Dynamics of bubble walls at the electroweak phase transition

First order phase transitions in the early universe naturally lead to the production of a stochastic background of gravitational waves and to the generation of a matter-antimatter asymmetry. The dynamics of the phase transition is affected by the density perturbations in the hot plasma. We address t...

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Main Authors: De Curtis Stefania, Rose Luigi Delle, Guiggiani Andrea, Muyor Ángel Gil, Panico Giuliano
Format: Article
Language:English
Published: EDP Sciences 2022-01-01
Series:EPJ Web of Conferences
Online Access:https://www.epj-conferences.org/articles/epjconf/pdf/2022/14/epjconf_qcd@work2022_00035.pdf
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author De Curtis Stefania
Rose Luigi Delle
Guiggiani Andrea
Muyor Ángel Gil
Panico Giuliano
author_facet De Curtis Stefania
Rose Luigi Delle
Guiggiani Andrea
Muyor Ángel Gil
Panico Giuliano
author_sort De Curtis Stefania
collection DOAJ
description First order phase transitions in the early universe naturally lead to the production of a stochastic background of gravitational waves and to the generation of a matter-antimatter asymmetry. The dynamics of the phase transition is affected by the density perturbations in the hot plasma. We address this topic by providing, for the first time, a full numerical solution to the linearized Boltzmann equation for the top quark species coupled to the Higgs field during a first order phase transition at the electroweak scale. Differently from the traditional approaches, our results do not depend on any ansatz and can fully describe the non-equilibrium distribution functions of the particle species in the plasma.
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spelling doaj.art-c757c85428a846de864812d0f1ff03432022-12-22T04:18:36ZengEDP SciencesEPJ Web of Conferences2100-014X2022-01-012700003510.1051/epjconf/202227000035epjconf_qcd@work2022_00035Dynamics of bubble walls at the electroweak phase transitionDe Curtis Stefania0Rose Luigi Delle1Guiggiani Andrea2Muyor Ángel Gil3Panico Giuliano4INFN Sezione di Firenze and Dipartimento di Fisica e Astronomia, Università di FirenzeDipartimento di Fisica, Universit‘a della CalabriaINFN Sezione di Firenze and Dipartimento di Fisica e Astronomia, Università di FirenzeIFAE and BIST, Universitat Autònoma de BarcelonaINFN Sezione di Firenze and Dipartimento di Fisica e Astronomia, Università di FirenzeFirst order phase transitions in the early universe naturally lead to the production of a stochastic background of gravitational waves and to the generation of a matter-antimatter asymmetry. The dynamics of the phase transition is affected by the density perturbations in the hot plasma. We address this topic by providing, for the first time, a full numerical solution to the linearized Boltzmann equation for the top quark species coupled to the Higgs field during a first order phase transition at the electroweak scale. Differently from the traditional approaches, our results do not depend on any ansatz and can fully describe the non-equilibrium distribution functions of the particle species in the plasma.https://www.epj-conferences.org/articles/epjconf/pdf/2022/14/epjconf_qcd@work2022_00035.pdf
spellingShingle De Curtis Stefania
Rose Luigi Delle
Guiggiani Andrea
Muyor Ángel Gil
Panico Giuliano
Dynamics of bubble walls at the electroweak phase transition
EPJ Web of Conferences
title Dynamics of bubble walls at the electroweak phase transition
title_full Dynamics of bubble walls at the electroweak phase transition
title_fullStr Dynamics of bubble walls at the electroweak phase transition
title_full_unstemmed Dynamics of bubble walls at the electroweak phase transition
title_short Dynamics of bubble walls at the electroweak phase transition
title_sort dynamics of bubble walls at the electroweak phase transition
url https://www.epj-conferences.org/articles/epjconf/pdf/2022/14/epjconf_qcd@work2022_00035.pdf
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AT guiggianiandrea dynamicsofbubblewallsattheelectroweakphasetransition
AT muyorangelgil dynamicsofbubblewallsattheelectroweakphasetransition
AT panicogiuliano dynamicsofbubblewallsattheelectroweakphasetransition