C. Jesch

Dawning of the N=32 shell closure seen through precision mass measurements of neutron-rich titanium isotopes

E. Leistenschneider [1,2,3,4], M. P. Reiter, S. Ayet San Andrés, B. Kootte [1,5], J. D. Holt, P. Navrátil, C. Babcock [1], C. Barbieri [6,1], B. R. Barquest, J. Bergmann [3], J. Bollig [1,7], T. Brunner [1,8], E. Dunling [1,9], A. Finlay [1,2], H. Geissel [3,4], L. Graham [1], F. Greiner [3], H. Hergert [10], C. Hornung [3], C. Jesch [3], R. Klawitter [1,11], Y. Lan [1,2], D. Lascar [1,12], K. G. Leach, W. Lippert [3,1,13,7], J. E. McKay, S. F. Paul, A. Schwenk [11,14,15], D. Short [1,16], J. Simonis [17,18,1,19], V. SomÃ, R. Steinbrügge, S. R. Stroberg, R. Thompson [20], M. E. Wieser, C. Will [3], M. Yavor [21], C. Andreoiu [16], T. Dickel [3,4], I. Dillmann [1,13], G. Gwinner [5,3,4], W. R. Plaß, C. Scheidenberger [3,4,1,13], A. A. Kwiatkowski, J. Dilling [1,2]

Abstract

A precision mass investigation of the neutron-rich titanium isotopes $^{51-55}$Ti 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 $^{52-55}$Ti mass values were significantly reduced. Our results confirm the existence of a weak shell effect at $N=32$, establishing the abrupt onset of this shell closure. Our data were compared with state-of-the-art \textit{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 (MR-TOF-MS), substantiated by independent measurements from TITAN's Penning trap mass spectrometer.