Dawning of the N=32 Shell Closure Seen through Precision Mass Measurements of Neutron-Rich Titanium Isotopes

E. Leistenschneider, M. P. Reiter, S. Ayet San Andrés, B. Kootte, J. D. Holt, P. Navrátil, C. Babcock, C. Barbieri, B. R. Barquest, J. Bergmann, J. Bollig, T. Brunner, E. Dunling, A. Finlay, H. Geissel, L. Graham, F. Greiner, H. Hergert, C. Hornung, C. JeschR. Klawitter, Y. Lan, D. Lascar, K. G. Leach, W. Lippert, J. E. McKay, S. F. Paul, A. Schwenk, D. Short, J. Simonis, V. Somà, R. Steinbrügge, S. R. Stroberg, R. Thompson, M. E. Wieser, C. Will, M. Yavor, C. Andreoiu, T. Dickel, I. Dillmann, G. Gwinner, W. R. Plaß, C. Scheidenberger, A. A. Kwiatkowski, J. Dilling

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Abstract

A precision mass investigation of the neutron-rich titanium isotopes Ti51-55 was performed at TRIUMF's Ion Trap for Atomic and Nuclear science (TITAN). The range of the measurements covers the N=32 shell closure, and the overall uncertainties of the Ti52-55 mass values were significantly reduced. Our results conclusively establish the existence of the weak shell effect at N=32, narrowing down the abrupt onset of this shell closure. Our data were compared with state-of-the-art ab initio shell model calculations which, despite very successfully describing where the N=32 shell gap is strong, overpredict its strength and extent in titanium and heavier isotones. These measurements also represent the first scientific results of TITAN using the newly commissioned multiple-reflection time-of-flight mass spectrometer, substantiated by independent measurements from TITAN's Penning trap mass spectrometer.

Original languageEnglish
Article number062503
JournalPhysical Review Letters
Volume120
Issue number6
DOIs
StatePublished - Feb 9 2018
Externally publishedYes

Funding

The authors want to thank the TRILIS group at TRIUMF for Ti beam development, C. Lotze, T. Wasem, R. Weiß, and the staff of the machine shop of the physics institutes of the JLU Gießen for excellent technical support. This work was partially supported by Canadian agencies NSERC and CFI, U.S.A. NSF (Grants No. PHY-1419765 and No. PHY-1614130) and DOE (Grant No. DE-SC0017649), Brazil’s CNPq (Grant No. 249121/2013-1), United Kingdom’s STFC (Grants No. ST/L005743/1 and No. ST/P005314/1), German institutions DFG (Grants No. FR 601/3-1 and No. SFB1245 and through PRISMA Cluster of Excellence), BMBF (Grants No. 05P15RDFN1 and No. 05P12RGFN8), the Helmholtz Association through NAVI (Grant No. VH-VI-417), HMWK through the LOEWE Center HICforFAIR, and the JLU-GSI partnership. Computations were performed with resources of the Jülich Supercomputing Center (JURECA), GENCI-TGCC (Grant No. 2017-0507392), MSUs iCER and UKs DiRAC Complexity system (Grants No. ST/K000373/1 and No. ST/K0003259/1). TRIUMF receives federal funding via NRC.

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