Ab initio study of spectroscopic factors in and neighboring isotones
Phys. Rev. C 113, 024305 – Published 4 February, 2026
DOI: https://doi.org/10.1103/wsdv-6jtv
Abstract
A recent transfer reaction measurement identified new excited states in 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 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 , 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 . Furthermore, we extend the ab initio calculations across the isotones, computing excitation energies and single-neutron transfer SFs from isotones ranging from to . By systematically removing protons from to , we trace the evolution of the shell strength via theoretical SFs values. Our results provide a microscopic pathway to quantify the weakening of the shell closure.