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

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DC Field	Value	Language
dc.contributor.author	한인식	*
dc.date.accessioned	2019-03-27T16:30:08Z	-
dc.date.available	2019-03-27T16:30:08Z	-
dc.date.issued	2019	*
dc.identifier.issn	0031-9007	*
dc.identifier.other	OAK-24493	*
dc.identifier.uri	https://dspace.ewha.ac.kr/handle/2015.oak/249522	-
dc.description.abstract	The first γ-ray spectroscopy of Ar52, with the neutron number N=34, was measured using the K53(p,2p) one-proton removal reaction at ∼210 MeV/u at the RIBF facility. The 21+ excitation energy is found at 1656(18) keV, the highest among the Ar isotopes with N>20. This result is the first experimental signature of the persistence of the N=34 subshell closure beyond Ca54, i.e., below the magic proton number Z=20. Shell-model calculations with phenomenological and chiral-effective-field-theory interactions both reproduce the measured 21+ systematics of neutron-rich Ar isotopes, and support a N=34 subshell closure in Ar52. © 2019 authors. Published by the American Physical Society.	*
dc.language	English	*
dc.publisher	American Physical Society	*
dc.title	How Robust is the N=34 Subshell Closure? First Spectroscopy of Ar 52	*
dc.type	Article	*
dc.relation.issue	7	*
dc.relation.volume	122	*
dc.relation.index	SCIE	*
dc.relation.index	SCOPUS	*
dc.relation.journaltitle	Physical Review Letters	*
dc.identifier.doi	10.1103/PhysRevLett.122.072502	*
dc.identifier.scopusid	2-s2.0-85062034151	*
dc.author.google	Liu H.N.	*
dc.author.google	Obertelli A.	*
dc.author.google	Doornenbal P.	*
dc.author.google	Bertulani C.A.	*
dc.author.google	Hagen G.	*
dc.author.google	Holt J.D.	*
dc.author.google	Jansen G.R.	*
dc.author.google	Morris T.D.	*
dc.author.google	Schwenk A.	*
dc.author.google	Stroberg R.	*
dc.author.google	Achouri N.	*
dc.author.google	Baba H.	*
dc.author.google	Browne F.	*
dc.author.google	Calvet D.	*
dc.author.google	Château F.	*
dc.author.google	Chen S.	*
dc.author.google	Chiga N.	*
dc.author.google	Corsi A.	*
dc.author.google	Cortés M.L.	*
dc.author.google	Delbart A.	*
dc.author.google	Gheller J.-M.	*
dc.author.google	Giganon A.	*
dc.author.google	Gillibert A.	*
dc.author.google	Hilaire C.	*
dc.author.google	Isobe T.	*
dc.author.google	Kobayashi T.	*
dc.author.google	Kubota Y.	*
dc.author.google	Lapoux V.	*
dc.author.google	Motobayashi T.	*
dc.author.google	Murray I.	*
dc.author.google	Otsu H.	*
dc.author.google	Panin V.	*
dc.author.google	Paul N.	*
dc.author.google	Rodriguez W.	*
dc.author.google	Sakurai H.	*
dc.author.google	Sasano M.	*
dc.author.google	Steppenbeck D.	*
dc.author.google	Stuhl L.	*
dc.author.google	Sun Y.L.	*
dc.author.google	Togano Y.	*
dc.author.google	Uesaka T.	*
dc.author.google	Wimmer K.	*
dc.author.google	Yoneda K.	*
dc.author.google	Aktas O.	*
dc.author.google	Aumann T.	*
dc.author.google	Chung L.X.	*
dc.author.google	Flavigny F.	*
dc.author.google	Franchoo S.	*
dc.author.google	Gašparić I.	*
dc.author.google	Gerst R.-B.	*
dc.author.google	Gibelin J.	*
dc.author.google	Hahn K.I.	*
dc.author.google	Kim D.	*
dc.author.google	Koiwai T.	*
dc.author.google	Kondo Y.	*
dc.author.google	Koseoglou P.	*
dc.author.google	Lee J.	*
dc.author.google	Lehr C.	*
dc.author.google	Linh B.D.	*
dc.author.google	Lokotko T.	*
dc.author.google	Maccormick M.	*
dc.author.google	Moschner K.	*
dc.author.google	Nakamura T.	*
dc.author.google	Park S.Y.	*
dc.author.google	Rossi D.	*
dc.author.google	Sahin E.	*
dc.author.google	Sohler D.	*
dc.author.google	Söderström P.-A.	*
dc.author.google	Takeuchi S.	*
dc.author.google	Törnqvist H.	*
dc.author.google	Vaquero V.	*
dc.author.google	Wagner V.	*
dc.author.google	Wang S.	*
dc.author.google	Werner V.	*
dc.author.google	Xu X.	*
dc.author.google	Yamada H.	*
dc.author.google	Yan D.	*
dc.author.google	Yang Z.	*
dc.author.google	Yasuda M.	*
dc.author.google	Zanetti L.	*
dc.contributor.scopusid	한인식(7201832280;57205469686;57192312712)	*
dc.date.modifydate	20240415134453	*