Maximal temperature of strongly-coupled dark sectors

DOI10.1007/JHEP05(2023)239arXiv2303.17973MaRDI QIDQ6105345

S. Procacci, Mikko Laine, Helena Kolešová

Publication date: 26 June 2023

Published in: Journal of High Energy Physics (Search for Journal in Brave)

Full work available at URL: https://arxiv.org/abs/2303.17973

zbMATH Keywords

thermal field theorycosmology of theories BSMphase transitions in the early universeearly universe particle physics

Mathematics Subject Classification ID

Quantum theory (81-XX) Relativity and gravitational theory (83-XX)

Cites Work

• The sphaleron rate in SU(\(N\)) gauge theory
• Dark matter and standard model reheating from conformal GUT inflation
• Shape of the hot topological charge density spectral function
• The sphaleron rate from 4D Euclidean lattices
• Minimal warm inflation with complete medium response
• Warming up cold inflation
• Turn up the volume: listening to phase transitions in hot dark sectors
• Effect of density fluctuations on gravitational wave production in first-order phase transitions
• Gravitational wave background from non-Abelian reheating after axion-like inflation
• Gravitational wave background from vacuum and thermal fluctuations during axion-like inflation
• Reconstructing the thermal Green functions at real times from those at imaginary times

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