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dc.contributor.authorSommer, Felix
dc.contributor.authorKönig, Kristian
dc.contributor.authorRossi, Dominic M.
dc.contributor.authorEverett, Nathan
dc.contributor.authorGarand, David
dc.contributor.authorde Groote, Ruben P.
dc.contributor.authorHolt, Jason D.
dc.contributor.authorImgram, Phillip
dc.contributor.authorIncorvati, Anthony
dc.contributor.authorKalman, Colton
dc.contributor.authorKlose, Andrew
dc.contributor.authorLantis, Jeremy
dc.contributor.authorLiu, Yuan
dc.contributor.authorMiller, Andrew J.
dc.contributor.authorMinamisono, Kei
dc.contributor.authorMiyagi, Takayuki
dc.contributor.authorNazarewicz, Witold
dc.contributor.authorNörtershäuser, Wilfried
dc.contributor.authorPineda, Skyy V.
dc.contributor.authorPowel, Robert
dc.contributor.authorReinhard, Paul-Gerhard
dc.contributor.authorRenth, Laura
dc.contributor.authorRomero-Romero, Elisa
dc.contributor.authorRoth, Robert
dc.contributor.authorSchwenk, Achim
dc.contributor.authorSumithrarachchi, Chandana
dc.contributor.authorTeigelhöfer, Andrea
dc.date.accessioned2022-11-02T06:46:52Z
dc.date.available2022-11-02T06:46:52Z
dc.date.issued2022
dc.identifier.citationSommer, F., König, K., Rossi, D. M., Everett, N., Garand, D., de Groote, R. P., Holt, J. D., Imgram, P., Incorvati, A., Kalman, C., Klose, A., Lantis, J., Liu, Y., Miller, A. J., Minamisono, K., Miyagi, T., Nazarewicz, W., Nörtershäuser, W., Pineda, S. V., . . . Teigelhöfer, A. (2022). Charge Radii of 55,56Ni Reveal a Surprisingly Similar Behavior at N=28 in Ca and Ni Isotopes. <i>Physical Review Letters</i>, <i>129</i>(13), Article 132501. <a href="https://doi.org/10.1103/PhysRevLett.129.132501" target="_blank">https://doi.org/10.1103/PhysRevLett.129.132501</a>
dc.identifier.otherCONVID_159319080
dc.identifier.urihttps://jyx.jyu.fi/handle/123456789/83764
dc.description.abstractNuclear charge radii of 55,56Ni were measured by collinear laser spectroscopy. The obtained information completes the behavior of the charge radii at the shell closure of the doubly magic nucleus 56Ni. The trend of charge radii across the shell closures in calcium and nickel is surprisingly similar despite the fact that the 56Ni core is supposed to be much softer than the 48Ca core. The very low magnetic moment μ(55Ni)=−1.108(20) μN indicates the impact of M1 excitations between spin-orbit partners across the N,Z=28 shell gaps. Our charge-radii results are compared to ab initio and nuclear density functional theory calculations, showing good agreement within theoretical uncertainties.en
dc.format.mimetypeapplication/pdf
dc.language.isoeng
dc.publisherAmerican Physical Society (APS)
dc.relation.ispartofseriesPhysical Review Letters
dc.rightsIn Copyright
dc.titleCharge Radii of 55,56Ni Reveal a Surprisingly Similar Behavior at N=28 in Ca and Ni Isotopes
dc.typearticle
dc.identifier.urnURN:NBN:fi:jyu-202211025069
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.issn0031-9007
dc.relation.numberinseries13
dc.relation.volume129
dc.type.versionpublishedVersion
dc.rights.copyright© 2022 American Physical Society
dc.rights.accesslevelopenAccessfi
dc.subject.ysonikkeli
dc.subject.ysokalsium
dc.subject.ysoydinfysiikka
dc.format.contentfulltext
jyx.subject.urihttp://www.yso.fi/onto/yso/p19926
jyx.subject.urihttp://www.yso.fi/onto/yso/p1852
jyx.subject.urihttp://www.yso.fi/onto/yso/p14759
dc.rights.urlhttp://rightsstatements.org/page/InC/1.0/?language=en
dc.relation.doi10.1103/PhysRevLett.129.132501
jyx.fundinginformationThis work was supported in part by the Deutsche Forschungsgemeinschaft (DFG, German Research Foundation)—Project-ID 279384907—SFB 1245, by the U.S. Department of Energy, Office of Science, Office of Nuclear Physics under Awards No. DE-SC0013365 and No. DE-SC0018083 (NUCLEI SciDAC-4 Collaboration), by the National Science Foundation under Grants No. PHY 19-13509, No. PHY-15-65546, and No. PHY-21-11185, and by NSERC under Grants No. SAPIN-2018-00027 and No. RGPAS-2018-522453. TRIUMF receives funding via a contribution through the National Research Council of Canada. Computations of VS-IMSRG were performed with an allocation of computing resources on Cedar at WestGrid and Compute Canada. We also thank the RRZE computing center of the Friedrich-Alexander University Erlangen–Nürnberg for supplying resources for this work.
dc.type.okmA1


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