Electromagnetic moments of scandium isotopes and N = 28 isotones in the distinctive 0f7/2 orbit
dc.contributor.author | Bai, S.W. | |
dc.contributor.author | Koszorús, Á. | |
dc.contributor.author | Hu, B.S. | |
dc.contributor.author | Yang, X.F. | |
dc.contributor.author | Billowes, J. | |
dc.contributor.author | Binnersley, C.L. | |
dc.contributor.author | Bissell, M.L. | |
dc.contributor.author | Blaum, K. | |
dc.contributor.author | Campbell, P. | |
dc.contributor.author | Cheal, B. | |
dc.contributor.author | Cocolios, T.E. | |
dc.contributor.author | de Groote, R.P. | |
dc.contributor.author | Devlin, C.S. | |
dc.contributor.author | Flanagan, K.T. | |
dc.contributor.author | Garcia Ruiz, R.F. | |
dc.contributor.author | Heylen, H. | |
dc.contributor.author | Holt, J.D. | |
dc.contributor.author | Kanellakopoulos, A. | |
dc.contributor.author | Krämer, J. | |
dc.contributor.author | Lagaki, V. | |
dc.contributor.author | Maaß, B. | |
dc.contributor.author | Malbrunot-Ettenauer, S. | |
dc.contributor.author | Miyagi, T. | |
dc.contributor.author | Neugart, R. | |
dc.contributor.author | Neyens, G. | |
dc.contributor.author | Nörtershäuser, W. | |
dc.contributor.author | Rodríguez, L.V. | |
dc.contributor.author | Sommer, F. | |
dc.contributor.author | Vernon, A.R. | |
dc.contributor.author | Wang, S.J. | |
dc.contributor.author | Wang, X.B. | |
dc.contributor.author | Wilkins, S.G. | |
dc.contributor.author | Xu, Z.Y. | |
dc.contributor.author | Yuan, C.X. | |
dc.date.accessioned | 2022-05-04T09:44:20Z | |
dc.date.available | 2022-05-04T09:44:20Z | |
dc.date.issued | 2022 | |
dc.identifier.citation | Bai, 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.other | CONVID_117769520 | |
dc.identifier.uri | https://jyx.jyu.fi/handle/123456789/80881 | |
dc.description.abstract | The 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.mimetype | application/pdf | |
dc.language.iso | eng | |
dc.publisher | Elsevier | |
dc.relation.ispartofseries | Physics Letters B | |
dc.rights | CC BY 4.0 | |
dc.subject.other | Collinear laser spectroscopy | |
dc.subject.other | Electromagnetic moments | |
dc.subject.other | Nucleon-nucleon correlation | |
dc.subject.other | Ab-initio calculation | |
dc.title | Electromagnetic moments of scandium isotopes and N = 28 isotones in the distinctive 0f7/2 orbit | |
dc.type | article | |
dc.identifier.urn | URN:NBN:fi:jyu-202205042543 | |
dc.contributor.laitos | Fysiikan laitos | fi |
dc.contributor.laitos | Department of Physics | en |
dc.type.uri | http://purl.org/eprint/type/JournalArticle | |
dc.type.coar | http://purl.org/coar/resource_type/c_2df8fbb1 | |
dc.description.reviewstatus | peerReviewed | |
dc.relation.issn | 0370-2693 | |
dc.relation.volume | 829 | |
dc.type.version | publishedVersion | |
dc.rights.copyright | © 2022 the Authors | |
dc.rights.accesslevel | openAccess | fi |
dc.subject.yso | ydinfysiikka | |
dc.subject.yso | isotoopit | |
dc.subject.yso | skandium | |
dc.format.content | fulltext | |
jyx.subject.uri | http://www.yso.fi/onto/yso/p14759 | |
jyx.subject.uri | http://www.yso.fi/onto/yso/p6387 | |
jyx.subject.uri | http://www.yso.fi/onto/yso/p38599 | |
dc.rights.url | https://creativecommons.org/licenses/by/4.0/ | |
dc.relation.doi | 10.1016/j.physletb.2022.137064 | |
jyx.fundinginformation | We 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.okm | A1 |