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dc.contributor.authorKainulainen, Kimmo
dc.contributor.authorVenkatesan, Niyati
dc.date.accessioned2024-10-23T11:32:44Z
dc.date.available2024-10-23T11:32:44Z
dc.date.issued2024
dc.identifier.citationKainulainen, K., & Venkatesan, N. (2024). Systematic moment expansion for electroweak baryogenesis. <i>Journal of Cosmology and Astroparticle Physics</i>, <i>2024</i>(08), Article 058. <a href="https://doi.org/10.1088/1475-7516/2024/08/058" target="_blank">https://doi.org/10.1088/1475-7516/2024/08/058</a>
dc.identifier.otherCONVID_242677385
dc.identifier.urihttps://jyx.jyu.fi/handle/123456789/97650
dc.description.abstractWe present a systematic moment expansion for solving the semiclassical Boltzmann equations for electroweak baryogenesis. The expansion is developed in powers of adiabatic coordinate velocity, and it is used for computing the CP-violating seed asymmetry at the front of the phase transition wall, that sources the eventual baryon asymmetry of the universe (BAU). We implement the method in a benchmark model, with a CP-violating mass arising from a dimension-5 operator coupling the fermion to a singlet scalar field. We find that the higher moment calculations yield a BAU that can significantly differ from the commonly used two-moment approximation. We discuss in detail the underlying approximations in the moment method and propose a new truncation scheme for the expansion, that appears to give more numerically robust results than the previous schemes.en
dc.format.mimetypeapplication/pdf
dc.language.isoeng
dc.publisherIOP Publishing
dc.relation.ispartofseriesJournal of Cosmology and Astroparticle Physics
dc.rightsCC BY 4.0
dc.subject.otherbaryon asymmetry
dc.subject.otherparticle physics
dc.subject.othercosmology connection
dc.subject.othercosmological phase transitions
dc.subject.otherphysics of the early universe
dc.titleSystematic moment expansion for electroweak baryogenesis
dc.typeresearch article
dc.identifier.urnURN:NBN:fi:jyu-202410236507
dc.contributor.laitosFysiikan laitosfi
dc.contributor.laitosMatemaattis-luonnontieteellinen tiedekuntafi
dc.contributor.laitosDepartment of Physicsen
dc.contributor.laitosFaculty of Mathematics and Scienceen
dc.type.urihttp://purl.org/eprint/type/JournalArticle
dc.type.coarhttp://purl.org/coar/resource_type/c_2df8fbb1
dc.description.reviewstatuspeerReviewed
dc.relation.issn1475-7516
dc.relation.numberinseries08
dc.relation.volume2024
dc.type.versionpublishedVersion
dc.rights.copyright© 2024 The Author(s). Published by IOP Publishing Ltd on behalf of Sissa Medialab.
dc.rights.accesslevelopenAccessfi
dc.type.publicationarticle
dc.subject.ysobaryogeneesi
dc.subject.ysohiukkasfysiikka
dc.subject.ysosähköheikko faasimuutos
dc.subject.ysokosmologia
dc.subject.ysomaailmankaikkeus
dc.format.contentfulltext
jyx.subject.urihttp://www.yso.fi/onto/yso/p40086
jyx.subject.urihttp://www.yso.fi/onto/yso/p15576
jyx.subject.urihttp://www.yso.fi/onto/yso/p39599
jyx.subject.urihttp://www.yso.fi/onto/yso/p7160
jyx.subject.urihttp://www.yso.fi/onto/yso/p4403
dc.rights.urlhttps://creativecommons.org/licenses/by/4.0/
dc.relation.doi10.1088/1475-7516/2024/08/058
jyx.fundinginformationNV was supported by grants from the Magnus Ehrnrooth Foundation, the Ellen and Artturi Nyyssönen Foundation, the Vilho, Yrjö and Kalle Väisälä Foundation and the University of Jyväskylä Postgraduate School.
dc.type.okmA1


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