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dc.contributor.authorMarkkanen, Tommi
dc.contributor.authorNurmi, Sami
dc.contributor.authorRajantie, Arttu
dc.contributor.authorStopyra, Stephen
dc.date.accessioned2018-06-27T05:53:03Z
dc.date.available2018-06-27T05:53:03Z
dc.date.issued2018fi
dc.identifier.citationMarkkanen, T., Nurmi, S., Rajantie, A., & Stopyra, S. (2018). The 1-loop effective potential for the Standard Model in curved spacetime. <em>Journal of High Energy Physics</em>, 2018 (6), 40. <a href="https://doi.org/10.1007/JHEP06(2018)040">doi:10.1007/JHEP06(2018)040</a>fi
dc.identifier.otherTUTKAID_78087
dc.identifier.urihttps://jyx.jyu.fi/handle/123456789/58737
dc.description.abstractThe renormalisation group improved Standard Model effective potential in an arbitrary curved spacetime is computed to one loop order in perturbation theory. The loop corrections are computed in the ultraviolet limit, which makes them independent of the choice of the vacuum state and allows the derivation of the complete set of β-functions. The potential depends on the spacetime curvature through the direct non-minimal Higgs-curvature coupling, curvature contributions to the loop diagrams, and through the curvature dependence of the renormalisation scale. Together, these lead to significant curvature dependence, which needs to be taken into account in cosmological applications, which is demonstrated with the example of vacuum stability in de Sitter space.fi
dc.format.mimetypeapplication/pdf
dc.language.isoeng
dc.publisherSpringer
dc.relation.ispartofseriesJournal of High Energy Physics
dc.rightsCC BY 4.0
dc.subject.otherkosmologiafi
dc.subject.othergravitaatiofi
dc.subject.otherhiukkasfysiikan standardimallifi
dc.subject.otherclassical theories of gravityfi
dc.subject.otherfield theories in higher dimensionsfi
dc.subject.otherfield theories in lower dimensionsfi
dc.titleThe 1-loop effective potential for the Standard Model in curved spacetimefi
dc.typearticle
dc.identifier.urnURN:NBN:fi:jyu-201806263364
dc.contributor.laitosFysiikan laitosfi
dc.contributor.laitosDepartment of Physicsen
dc.type.urihttp://purl.org/eprint/type/JournalArticle
dc.date.updated2018-06-26T09:15:13Z
dc.description.reviewstatuspeerReviewed
dc.relation.issn1126-6708
dc.relation.numberinseries6
dc.relation.volume2018
dc.type.versionpublishedVersion
dc.rights.copyright© Authors, 2018
dc.rights.accesslevelopenAccessfi
dc.format.contentfulltext
dc.rights.urlhttps://creativecommons.org/licenses/by/4.0/
dc.relation.doi10.1007/JHEP06(2018)040


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