck (2015) is able to provide up-to-date bounds on parameters controlling the degree of non-Gaussianity in given models of inflation, thus favouring or disfavouring certain models. Starting from the statistics of random fields, this essay reviews non-Gaussianity from first principles, including Juan Maldacena's seminal calculation of non-Gaussianity in single-field, slow-roll inflation. Following this, models whereby the initial quantum state of inflation is so-called non-Bunch-Davis is considered. The non-Gaussian signature produced by such models is quantified, and parameters controlling the degree of non-Gaussianity are constrained using data from Planck (2015).