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Evolution of shell gaps in the neutron-poor calcium region from invariant-mass spectroscopy of Sc37,38, Ca35, and K34

N. Dronchi1,*, R. J. Charity2, L. G. Sobotka1,2, B. A. Brown3,4, D. Weisshaar3, A. Gade3,4, K. W. Brown3,5, W. Reviol6, D. Bazin3,4 et al.

P. J. Farris3,4, A. M. Hill3,4, J. Li3, B. Longfellow3,4, D. Rhodes3,4, S. N. Paneru3, S. A. Gillespie3, A. K. Anthony3, E. Rubino3, and S. Biswas3

  • *Contact author: n.dronchi@wustl.edu

Phys. Rev. C 110, L031302 – Published 12 September, 2024

DOI: https://doi.org/10.1103/PhysRevC.110.L031302

Abstract

A fast secondary beam of Ca37 impinged on a Be9 target resulting in a set of reactions populating proton-rich nuclei including Ca35 and the first observations of Sc37,38 and K34. Invariant-mass spectroscopy, used to reconstruct proton decays for these nuclei, yielded three new ground-state masses and information on their low-lying structures. The newly measured mass excesses are: ΔM(Sc37)=3500(410)keV, ΔM(Sc38)=−4656(14)keV, and ΔM(K34)=−1487(17)keV. These nuclei straddle the well-known Z=20 shell closure as well as the N=16 subshell closure. Trends in separation energies help elucidate how nuclear structure evolves showing a fading of the Z=20 shell gap for N≤18 and indications of a N=16 subshell gap.

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