Infrared Behavior of Quantum Fields in Inflationary Cosmology -- Issues and Approaches: an overview
Bei-Lok Hu

TL;DR
This paper provides a comprehensive overview of the various approaches to studying the infrared behavior of quantum fields during inflation, clarifying their connections and guiding new researchers in the field.
Contribution
It synthesizes three main research approaches—Euclidean, Lorentzian, and stochastic methods—highlighting their interrelations and recent developments in inflationary quantum field theory.
Findings
Clarifies the connections between different theoretical approaches
Summarizes recent advances and future research directions
Serves as an educational resource for newcomers
Abstract
This is a pedagogical guide to works on this subject which began in the 80s but has seen vibrant activities in the last decade. It aims to help orient readers, especially students, who wish to enter into research but bewildered by the vast and diverse literature on this subject. We describe the three main veins of activities: the Euclidean zero-mode dominance, the Lorentzian interacting quantum field theory and the classical stochastic field theory approaches in some detail, explaining the underlying physics and the technicalities of each. We show how these approaches are interconnected, and highlight recent papers which contain germs of worthy directions for future developments.
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Taxonomy
TopicsCosmology and Gravitation Theories · Black Holes and Theoretical Physics · Relativity and Gravitational Theory
