Proton Shell Gaps in N=28 Nuclei from the First Complete Spectroscopy Study with FRIB Decay Station Initiator

I. Cox, Z. Y. Xu, R. Grzywacz, W. J. Ong, B. C. Rasco, N. Kitamura, D. Hoskins, S. Neupane, T. J. Ruland, J. M. Allmond, T. T. King, R. S. Lubna, K. P. Rykaczewski, H. Schatz, B. M. Sherrill, O. B. Tarasov, A. D. Ayangeakaa, H. C. Berg, D. L. Bleuel, G. CerizzaJ. Christie, A. Chester, J. Davis, C. Dembski, A. A. Doetsch, J. G. Duarte, A. Estrade, A. Fijałkowska, T. J. Gray, E. C. Good, K. Haak, S. Hanai, J. T. Harke, C. Harris, K. Hermansen, D. E.M. Hoff, R. Jain, M. Karny, K. Kolos, A. Laminack, S. N. Liddick, B. Longfellow, S. Lyons, M. Madurga, M. J. Mogannam, A. Nowicki, T. H. Ogunbeku, G. Owens-Fryar, M. M. Rajabali, A. L. Richard, E. K. Ronning, G. E. Rose, K. Siegl, M. Singh, A. Spyrou, A. Sweet, A. Tsantiri, W. B. Walters, R. Yokoyama

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Abstract

The first complete measurement of the β-decay strength distribution of Cl281745 was performed at the Facility for Rare Isotope Beams (FRIB) with the FRIB Decay Station Initiator during the second FRIB experiment. The measurement involved the detection of neutrons and γ rays in two focal planes of the FRIB Decay Station Initiator in a single experiment for the first time. This enabled an analytical consistency in extracting the β-decay strength distribution over the large range of excitation energies, including neutron unbound states. We observe a rapid increase in the β-decay strength distribution above the neutron separation energy in Ar271845. This was interpreted to be caused by the transitioning of neutrons into protons excited across the Z=20 shell gap. The SDPF-MU interaction with reduced shell gap best reproduced the data. The measurement demonstrates a new approach that is sensitive to the proton shell gap in neutron rich nuclei according to SDPF-MU calculations.

Original languageEnglish
Article number152503
JournalPhysical Review Letters
Volume132
Issue number15
DOIs
StatePublished - Apr 12 2024

Funding

We would like to thank the entire operations team at FRIB for reliable beam delivery during the experiment, and for all the work leading up to the experiment. Calculations for this work were performed using the kshell code . This material is based upon work supported in part by the U.S. Department of Energy, Office of Science, Office of Nuclear Physics under Contracts No. DE-AC52-07NA27344 (LLNL), No. DE-AC05-00OR22725 (ORNL), No. DE-FG02-96ER40983 (UTK), No. DE-SC0016988 (TTU), No. DE-SC0020451 (MSU), Award No. DE-SC0020451 (FRIB), and used resources of the Facility for Rare Isotope Beams (FRIB) Operations, which is a DOE Office of Science User Facility under Award No. DE-SC0023633. This work was also sponsored by the Stewardship Science Academic Alliances program through DOE Awards No. DE-NA0003899 (UTK) and No. DOE-DE-NA0003906 (MSU), NSF Major Research Instrumentation Program Grant No. 1919735 (UTK), and the US National Science Foundation under Grants No. PHY-1714153 (CMU), No. PHY-20-12040 (B.\u2009M.\u2009S., O.\u2009B.\u2009T.), and No. PHY-2209429 (H.\u2009S.). This material is based upon work supported by the Department of Energy National Nuclear Security Administration through the Nuclear Science and Security Consortium under Grant No. DE-NA0003996 and U.S. Department of Energy, National Nuclear Security Administration under Award No. DE-NA0003180 (MSU). S.\u2009L. and J.\u2009D. were supported by the Laboratory Directed Research and Development Program at Pacific Northwest National Laboratory operated by Battelle for the U.S. Department of Energy.

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