Towards self-consistent models for Inflation and Early Universe Cosmology

TL;DR

This thesis explores models linking the early universe's inflationary period with particle physics, proposing new mechanisms for inflation, dark matter, and dark energy within a unified framework.

Contribution

It introduces novel inflationary models with symmetries that stabilize potentials and connect dark matter production to early universe dynamics.

Findings

Successful Higgs inflation without large non-minimal coupling

Dark matter produced during preheating in twin waterfall models

Reproduction of observed dark matter abundance via axion kinetic misalignment

Abstract

In this PhD thesis we take smalls steps towards linking our knowledge of the Early Universe with our knowledge of particle physics. Chapters 3, 4 and 5 deal with Higgs inflation UV completions and their phenomenology. In Chapter 6 we consider a model for natural inflation with twin waterfalls, in which a Z2 symmetry is responsible for the radiative stability of the potential. Including a separate Z2' symmetry allows us to identify one of the waterfall fields with Dark Matter, that can be sufficiently produced during preheating. In Chapter 7, we take conformal couplings and expand around the pole of the Einstein-frame kinetic term. Using this structure we can recover successful Higgs inflation without the need of a large non-minimal coupling. Finally, in Chapter 8 we apply the setup to the Peccei-Quinn field responsible for the axion solution the Strong CP problem, and reproduce the observed Dark Matter relic abundance through the axion kinetic misalignment mechanism.