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    Ab initio study of spectroscopic factors in K48 and neighboring N=28 isotones

    P. Y. Wang1,2, M. R. Xie3,4,*, Q. Yuan3,4, W. J. Huang1, and J. G. Li3,4,5

    • *Contact author: xiemengran@impcas.ac.cn

    Phys. Rev. C 113, 024305 – Published 4 February, 2026

    DOI: https://doi.org/10.1103/wsdv-6jtv

    Abstract

    A recent K47(d,pγ)K48 transfer reaction measurement identified new excited states in K48 and extracted the corresponding spectroscopic factors (SFs) [C. J. Paxman et al., Phys. Rev. Lett. 134, 162504 (2025)], but exposed sizable discrepancies with large-scale shell-model (LSSM) calculations—especially for the low-lying states—suggesting shortcomings in the proton-neutron interaction employed by the LSSM. In this work, we revisit the low-lying states and SFs of K48 using the ab initio valence-space in-medium similarity renormalization group (VS-IMSRG) approach based on the chiral two- and three-nucleon forces. The calculated excitation energies reproduce the experimental data for K48, whereas computed SFs systematically exceed experimental values. We trace this overestimation to missing reduction factors that account for nonidealities of the transfer reaction. After introducing a phenomenological reduction factor, our VS-IMSRG results and the LSSM calculations achieve agreement with experiment. We also perform the same analysis for the neutron SFs of Ar47. Furthermore, we extend the ab initio calculations across the N=28 isotones, computing excitation energies and single-neutron transfer SFs from N=29 isotones ranging from K48 to S45. By systematically removing protons from K48 to S45, we trace the evolution of the N=28 shell strength via theoretical SFs values. Our results provide a microscopic pathway to quantify the weakening of the N=28 shell closure.

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