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Perturbative effective field theory expansions for cosmological phase transitions
School of Physics and Astronomy, University of Nottingham, University Park, Nottingham, NG7 2RD, UK.
Nordita, SU.
2024 (English)In: Journal of High Energy Physics (JHEP), ISSN 1126-6708, E-ISSN 1029-8479, Vol. 2024, no 1, article id 48Article in journal (Refereed) Published
Abstract [en]

Guided by previous non-perturbative lattice simulations of a two-step electroweak phase transition, we reformulate the perturbative analysis of equilibrium thermodynamics for generic cosmological phase transitions in terms of effective field theory (EFT) expansions. Based on thermal scale hierarchies, we argue that the scale of many interesting phase transitions is in-between the soft and ultrasoft energy scales, which have been the focus of studies utilising high-temperature dimensional reduction. The corresponding EFT expansions provide a handle to control the perturbative expansion, and allow us to avoid spurious infrared divergences, imaginary parts, gauge dependence and renormalisation scale dependence that have plagued previous studies. As a direct application, we present a novel approach to two-step electroweak phase transitions, by constructing separate effective descriptions for two consecutive transitions. Our approach provides simple expressions for effective potentials separately in different phases, a numerically inexpensive method to determine thermodynamics, and significantly improves agreement with the non-perturbative lattice simulations.

Place, publisher, year, edition, pages
Springer Nature , 2024. Vol. 2024, no 1, article id 48
Keywords [en]
Cosmology of Theories BSM, Early Universe Particle Physics, Multi-Higgs Models, Phase Transitions in the Early Universe
National Category
Subatomic Physics
Identifiers
URN: urn:nbn:se:kth:diva-342380DOI: 10.1007/JHEP01(2024)048ISI: 001141541500002Scopus ID: 2-s2.0-85181952999OAI: oai:DiVA.org:kth-342380DiVA, id: diva2:1828892
Note

QC 20240122

Available from: 2024-01-17 Created: 2024-01-17 Last updated: 2024-02-06Bibliographically approved

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