Non-Equilibrium Dynamics of Phase Transitions: From the Early Universe to Chiral Condensates
D. Boyanovsky, H.J. de Vega, R. Holman

TL;DR
This paper reviews quantum field theory methods for studying non-equilibrium phase transitions, focusing on early universe inflation, domain formation, and chiral condensate dynamics, with implications for cosmology and accelerator experiments.
Contribution
It introduces non-equilibrium techniques to analyze phase transition dynamics, including instabilities, domain formation, and fluctuations, in cosmological and particle physics contexts.
Findings
Instabilities significantly alter slow-roll phase transition models.
Dynamics of supercooled phase transitions are analyzed in Minkowski space.
Quantum and thermal fluctuations influence chiral condensate formation.
Abstract
In this brief review we introduce the methods of quantum field theory out of equilibrium and study the non-equilibrium aspects of phase transitions. Specifically we critically study the picture of the ``slow-roll'' phase transition in the new inflationary models, we show that the instabilities that are the hallmark of the phase transition, that is the formation of correlated domains, dramatically change this picture. We analyze in detail the dynamics of phase separation in strongly supercooled phase transitions in Minkowski space. We argue that this is typically the situation in weakly coupled scalar theories. The effective evolution equations for the expectation value and the fluctuations of an inflaton field in a FRW cosmology are derived both in the loop expansion and in a self-consistent non-perturbative scheme. Finally we use these non-equilibrium techniques and concepts to study…
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Taxonomy
TopicsCosmology and Gravitation Theories · High-Energy Particle Collisions Research · Quantum, superfluid, helium dynamics
