Computing the gauge-invariant bubble nucleation rate in finite temperature effective field theory

DOI10.1007/JHEP07(2022)135MaRDI QIDQ2104684

Tuomas V. I. Tenkanen, Philipp Schicho, Joonas Hirvonen, Michael J. Ramsey-Musolf, Johan Löfgren

Publication date: 7 December 2022

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

Full work available at URL: https://arxiv.org/abs/2112.08912

zbMATH Keywords

thermal field theoryeffective field theoriesphase transitions in the early universe

Mathematics Subject Classification ID

Quantum theory (81-XX)

Related Items (5)

Bubble nucleation to all orders ⋮ \texttt{DRalgo}: a package for effective field theory approach for thermal phase transitions ⋮ Combining thermal resummation and gauge invariance for electroweak phase transition ⋮ Conformal model for gravitational waves and dark matter: a status update ⋮ \texttt{BubbleDet}: a Python package to compute functional determinants for bubble nucleation

Uses Software

• FORM
• CosmoTransitions
• FindBounce
• DRalgo

Cites Work

• Baryon washout, electroweak phase transition, and perturbation theory
• Strong electroweak phase transitions in the Standard Model with a singlet
• Perturbative thermal QCD: formalism and applications
• On the gauge invariance of the decay rate of false vacuum
• A New Approach to Quantum-Statistical Mechanics
• Supersymmetric phase transitions and gravitational waves at LISA
• Gravitational waves from a first-order electroweak phase transition: a brief review
• A fresh look at the calculation of tunneling actions
• Efficient numerical solution to vacuum decay with many fields
• A fresh look at the calculation of tunneling actions in multi-field potentials
• The Ising model universality of the electroweak theory
• The end point of the first-order phase transition of the SU(2) gauge-Higgs model on a four-dimensional isotropic lattice
• Where does the hot electroweak phase transition end?
• \texttt{FindBounce}: package for multi-field bounce actions
• An optimisation based algorithm for finding the nucleation temperature of cosmological phase transitions

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