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dc.contributor.authorBai, S.W.
dc.contributor.authorKoszorús, Á.
dc.contributor.authorHu, B.S.
dc.contributor.authorYang, X.F.
dc.contributor.authorBillowes, J.
dc.contributor.authorBinnersley, C.L.
dc.contributor.authorBissell, M.L.
dc.contributor.authorBlaum, K.
dc.contributor.authorCampbell, P.
dc.contributor.authorCheal, B.
dc.contributor.authorCocolios, T.E.
dc.contributor.authorde Groote, R.P.
dc.contributor.authorDevlin, C.S.
dc.contributor.authorFlanagan, K.T.
dc.contributor.authorGarcia Ruiz, R.F.
dc.contributor.authorHeylen, H.
dc.contributor.authorHolt, J.D.
dc.contributor.authorKanellakopoulos, A.
dc.contributor.authorKrämer, J.
dc.contributor.authorLagaki, V.
dc.contributor.authorMaaß, B.
dc.contributor.authorMalbrunot-Ettenauer, S.
dc.contributor.authorMiyagi, T.
dc.contributor.authorNeugart, R.
dc.contributor.authorNeyens, G.
dc.contributor.authorNörtershäuser, W.
dc.contributor.authorRodríguez, L.V.
dc.contributor.authorSommer, F.
dc.contributor.authorVernon, A.R.
dc.contributor.authorWang, S.J.
dc.contributor.authorWang, X.B.
dc.contributor.authorWilkins, S.G.
dc.contributor.authorXu, Z.Y.
dc.contributor.authorYuan, C.X.
dc.date.accessioned2022-05-04T09:44:20Z
dc.date.available2022-05-04T09:44:20Z
dc.date.issued2022
dc.identifier.citationBai, S.W., Koszorús, Á., Hu, B.S., Yang, X.F., Billowes, J., Binnersley, C.L., Bissell, M.L., Blaum, K., Campbell, P., Cheal, B., Cocolios, T.E., de Groote, R.P., Devlin, C.S., Flanagan, K.T., Garcia Ruiz, R.F., Heylen, H., Holt, J.D., Kanellakopoulos, A., Krämer, J., . . . Yuan, C.X. (2022). Electromagnetic moments of scandium isotopes and N = 28 isotones in the distinctive 0f7/2 orbit. <i>Physics Letters B</i>, <i>829</i>, Article 137064. <a href="https://doi.org/10.1016/j.physletb.2022.137064" target="_blank">https://doi.org/10.1016/j.physletb.2022.137064</a>
dc.identifier.otherCONVID_117769520
dc.identifier.urihttps://jyx.jyu.fi/handle/123456789/80881
dc.description.abstractThe electric quadrupole moment of 49Sc was measured by collinear laser spectroscopy at CERN-ISOLDE to be Qs=−0.159(8) eb, and a nearly tenfold improvement in precision was reached for the electromagnetic moments of 47,49Sc. The single-particle behavior and nucleon-nucleon correlations are investigated with the electromagnetic moments of Z=21 isotopes and N=28 isotones as valence neutrons and protons fill the distinctive 0f7/2 orbit, respectively, located between magic numbers, 20 and 28. The experimental data are interpreted with shell-model calculations using an effective interaction, and ab-initio valence-space in-medium similarity renormalization group calculations based on chiral interactions. These results highlight the sensitivity of nuclear electromagnetic moments to different types of nucleon-nucleon correlations, and establish an important benchmark for further developments of theoretical calculations.en
dc.format.mimetypeapplication/pdf
dc.language.isoeng
dc.publisherElsevier
dc.relation.ispartofseriesPhysics Letters B
dc.rightsCC BY 4.0
dc.subject.otherCollinear laser spectroscopy
dc.subject.otherElectromagnetic moments
dc.subject.otherNucleon-nucleon correlation
dc.subject.otherAb-initio calculation
dc.titleElectromagnetic moments of scandium isotopes and N = 28 isotones in the distinctive 0f7/2 orbit
dc.typearticle
dc.identifier.urnURN:NBN:fi:jyu-202205042543
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.volume829
dc.type.versionpublishedVersion
dc.rights.copyright© 2022 the Authors
dc.rights.accesslevelopenAccessfi
dc.subject.ysoydinfysiikka
dc.subject.ysoisotoopit
dc.subject.ysoskandium
dc.format.contentfulltext
jyx.subject.urihttp://www.yso.fi/onto/yso/p14759
jyx.subject.urihttp://www.yso.fi/onto/yso/p6387
jyx.subject.urihttp://www.yso.fi/onto/yso/p38599
dc.rights.urlhttps://creativecommons.org/licenses/by/4.0/
dc.relation.doi10.1016/j.physletb.2022.137064
jyx.fundinginformationWe acknowledge the support of the ISOLDE collaboration and technical teams and S. R. Stroberg for the imsrg++ code [64] used to perform VS-IMSRG calculations. This work was supported by the National Key R&D Program of China (Contract No. 2018YFA0404403), the National Natural Science Foundation of China (No:11875073, U1967201, 11775316); the BriX Research Program No. P7/12, FWO-Vlaanderen (Belgium), GOA 15/010 from KU Leuven; the UK Science and Technology Facilities Council grants ST/L005794/1 and ST/P004598/1; ERC Consolidator Grant No.648381 (FNPMLS); the NSF grant PHY-1068217, the BMBF Contract No. 05P18RDCIA; the Max-Planck Society, the Helmholtz International Center for FAIR (HIC for FAIR); the EU Horizon 2020 research and innovation programme through ENSAR2 (no. 654002), NSERC under grants SAPIN-2018-00027 and RGPAS-2018-522453 and the Arthur B. McDonald Canadian Astroparticle Physics Research Institute. TRIUMF receives funding via a contribution through the National Research Council of Canada and computations of VS-IMSRG were performed with an allocation of computing resources on the Cedar at WestGrid and Compute Canada.
dc.type.okmA1


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