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Article: How Robust is the N=34 Subshell Closure? First Spectroscopy of 52Ar

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dc.contributor.authorLiu, HN-
dc.contributor.authorObertelli, A-
dc.contributor.authorDoornenbal, P-
dc.contributor.authorBertulani, CA-
dc.contributor.authorHagen, G-
dc.contributor.authorHolt, JD-
dc.contributor.authorJansen, GR-
dc.contributor.authorMorris, TD-
dc.contributor.authorSchwenk, A-
dc.contributor.authorStroberg, R-
dc.contributor.authorAchouri, N-
dc.contributor.authorBaba, H-
dc.contributor.authorBrowne, F-
dc.contributor.authorCalvet, D-
dc.contributor.authorChâteau, F-
dc.contributor.authorChen, S-
dc.contributor.authorChiga, N-
dc.contributor.authorCorsi, A-
dc.contributor.authorCortés, ML-
dc.contributor.authorDelbart, A-
dc.contributor.authorGheller, JM-
dc.contributor.authorGiganon, A-
dc.contributor.authorGillibert, A-
dc.contributor.authorHilaire, C-
dc.contributor.authorIsobe, T-
dc.contributor.authorKobayashi, T-
dc.contributor.authorKubota, Y-
dc.contributor.authorLapoux, V-
dc.contributor.authorMotobayashi, T-
dc.contributor.authorMurray, I-
dc.contributor.authorOtsu, H-
dc.contributor.authorPanin, V-
dc.contributor.authorPaul, N-
dc.contributor.authorRodriguez, W-
dc.contributor.authorSakurai, H-
dc.contributor.authorSasano, M-
dc.contributor.authorSteppenbeck, D-
dc.contributor.authorStuhl, L-
dc.contributor.authorSun, YL-
dc.contributor.authorTogano, Y-
dc.contributor.authorUesaka, T-
dc.contributor.authorWimmer, K-
dc.contributor.authorYoneda, K-
dc.contributor.authorAktas, O-
dc.contributor.authorAumann, T-
dc.contributor.authorChung, LX-
dc.contributor.authorFlavigny, F-
dc.contributor.authorFranchoo, S-
dc.contributor.authorGašparić, I-
dc.contributor.authorGerst, RB-
dc.contributor.authorGibelin, J-
dc.contributor.authorHahn, KI-
dc.contributor.authorKim, D-
dc.contributor.authorKoiwai, T-
dc.contributor.authorKondo, Y-
dc.contributor.authorKoseoglou, P-
dc.contributor.authorLee, HCJ-
dc.contributor.authorLehr, C-
dc.contributor.authorLinh, BD-
dc.contributor.authorLokotko, T-
dc.contributor.authorMacCormick, M-
dc.contributor.authorMoschner, K-
dc.contributor.authorNakamura, T-
dc.contributor.authorPark, SY-
dc.contributor.authorRossi, D-
dc.contributor.authorSahin, E-
dc.contributor.authorSohler, D-
dc.contributor.authorSöderström, PA-
dc.contributor.authorTakeuchi, S-
dc.contributor.authorTörnqvist, H-
dc.contributor.authorVaquero, V-
dc.contributor.authorWagner, V-
dc.contributor.authorWang, S-
dc.contributor.authorWerner, V-
dc.contributor.authorXu, X-
dc.contributor.authorYamada, H-
dc.contributor.authorYan, D-
dc.contributor.authorYang, Z-
dc.contributor.authorYasuda, M-
dc.contributor.authorZanetti, L-
dc.date.accessioned2019-03-18T04:20:52Z-
dc.date.available2019-03-18T04:20:52Z-
dc.date.issued2019-
dc.identifier.citationPhysical Review Letters, 2019, v. 122 n. 7, article no. 072502 , p. 1-7-
dc.identifier.issn0031-9007-
dc.identifier.urihttp://hdl.handle.net/10722/268211-
dc.languageeng-
dc.publisherAmerican Physical Society. The Journal's web site is located at http://prl.aps.org-
dc.relation.ispartofPhysical Review Letters-
dc.rightsThis work is licensed under a Creative Commons Attribution-NonCommercial-NoDerivatives 4.0 International License.-
dc.titleHow Robust is the N=34 Subshell Closure? First Spectroscopy of 52Ar-
dc.typeArticle-
dc.identifier.emailChen, S: sdchen@hku.hk-
dc.identifier.emailLee, HCJ: jleehc@hku.hk-
dc.identifier.emailLokotko, T: tlokotko@hku.hk-
dc.identifier.emailXu, X: xinxing@hku.hk-
dc.identifier.authorityLee, HCJ=rp01902-
dc.description.naturepublished_or_final_version-
dc.identifier.doi10.1103/PhysRevLett.122.072502-
dc.identifier.hkuros297166-
dc.identifier.volume122-
dc.identifier.issue7-
dc.identifier.spagearticle no. 072502, p. 1-
dc.identifier.epagearticle no. 072502, p. 7-
dc.publisher.placeUnited States-

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