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dc.contributor.authorde Groote, R. P.
dc.contributor.authorKujanpää, S.
dc.contributor.authorKoszorús, Á.
dc.contributor.authorLi, J. G.
dc.contributor.authorMoore, I. D.
dc.date.accessioned2021-05-05T07:04:16Z
dc.date.available2021-05-05T07:04:16Z
dc.date.issued2021
dc.identifier.citationde Groote, R. P., Kujanpää, S., Koszorús, Á., Li, J. G., & Moore, I. D. (2021). Magnetic octupole moment of 173Yb using collinear laser spectroscopy. <i>Physical Review A</i>, <i>103</i>(3), Article 032826. <a href="https://doi.org/10.1103/PhysRevA.103.032826" target="_blank">https://doi.org/10.1103/PhysRevA.103.032826</a>
dc.identifier.otherCONVID_68758860
dc.identifier.urihttps://jyx.jyu.fi/handle/123456789/75306
dc.description.abstractThe hyperfine constants of the 4f146s6p3Po2 state in neutral Yb have been measured using three different dipole transitions. This state was recently shown to have a comparatively large hyperfine magnetic octupole splitting, and thus a puzzlingly large magnetic octupole moment. The measurement is performed using collinear laser spectroscopy on a fast atomic beam, which provides a straightforward route to probing long-lived metastable atomic states with high resolution. From the combined analysis of all three lines we find no significant evidence for a nonzero octupole moment in 173Yb.en
dc.format.mimetypeapplication/pdf
dc.language.isoeng
dc.publisherAmerican Physical Society (APS)
dc.relation.ispartofseriesPhysical Review A
dc.rightsIn Copyright
dc.titleMagnetic octupole moment of 173Yb using collinear laser spectroscopy
dc.typearticle
dc.identifier.urnURN:NBN:fi:jyu-202105052620
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.issn2469-9926
dc.relation.numberinseries3
dc.relation.volume103
dc.type.versionpublishedVersion
dc.rights.copyright©2021 American Physical Society
dc.rights.accesslevelopenAccessfi
dc.relation.grantnumber844829
dc.relation.grantnumber844829
dc.relation.projectidinfo:eu-repo/grantAgreement/EC/H2020/844829/EU//RAPTOR
dc.subject.ysoatomifysiikka
dc.subject.ysoydinfysiikka
dc.format.contentfulltext
jyx.subject.urihttp://www.yso.fi/onto/yso/p16034
jyx.subject.urihttp://www.yso.fi/onto/yso/p14759
dc.rights.urlhttp://rightsstatements.org/page/InC/1.0/?language=en
dc.relation.doi10.1103/PhysRevA.103.032826
dc.relation.funderEuropean Commissionen
dc.relation.funderEuroopan komissiofi
jyx.fundingprogramMSCA Individual Fellowship (IF)en
jyx.fundingprogramMSCA Individual Fellowship (IF)fi
jyx.fundinginformationR.P.D.G. received funding from the European Union's Horizon 2020 research and innovation programme under the Marie Skłodowska-Curie Grant Agreement No. 844829. J.G.L. acknowledges the support of the National Natural Science Foundation of China under Grant No. 11874090.
dc.type.okmA1


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