Investigating nuclear structure near N=32 and N=34: Precision mass measurements of neutron-rich Ca, Ti, and V isotopes

W. S. Porter, E. Dunling, E. Leistenschneider, J. Bergmann, G. Bollen, T. Dickel, K. A. Dietrich, A. Hamaker, Z. Hockenbery, C. Izzo, A. Jacobs, A. Javaji, B. Kootte, Y. Lan, I. Miskun, I. Mukul, T. Murböck, S. F. Paul, W. R. Plaß, D. PuentesM. Redshaw, M. P. Reiter, R. Ringle, J. Ringuette, R. Sandler, C. Scheidenberger, R. Silwal, R. Simpson, C. S. Sumithrarachchi, A. Teigelhöfer, A. A. Valverde, R. Weil, I. T. Yandow, J. Dilling, A. A. Kwiatkowski

Research output: Contribution to journalArticlepeer-review

7 Scopus citations

Abstract

Nuclear mass measurements of isotopes are key to improving our understanding of nuclear structure across the chart of nuclides, in particular, for the determination of the appearance or disappearance of nuclear shell closures. We present high-precision mass measurements of neutron-rich Ca, Ti, and V isotopes performed at TRIUMF's Ion Trap for Atomic and Nuclear science (TITAN) and the Low Energy Beam and Ion Trap (LEBIT) facilities. These measurements were made using the TITAN multiple-reflection time-of-flight mass spectrometer (MR-ToF-MS) and the LEBIT 9.4T Penning trap mass spectrometer. In total, 13 masses were measured, 8 of which represent increases in precision over previous measurements. These measurements refine trends in the mass surface around N=32 and N=34, and support the disappearance of the N=32 shell closure with increasing proton number. Additionally, our data do not support the presence of a shell closure at N=34.

Original languageEnglish
Article number024312
JournalPhysical Review C
Volume106
Issue number2
DOIs
StatePublished - Aug 2022
Externally publishedYes

Funding

We would like to thank J. Lassen and the laser ion source group at TRIUMF for their development of the relevant laser scheme as well as the NSCL staff, the ISAC Beam Delivery group, and M. Good for their technical support. This work was supported by the Natural Sciences and Engineering Research Council (NSERC) of Canada under Grants No. SAPIN-2018-00027, No. RGPAS-2018-522453, and No. SAPPJ-2018-00028, the National Research Council (NRC) of Canada through TRIUMF, the U.S. National Science Foundation through Grants No. PHY-1565546, No. PHY-2111185, and No. PHY-1811855, the U.S. Department of Energy, Office of Science under Grants No. DE-FG02-93ER40789 and No. DE-SC0015927, the German Research Foundation (DFG), Grant No. SCHE 1969/2-1, the German Federal Ministry for Education and Research (BMBF), Grants No. 05P19RGFN1 and No. 05P21RGFN1, and the Hessian Ministry for Science and Art through the LOEWE Center HICforFAIR, by the JLU and GSI under the JLU-GSI strategic Helmholtz partnership agreement. E.D. acknowledges financial support from the U.K.-Canada Foundation.

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