期刊
PHYSICAL REVIEW LETTERS
卷 122, 期 7, 页码 -出版社
AMER PHYSICAL SOC
DOI: 10.1103/PhysRevLett.122.072502
关键词
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资金
- European Research Council through the ERC [MINOS-258567]
- Enhanced Eurotalents program - CEA [PCOFUND-GA-2013-600382]
- European Union
- Deutsche Forschungsgemeinschaft (DFG, German Research Foundation) [279384907-SFB 1245]
- U.S. NSF [1415656]
- U.S. DOE [DE-FG02-08ER41533]
- NSERC
- National Research Council Canada
- Marie Sklodowska-Curie Individual Fellowship from the European Union [H2020-MSCA-IF-2015-705023]
- Croatian Science Foundation
- Vietnam MOST through the Physics Development Program [DTDLCN.25/18]
- NRF - Korea government [2017R1A2B2012382, 2018R1A5A1025563]
- JSPS KAKENHI [16H02179]
- MEXT KAKENHI [24105005, 18H05404]
- Office of Nuclear Physics, U.S. Department of Energy [de-sc0018223]
- Office of Science of the Department of Energy [DE-AC05-00OR22725]
- HIC for FAIR
- National Research Foundation of Korea [2018R1A5A1025563, 2017R1A2B2012382] Funding Source: Korea Institute of Science & Technology Information (KISTI), National Science & Technology Information Service (NTIS)
- Grants-in-Aid for Scientific Research [18H05404] Funding Source: KAKEN
The first gamma-ray spectroscopy of Ar-52, with the neutron number N = 34, was measured using the K-53(p, 2p) one-proton removal reaction at similar to 210 MeV/u at the RIBF facility. The 2(1)(+) 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 Ca-54, i.e., below the magic proton number Z = 20. Shell-model calculations with phenomenological and chiral-effective-field-theory interactions both reproduce the measured 2(1)(+) systematics of neutron-rich Ar isotopes, and support a N = 34 subshell closure in Ar-52.
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