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Article: Structure of 136Sn and the Z = 50 magicity

TitleStructure of 136Sn and the Z = 50 magicity
Authors
Wang, HeAoi, NoriTakeuchi, SatoshiMatsushita, MasafumiDoornenbal, Pieter C.Motobayashi, TohruSteppenbeck, DavidYoneda, KenichiroBaba, HidetadaDombrádi, Zs S.Kobayashi, KotaKondo, YosukeLee, JennyLiu, HongnaMinakata, RyogoNishimura, DaiOtsu, HideakiSakuraï, HiroyoshiSohler, DoraSun, YeleiTian, ZhengyangTanaka, RyukiVajta, ZsYang, ZaihongYamamoto, TetsuyaYe, YanlinYokoyama, Rin
Issue Date2014
Citation
Progress of Theoretical and Experimental Physics, 2014, v. 2014, n. 2, article no. 023D02 How to Cite?
DOI: http://dx.doi.org/10.1093/ptep/ptu003
AbstractThe first 2+ excited state in the neutron-rich tin isotope 136Sn has been identified at 682(13) keV by measuring γ -rays in coincidence with the one proton removal channel from 137Sb. This value is higher than those known for heavier even-even N = 86 isotones, indicating the Z = 50 shell closure. It compares well to the first 2+ excited state of the lighter tin isotope 134Sn, which may suggest that the seniority scheme also holds for 136Sn. Our result confirms the trend of lower 2+ excitation energies of even-even tin isotopes beyond N = 82 compared to the known values in between the two doubly magic nuclei 100Sn and 132Sn. © The Author(s) 2014.
Persistent Identifierhttp://hdl.handle.net/10722/200148
ISI Accession Number ID
WOS:000332336600010

 

DC FieldValueLanguage
dc.contributor.authorWang, He-
dc.contributor.authorAoi, Nori-
dc.contributor.authorTakeuchi, Satoshi-
dc.contributor.authorMatsushita, Masafumi-
dc.contributor.authorDoornenbal, Pieter C.-
dc.contributor.authorMotobayashi, Tohru-
dc.contributor.authorSteppenbeck, David-
dc.contributor.authorYoneda, Kenichiro-
dc.contributor.authorBaba, Hidetada-
dc.contributor.authorDombrádi, Zs S.-
dc.contributor.authorKobayashi, Kota-
dc.contributor.authorKondo, Yosuke-
dc.contributor.authorLee, Jenny-
dc.contributor.authorLiu, Hongna-
dc.contributor.authorMinakata, Ryogo-
dc.contributor.authorNishimura, Dai-
dc.contributor.authorOtsu, Hideaki-
dc.contributor.authorSakuraï, Hiroyoshi-
dc.contributor.authorSohler, Dora-
dc.contributor.authorSun, Yelei-
dc.contributor.authorTian, Zhengyang-
dc.contributor.authorTanaka, Ryuki-
dc.contributor.authorVajta, Zs-
dc.contributor.authorYang, Zaihong-
dc.contributor.authorYamamoto, Tetsuya-
dc.contributor.authorYe, Yanlin-
dc.contributor.authorYokoyama, Rin-
dc.date.accessioned2014-07-26T23:11:11Z-
dc.date.available2014-07-26T23:11:11Z-
dc.date.issued2014-
dc.identifier.citationProgress of Theoretical and Experimental Physics, 2014, v. 2014, n. 2, article no. 023D02-
dc.identifier.urihttp://hdl.handle.net/10722/200148-
dc.description.abstractThe first 2+ excited state in the neutron-rich tin isotope 136Sn has been identified at 682(13) keV by measuring γ -rays in coincidence with the one proton removal channel from 137Sb. This value is higher than those known for heavier even-even N = 86 isotones, indicating the Z = 50 shell closure. It compares well to the first 2+ excited state of the lighter tin isotope 134Sn, which may suggest that the seniority scheme also holds for 136Sn. Our result confirms the trend of lower 2+ excitation energies of even-even tin isotopes beyond N = 82 compared to the known values in between the two doubly magic nuclei 100Sn and 132Sn. © The Author(s) 2014.-
dc.languageeng-
dc.relation.ispartofProgress of Theoretical and Experimental Physics-
dc.titleStructure of 136Sn and the Z = 50 magicity-
dc.typeArticle-
dc.description.naturepublished_or_final_version-
dc.identifier.doi10.1093/ptep/ptu003-
dc.identifier.scopuseid_2-s2.0-84898401709-
dc.identifier.volume2014-
dc.identifier.issue2-
dc.identifier.spagearticle no. 023D02-
dc.identifier.epagearticle no. 023D02-
dc.identifier.eissn2050-3911-
dc.identifier.isiWOS:000332336600010-
dc.identifier.issnl2050-3911-

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