TY - JOUR
T1 - Precision Mass Measurements of Neutron-Rich Scandium Isotopes Refine the Evolution of N=32 and N=34 Shell Closures
AU - The LEBIT Collaboration and the TITAN Collaboration
AU - Leistenschneider, E.
AU - Dunling, E.
AU - Bollen, G.
AU - Brown, B. A.
AU - Dilling, J.
AU - Hamaker, A.
AU - Holt, J. D.
AU - Jacobs, A.
AU - Kwiatkowski, A. A.
AU - Miyagi, T.
AU - Porter, W. S.
AU - Puentes, D.
AU - Redshaw, M.
AU - Reiter, M. P.
AU - Ringle, R.
AU - Sandler, R.
AU - Sumithrarachchi, C. S.
AU - Valverde, A. A.
AU - Yandow, I. T.
N1 - Funding Information:
The authors would like to thank J. Simonis and P. Navrátil for providing the and matrix element files and S. R. Stroberg for the imsrg ++ code used to perform the VS-IMSRG calculations. We are grateful to Z. Meisel for the fruitful discussions regarding data obtained in previous experiments. We also thank NSCL staff, the ISAC Beam Delivery group, the TRILIS group, and M. Good for their technical support, as well as J. Bergmann for his assistance with analysis software employed in this work. This work was conducted with the support of Michigan State University, the U.S. National Science Foundation under Contracts No. PHY-1565546 and No. PHY-1811855, the U.S. Department of Energy, Office of Science, Office of Nuclear Physics under Award No. DE-SC0015927, the Natural Sciences and Engineering Research Council (NSERC) of Canada through Contract No. SAPPJ-2018-00015 and the National Research Council (NRC) of Canada through TRIUMF. E. D. acknowledges financial support from the U.K.-Canada foundation. M. P. R. acknowledges support from BMBF (Grants No. 05P16RGFN1 and No. 05P19RGFN8), Hessisches Ministerium für Wissenschaft und Kunst (HMWK) through the LOEWE Center HICforFAIR, by the JLU and GSI Helmholtzzentrum für Schwerionenforschung under the JLU-GSI strategic Helmholtz partnership agreement. A. A. V. acknowledges support from NSERC (Canada) under Contract No. SAPPJ-2018-00028.
Publisher Copyright:
© 2021 American Physical Society.
PY - 2021/1/26
Y1 - 2021/1/26
N2 - 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 Sc53-55. 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 Ca52. Moreover, our data, combined with other recent measurements, do not support the existence of a closed neutron shell in Sc55 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.
AB - 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 Sc53-55. 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 Ca52. Moreover, our data, combined with other recent measurements, do not support the existence of a closed neutron shell in Sc55 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.
UR - http://www.scopus.com/inward/record.url?scp=85100238495&partnerID=8YFLogxK
U2 - 10.1103/PhysRevLett.126.042501
DO - 10.1103/PhysRevLett.126.042501
M3 - Article
C2 - 33576685
AN - SCOPUS:85100238495
SN - 0031-9007
VL - 126
JO - Physical Review Letters
JF - Physical Review Letters
IS - 4
M1 - 042501
ER -