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

Hirvonen, Joonas and Löfgren, Johan and Ramsey-Musolf, Michael J. and Schicho, Philipp and Tenkanen, Tuomas V. I. (2022) Computing the gauge-invariant bubble nucleation rate in finite temperature effective field theory. Journal of High Energy Physics, 2022 (7). Art. No. 135. ISSN 1029-8479. doi:10.1007/jhep07(2022)135. https://resolver.caltech.edu/CaltechAUTHORS:20220726-997404000

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Abstract

A gauge-invariant framework for computing bubble nucleation rates at finite temperature in the presence of radiative barriers was presented and advocated for model-building and phenomenological studies in an accompanying article [1]. Here, we detail this computation using the Abelian Higgs Model as an illustrative example. Subsequently, we recast this approach in the dimensionally-reduced high-temperature effective field theory for nucleation. This allows for including several higher order thermal resummations and furthermore delineate clearly the approach’s limits of validity. This approach provides for robust perturbative treatments of bubble nucleation during possible first-order cosmic phase transitions, with implications for electroweak baryogenesis and production of a stochastic gravitational wave background. Furthermore, it yields a sound comparison between results of perturbative and non-perturbative computations.


Item Type:Article
Related URLs:
URLURL TypeDescription
https://doi.org/10.1007/JHEP07(2022)135DOIArticle
https://arxiv.org/abs/2112.08912arXivDiscussion Paper
ORCID:
AuthorORCID
Ramsey-Musolf, Michael J.0000-0001-8110-2479
Schicho, Philipp0000-0001-5869-7611
Additional Information:© 2022 The Authors. This article is distributed under the terms of the Creative Commons Attribution License (CC-BY 4.0), which permits any use, distribution and reproduction in any medium, provided the original author(s) and source are credited. Received 24 January 2022. Revised 06 June 2022. Accepted 08 June 2022. Article funded by SCOAP3. We wish to thank Andreas Ekstedt, Oliver Gould and Anders Thomsen for enlightening discussions. Specially we thank Suntharan Arunasalam for his contributions at the early stage of this project. In addition, we thank the anonymous referee for pointing out the resummation scheme based on freedom to choose the 3d RG scale, in section 3.4. MJRM and TT are supported in part under National Science Foundation of China grant no. 19Z103010239. PS has been supported by the European Research Council, grant no. 725369, and by the Academy of Finland, grant no. 1322507.
Funders:
Funding AgencyGrant Number
National Natural Science Foundation of China19Z103010239
European Research Council (ERC)725369
Academy of Finland1322507
SCOAP3UNSPECIFIED
Subject Keywords:Effective Field Theories, Phase Transitions in the Early Universe, Thermal Field Theory
Issue or Number:7
DOI:10.1007/jhep07(2022)135
Record Number:CaltechAUTHORS:20220726-997404000
Persistent URL:https://resolver.caltech.edu/CaltechAUTHORS:20220726-997404000
Official Citation:Hirvonen, J., Löfgren, J., Ramsey-Musolf, M.J. et al. Computing the gauge-invariant bubble nucleation rate in finite temperature effective field theory. J. High Energ. Phys. 2022, 135 (2022). https://doi.org/10.1007/JHEP07(2022)135
Usage Policy:No commercial reproduction, distribution, display or performance rights in this work are provided.
ID Code:115852
Collection:CaltechAUTHORS
Deposited By: George Porter
Deposited On:27 Jul 2022 21:48
Last Modified:27 Jul 2022 21:48

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