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dc.contributor.authorShaposhnikov, Mikhail
dc.contributor.authorTokareva, Anna
dc.date.accessioned2023-04-19T11:44:53Z
dc.date.available2023-04-19T11:44:53Z
dc.date.issued2023
dc.identifier.citationShaposhnikov, M., & Tokareva, A. (2023). Anomaly-free scale symmetry and gravity. <i>Physics Letters B</i>, <i>840</i>, Article 137898. <a href="https://doi.org/10.1016/j.physletb.2023.137898" target="_blank">https://doi.org/10.1016/j.physletb.2023.137898</a>
dc.identifier.otherCONVID_182735474
dc.identifier.urihttps://jyx.jyu.fi/handle/123456789/86452
dc.description.abstractIn this Letter, we address the question of whether the conformal invariance can be considered as a global symmetry of a theory of fundamental interactions. To describe Nature, this theory must contain a mechanism of spontaneous breaking of the scale symmetry. Besides that, the fundamental theory must include gravity, whereas all known extensions of the conformal invariance to the curved space-time suffer from the Weyl anomaly. We show that conformal symmetry can be made free from quantum anomaly only in flat space. The presence of gravity would reduce the global symmetry group of the fundamental theory to the scale invariance only. We discuss how the effective Lagrangian respecting the scale symmetry can be used for the description of particle phenomenology and cosmology.en
dc.format.mimetypeapplication/pdf
dc.language.isoeng
dc.publisherElsevier BV
dc.relation.ispartofseriesPhysics Letters B
dc.rightsCC BY 4.0
dc.titleAnomaly-free scale symmetry and gravity
dc.typearticle
dc.identifier.urnURN:NBN:fi:jyu-202304192571
dc.contributor.laitosFysiikan laitosfi
dc.contributor.laitosDepartment of Physicsen
dc.type.urihttp://purl.org/eprint/type/JournalArticle
dc.type.coarhttp://purl.org/coar/resource_type/c_2df8fbb1
dc.description.reviewstatuspeerReviewed
dc.relation.issn0370-2693
dc.relation.volume840
dc.type.versionpublishedVersion
dc.rights.copyright© 2023 the Authors
dc.rights.accesslevelopenAccessfi
dc.relation.grantnumber318319
dc.subject.ysoperusvuorovaikutukset
dc.subject.ysokosmologia
dc.subject.ysogravitaatio
dc.subject.ysosymmetria
dc.format.contentfulltext
jyx.subject.urihttp://www.yso.fi/onto/yso/p29742
jyx.subject.urihttp://www.yso.fi/onto/yso/p7160
jyx.subject.urihttp://www.yso.fi/onto/yso/p1175
jyx.subject.urihttp://www.yso.fi/onto/yso/p15022
dc.rights.urlhttps://creativecommons.org/licenses/by/4.0/
dc.relation.doi10.1016/j.physletb.2023.137898
dc.relation.funderResearch Council of Finlanden
dc.relation.funderSuomen Akatemiafi
jyx.fundingprogramAcademy Project, AoFen
jyx.fundingprogramAkatemiahanke, SAfi
jyx.fundinginformationThis work was supported by ERC-AdG-2015 grant 694896 and by the Swiss National Science Foundation Excellence grant 200020B 182864. The work was also supported by the Academy of Finland grant 318319.
dc.type.okmA1


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