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The spectroscopic quadrupole moment of the 21+ state of 12C : A benchmark of theoretical models

dc.contributor.authorSaiz-Lomas, J.
dc.contributor.authorPetri, M.
dc.contributor.authorLee, I. Y.
dc.contributor.authorSyndikus, I.
dc.contributor.authorHeil, S.
dc.contributor.authorAllmond, J. M.
dc.contributor.authorGaffney, L. P.
dc.contributor.authorPakarinen, J.
dc.contributor.authorBadran, H.
dc.contributor.authorCalverley, T.
dc.contributor.authorCox, D. M.
dc.contributor.authorForsberg, U.
dc.contributor.authorGrahn, T.
dc.contributor.authorGreenlees, P.
dc.contributor.authorHadyńska-Klȩk, K.
dc.contributor.authorHilton, J.
dc.contributor.authorJenkinson, M.
dc.contributor.authorJulin, R.
dc.contributor.authorKonki, J.
dc.contributor.authorMacchiavelli, A. O.
dc.contributor.authorMathy, M.
dc.contributor.authorOjala, J.
dc.contributor.authorPapadakis, P.
dc.contributor.authorPartanen, J.
dc.contributor.authorRahkila, P.
dc.contributor.authorRuotsalainen, P.
dc.contributor.authorSandzelius, M.
dc.contributor.authorSarén, J.
dc.contributor.authorStolze, S.
dc.contributor.authorUusitalo, J.
dc.contributor.authorWadsworth, R.
dc.date.accessioned2023-09-08T11:39:01Z
dc.date.available2023-09-08T11:39:01Z
dc.date.issued2023
dc.identifier.citationSaiz-Lomas, J., Petri, M., Lee, I. Y., Syndikus, I., Heil, S., Allmond, J. M., Gaffney, L. P., Pakarinen, J., Badran, H., Calverley, T., Cox, D. M., Forsberg, U., Grahn, T., Greenlees, P., Hadyńska-Klȩk, K., Hilton, J., Jenkinson, M., Julin, R., Konki, J., . . . Wadsworth, R. (2023). The spectroscopic quadrupole moment of the 21+ state of 12C : A benchmark of theoretical models. <i>Physics Letters B</i>, <i>845</i>, Article 138114. <a href="https://doi.org/10.1016/j.physletb.2023.138114" target="_blank">https://doi.org/10.1016/j.physletb.2023.138114</a>
dc.identifier.otherCONVID_184153445
dc.identifier.urihttps://jyx.jyu.fi/handle/123456789/89007
dc.description.abstractThe spectroscopic quadrupole moment of the first 2+ state of 12C has been measured employing the Coulomb-excitation re-orientation technique. Our result of Qs (2+ 1 ) = +9.3+3.5 −3.8 efm2 suggests a larger oblate deformation than previously reported. Combining this with the consistently re-analyzed adopted value, we present the most precise value to date of Qs(2+ 1 ) = +9.5(18) efm2, which is consistent with a geometrical rotor description. This simple outcome is compared to state-of-the-art shell-model, mean field, ab initio calculations, cluster-based and geometrical-like theories, which show varying degrees of emergent quadrupole collectivity.en
dc.format.mimetypeapplication/pdf
dc.language.isoeng
dc.publisherElsevier
dc.relation.ispartofseriesPhysics Letters B
dc.rightsCC BY 4.0
dc.titleThe spectroscopic quadrupole moment of the 21+ state of 12C : A benchmark of theoretical models
dc.typeresearch article
dc.identifier.urnURN:NBN:fi:jyu-202309085035
dc.contributor.laitosFysiikan laitosfi
dc.contributor.laitosDepartment of Physicsen
dc.contributor.oppiaineYdin- ja kiihdytinfysiikan huippuyksikköfi
dc.contributor.oppiaineFysiikkafi
dc.contributor.oppiaineKiihdytinlaboratoriofi
dc.contributor.oppiaineCentre of Excellence in Nuclear and Accelerator Based Physicsen
dc.contributor.oppiainePhysicsen
dc.contributor.oppiaineAccelerator Laboratoryen
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.volume845
dc.type.versionpublishedVersion
dc.rights.copyright© 2023 the Authors
dc.rights.accesslevelopenAccessfi
dc.type.publicationarticle
dc.subject.ysospektroskopia
dc.subject.ysohiili
dc.subject.ysoydinfysiikka
dc.format.contentfulltext
jyx.subject.urihttp://www.yso.fi/onto/yso/p10176
jyx.subject.urihttp://www.yso.fi/onto/yso/p138
jyx.subject.urihttp://www.yso.fi/onto/yso/p14759
dc.rights.urlhttps://creativecommons.org/licenses/by/4.0/
dc.relation.doi10.1016/j.physletb.2023.138114
jyx.fundinginformationThe authors acknowledge C. Bertulani, A. Vitturi, A. Moro, M. Gomez, J. M. Quesada, M. Zielinska, and C. Barton for enlightening discussions, and I. Moore for proposing and supporting the production of the 66Ga source. This work was supported by the Deutsche Forschungsgemeinschaft (DFG, German Research Foundation) – Projektnummer 279384907 – SFB 1245, the Royal Society under contract number UF150476, the UK STFC under grant numbers ST/L005727/1, ST/P003885/1, the UK STFC ERF fellowship ST/R004056/1, and by the Director, Office of Science, Office of Nuclear Physics, of the U.S. Department of Energy under Contract No. DE-AC02-05CH11231 (LBNL). This project has received funding from the EU HORIZON2020 programme “Infrastructures”, project number 654002 (ENSAR2). U. Forsberg would like to thank Birgit and Hellmuth Hertz' Foundation for financial support.
dc.type.okmA1


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