4.8 Article

Precision Mass Measurements of Neutron-Rich Scandium Isotopes Refine the Evolution of N=32 and N=34 Shell Closures

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

-

资金

  1. U.S. National Science Foundation [PHY-1565546, PHY-1811855]
  2. U.S. Department of Energy, Office of Science, Office of Nuclear Physics [DE-SC0015927]
  3. Natural Sciences and Engineering Research Council (NSERC) of Canada [SAPPJ-2018-00015]
  4. National Research Council (NRC) of Canada through TRIUMF
  5. U.K.-Canada foundation
  6. BMBF [05P16RGFN1, 05P19RGFN8]
  7. Hessisches Ministerium fur Wissenschaft und Kunst (HMWK) through the LOEWE Center HICforFAIR
  8. JLU
  9. GSI Helmholtzzentrum fur Schwerionenforschung under the JLU-GSI strategic Helmholtz partnership agreement
  10. NSERC (Canada) [SAPPJ-2018-00028]
  11. Michigan State University

向作者/读者索取更多资源

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.

作者

我是这篇论文的作者
点击您的名字以认领此论文并将其添加到您的个人资料中。

评论

主要评分

4.8
评分不足

次要评分

新颖性
-
重要性
-
科学严谨性
-
评价这篇论文

推荐

暂无数据
暂无数据