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dc.contributor.authorHeylen, H.
dc.contributor.authorDevlin, C. S.
dc.contributor.authorGins, W.
dc.contributor.authorBissell, M. L.
dc.contributor.authorBlaum, K.
dc.contributor.authorCheal, B.
dc.contributor.authorFilippin, L.
dc.contributor.authorRuiz, R. F. Garcia
dc.contributor.authorGodefroid, M.
dc.contributor.authorGorges, C.
dc.contributor.authorHolt, J. D.
dc.contributor.authorKanellakopoulos, A.
dc.contributor.authorKaufmann, S.
dc.contributor.authorKoszorús, Á.
dc.contributor.authorKönig, K.
dc.contributor.authorMalbrunot-Ettenauer, S.
dc.contributor.authorMiyagi, T.
dc.contributor.authorNeugart, R.
dc.contributor.authorNeyens, G.
dc.contributor.authorNörtershäuser, W.
dc.contributor.authorSánchez, R.
dc.contributor.authorSommer, F.
dc.contributor.authorRodríguez, L. V.
dc.contributor.authorXie, L.
dc.contributor.authorXu, Z. Y.
dc.contributor.authorYang, X. F.
dc.contributor.authorYordanov, D. T.
dc.date.accessioned2021-02-25T08:46:59Z
dc.date.available2021-02-25T08:46:59Z
dc.date.issued2021
dc.identifier.citationHeylen, H., Devlin, C. S., Gins, W., Bissell, M. L., Blaum, K., Cheal, B., Filippin, L., Ruiz, R. F. G., Godefroid, M., Gorges, C., Holt, J. D., Kanellakopoulos, A., Kaufmann, S., Koszorús, Á., König, K., Malbrunot-Ettenauer, S., Miyagi, T., Neugart, R., Neyens, G., . . . Yordanov, D. T. (2021). High-resolution laser spectroscopy of 27–32Al. <i>Physical Review C</i>, <i>103</i>(1), Article 014318. <a href="https://doi.org/10.1103/PhysRevC.103.014318" target="_blank">https://doi.org/10.1103/PhysRevC.103.014318</a>
dc.identifier.otherCONVID_51620816
dc.identifier.urihttps://jyx.jyu.fi/handle/123456789/74391
dc.description.abstractHyperfine spectra of 27–32Al (Z=13) have been measured at the ISOLDE-CERN facility via collinear laser spectroscopy using the 3s23p2Po3/2→3s24s2S1/2 atomic transition. For the first time, mean-square charge radii of radioactive aluminum isotopes have been determined alongside the previously unknown magnetic dipole moment of 29Al and electric quadrupole moments of 29,30Al. A potentially reduced charge radius at N=19 may suggest an effect of the N=20 shell closure, which is visible in the Al chain, contrary to other isotopic chains in the sd shell. The experimental results are compared with theoretical calculations in the framework of the valence-space in-medium similarity renormalization group using multiple sets of two- and three-nucleon forces from chiral effective field theory. While the trend of experimental magnetic dipole and electric quadrupole moments is well reproduced, the absolute values are underestimated by theory, which is consistent with earlier studies. Moreover, both the scale and trend of the charge radii appear to be very sensitive to the chosen interaction.en
dc.format.mimetypeapplication/pdf
dc.languageeng
dc.language.isoeng
dc.publisherAmerican Physical Society (APS)
dc.relation.ispartofseriesPhysical Review C
dc.rightsCC BY 4.0
dc.titleHigh-resolution laser spectroscopy of 27–32Al
dc.typearticle
dc.identifier.urnURN:NBN:fi:jyu-202102251771
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.issn2469-9985
dc.relation.numberinseries1
dc.relation.volume103
dc.type.versionpublishedVersion
dc.rights.copyright© Authors, 2021
dc.rights.accesslevelopenAccessfi
dc.subject.ysospektroskopia
dc.subject.ysoisotoopit
dc.subject.ysoydinfysiikka
dc.subject.ysoalumiini
dc.format.contentfulltext
jyx.subject.urihttp://www.yso.fi/onto/yso/p10176
jyx.subject.urihttp://www.yso.fi/onto/yso/p6387
jyx.subject.urihttp://www.yso.fi/onto/yso/p14759
jyx.subject.urihttp://www.yso.fi/onto/yso/p19563
dc.rights.urlhttps://creativecommons.org/licenses/by/4.0/
dc.relation.doi10.1103/PhysRevC.103.014318
jyx.fundinginformationWe acknowledge the support from FWO-Vlaanderen, the Max-Planck Society, UK Science and Technology Facilities Council (STFC) grant ST/P004598/1, the BMBF under Contract No. 05P18RDCIA, the Helmholtz International Center for FAIR (HIC for FAIR), the FWO and FNRS Excellence of Science Programme (EOS-O022818F) and STFC grant ST/P004423/1.
dc.type.okmA1


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