dc.contributor.author | Kainulainen, Kimmo | |
dc.contributor.author | Venkatesan, Niyati | |
dc.date.accessioned | 2024-10-23T11:32:44Z | |
dc.date.available | 2024-10-23T11:32:44Z | |
dc.date.issued | 2024 | |
dc.identifier.citation | Kainulainen, 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.other | CONVID_242677385 | |
dc.identifier.uri | https://jyx.jyu.fi/handle/123456789/97650 | |
dc.description.abstract | We 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.mimetype | application/pdf | |
dc.language.iso | eng | |
dc.publisher | IOP Publishing | |
dc.relation.ispartofseries | Journal of Cosmology and Astroparticle Physics | |
dc.rights | CC BY 4.0 | |
dc.subject.other | baryon asymmetry | |
dc.subject.other | particle physics | |
dc.subject.other | cosmology connection | |
dc.subject.other | cosmological phase transitions | |
dc.subject.other | physics of the early universe | |
dc.title | Systematic moment expansion for electroweak baryogenesis | |
dc.type | research article | |
dc.identifier.urn | URN:NBN:fi:jyu-202410236507 | |
dc.contributor.laitos | Fysiikan laitos | fi |
dc.contributor.laitos | Matemaattis-luonnontieteellinen tiedekunta | fi |
dc.contributor.laitos | Department of Physics | en |
dc.contributor.laitos | Faculty of Mathematics and Science | en |
dc.type.uri | http://purl.org/eprint/type/JournalArticle | |
dc.type.coar | http://purl.org/coar/resource_type/c_2df8fbb1 | |
dc.description.reviewstatus | peerReviewed | |
dc.relation.issn | 1475-7516 | |
dc.relation.numberinseries | 08 | |
dc.relation.volume | 2024 | |
dc.type.version | publishedVersion | |
dc.rights.copyright | © 2024 The Author(s). Published by IOP Publishing Ltd on behalf of Sissa Medialab. | |
dc.rights.accesslevel | openAccess | fi |
dc.type.publication | article | |
dc.subject.yso | baryogeneesi | |
dc.subject.yso | hiukkasfysiikka | |
dc.subject.yso | sähköheikko faasimuutos | |
dc.subject.yso | kosmologia | |
dc.subject.yso | maailmankaikkeus | |
dc.format.content | fulltext | |
jyx.subject.uri | http://www.yso.fi/onto/yso/p40086 | |
jyx.subject.uri | http://www.yso.fi/onto/yso/p15576 | |
jyx.subject.uri | http://www.yso.fi/onto/yso/p39599 | |
jyx.subject.uri | http://www.yso.fi/onto/yso/p7160 | |
jyx.subject.uri | http://www.yso.fi/onto/yso/p4403 | |
dc.rights.url | https://creativecommons.org/licenses/by/4.0/ | |
dc.relation.doi | 10.1088/1475-7516/2024/08/058 | |
jyx.fundinginformation | NV 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.okm | A1 | |