View : 35 Download: 0

Full metadata record

DC Field Value Language
dc.contributor.author한인식-
dc.date.accessioned2019-03-27T16:30:08Z-
dc.date.available2019-03-27T16:30:08Z-
dc.date.issued2019-
dc.identifier.issn0031-9007-
dc.identifier.otherOAK-24493-
dc.identifier.urihttp://dspace.ewha.ac.kr/handle/2015.oak/249522-
dc.description.abstractThe 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.languageEnglish-
dc.publisherAmerican Physical Society-
dc.titleHow Robust is the N=34 Subshell Closure? First Spectroscopy of Ar 52-
dc.typeArticle-
dc.relation.issue7-
dc.relation.volume122-
dc.relation.indexSCI-
dc.relation.indexSCIE-
dc.relation.indexSCOPUS-
dc.relation.journaltitlePhysical Review Letters-
dc.identifier.doi10.1103/PhysRevLett.122.072502-
dc.identifier.scopusid2-s2.0-85062034151-
dc.author.googleLiu H.N.-
dc.author.googleObertelli A.-
dc.author.googleDoornenbal P.-
dc.author.googleBertulani C.A.-
dc.author.googleHagen G.-
dc.author.googleHolt J.D.-
dc.author.googleJansen G.R.-
dc.author.googleMorris T.D.-
dc.author.googleSchwenk A.-
dc.author.googleStroberg R.-
dc.author.googleAchouri N.-
dc.author.googleBaba H.-
dc.author.googleLee J.-
dc.author.googleLehr C.-
dc.author.googleLinh B.D.-
dc.author.googleLokotko T.-
dc.author.googleMaccormick M.-
dc.author.googleMoschner K.-
dc.author.googleNakamura T.-
dc.author.googlePark S.Y.-
dc.author.googleBrowne F.-
dc.author.googleCalvet D.-
dc.author.googleChâteau F.-
dc.author.googleChen S.-
dc.author.googleChiga N.-
dc.author.googleCorsi A.-
dc.author.googleCortés M.L.-
dc.author.googleDelbart A.-
dc.author.googleGheller J.-M.-
dc.author.googleGiganon A.-
dc.author.googleGillibert A.-
dc.author.googleHilaire C.-
dc.author.googleIsobe T.-
dc.author.googleKobayashi T.-
dc.author.googleKubota Y.-
dc.author.googleLapoux V.-
dc.author.googleMotobayashi T.-
dc.author.googleMurray I.-
dc.author.googleOtsu H.-
dc.author.googlePanin V.-
dc.author.googlePaul N.-
dc.author.googleRodriguez W.-
dc.author.googleSakurai H.-
dc.author.googleSasano M.-
dc.author.googleSteppenbeck D.-
dc.author.googleStuhl L.-
dc.author.googleSun Y.L.-
dc.author.googleTogano Y.-
dc.author.googleUesaka T.-
dc.author.googleWimmer K.-
dc.author.googleYoneda K.-
dc.author.googleAktas O.-
dc.author.googleAumann T.-
dc.author.googleChung L.X.-
dc.author.googleFlavigny F.-
dc.author.googleFranchoo S.-
dc.author.googleGašparić I.-
dc.author.googleGerst R.-B.-
dc.author.googleGibelin J.-
dc.author.googleHahn K.I.-
dc.author.googleKim D.-
dc.author.googleKoiwai T.-
dc.author.googleKondo Y.-
dc.author.googleKoseoglou P.-
dc.author.googleRossi D.-
dc.author.googleSahin E.-
dc.author.googleSohler D.-
dc.author.googleSöderström P.-A.-
dc.author.googleTakeuchi S.-
dc.author.googleTörnqvist H.-
dc.author.googleVaquero V.-
dc.author.googleWagner V.-
dc.author.googleWang S.-
dc.author.googleWerner V.-
dc.author.googleXu X.-
dc.author.googleYamada H.-
dc.author.googleYan D.-
dc.author.googleYang Z.-
dc.author.googleYasuda M.-
dc.author.googleZanetti L.-
dc.contributor.scopusid한인식(7201832280)-
dc.date.modifydate20190327100619-
Appears in Collections:
사범대학 > 과학교육과 > Journal papers
Files in This Item:
There are no files associated with this item.
Export
RIS (EndNote)
XLS (Excel)
XML


qrcode

Items in DSpace are protected by copyright, with all rights reserved, unless otherwise indicated.

BROWSE