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    Linear correlations related to neutron skin thickness

    Y. Lei (雷杨)1,*, J. Qi (漆洁)2, X. Lian (连新)3, Z. Z. Qin (覃珍珍)2, and C. L. Bai (白春林)3,†

    • *Contact author: leiyang19850228@gmail.com
    • †Contact author: bclphy@scu.edu.cn

    Phys. Rev. C 113, 024314 – Published 11 February, 2026

    DOI: https://doi.org/10.1103/qvsg-hqxm

    Abstract

    Within many-body systems governed by Skyrme density functional, we confirm that the correlations between neutron skin thickness ΔRnp (or charge radius difference of mirror nuclei,ΔRmirr) and the isospin asymmetry (I=N−ZA) persistently emerge, demonstrating the parameter-independent nature of these correlations when using the Skyrme force. We further determine that the slopes of the linear ΔRmirr−I or ΔRnp−I correlations (denoted as Cnp and Cmirr, respectively) are also correlated to the slope of the symmetry energy (L), which may offer a new approach to constrain L while mitigating the influence of density irregularities in specific nuclei. The linear correlations of Cnp−L and Cmirr−L are adopted to constrain L to 12–44 MeV with 1σ confidence. Shape coexistence, or shape effect on charge radius, is considered to explain the experimental deviation of O/Ne18 and some odd-AΔRmirr's from the ΔRmirr−I linearity. Considering the deviation of O/Ne18ΔRmirr due to shape coexistence, the 1σ range for L is further narrowed to 24–40 MeV, suggesting a soft equation of state for nuclear matter.

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