期刊
PHYSICAL REVIEW LETTERS
卷 126, 期 4, 页码 -出版社
AMER PHYSICAL SOC
DOI: 10.1103/PhysRevLett.126.042501
关键词
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资金
- U.S. National Science Foundation [PHY-1565546, PHY-1811855]
- U.S. Department of Energy, Office of Science, Office of Nuclear Physics [DE-SC0015927]
- Natural Sciences and Engineering Research Council (NSERC) of Canada [SAPPJ-2018-00015]
- National Research Council (NRC) of Canada through TRIUMF
- U.K.-Canada foundation
- BMBF [05P16RGFN1, 05P19RGFN8]
- Hessisches Ministerium fur Wissenschaft und Kunst (HMWK) through the LOEWE Center HICforFAIR
- JLU
- GSI Helmholtzzentrum fur Schwerionenforschung under the JLU-GSI strategic Helmholtz partnership agreement
- NSERC (Canada) [SAPPJ-2018-00028]
- Michigan State University
High-precision mass measurements of Sc50-55 isotopes show significant deviations from previously recommended values, providing important updates for understanding closed-shell phenomena at neutron numbers N = 32 and N = 34 above proton-magic Z = 20. The results also indicate a lack of support for the existence of a closed neutron shell in Sc-55 at N = 34, and highlight discrepancies in predictions from different nuclear theories for the N = 34 isotone.
We report high-precision mass measurements of Sc50-55 isotopes performed at the LEBIT facility at NSCL and at the TITAN facility at TRIUMF. Our results provide a substantial reduction of their uncertainties and indicate significant deviations, up to 0.7 MeV, from the previously recommended mass values for 53-55SC. The results of this work provide an important update to the description of emerging closed-shell phenomena at neutron numbers N = 32 and N = 34 above proton-magic Z = 20. In particular, they finally enable a complete and precise characterization of the trends in ground state binding energies along the N = 32 isotone, confirming that the empirical neutron shell gap energies peak at the doubly magic Ca-52. Moreover, our data, combined with other recent measurements, do not support the existence of a closed neutron shell in Sc-55 at N = 34. The results were compared to predictions from both ab initio and phenomenological nuclear theories, which all had success describing N = 32 neutron shell gap energies but were highly disparate in the description of the N = 34 isotone.
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