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    Charge radii of Sn isotopes in the relativistic mean field approximation

    S. Marcos1,*, N. Sandulescu2,†, and R. Niembro1,‡

    • *Contact author: marcoss@unican.es
    • †Contact author: sandulescu@thery.nipne.ro
    • ‡Contact author: niembror@unican.es

    Phys. Rev. C 113, 054304 – Published 14 May, 2026

    DOI: https://doi.org/10.1103/v95x-5fw5

    Abstract

    The kink observed in the nuclear charge radius of Sn isotopes around neutron number N=82 is investigated within the relativistic mean-field framework using the NL3* parameter set. It is shown that the small components of the Dirac spinors for the neutron single-particle states near the Fermi level play a crucial role in forming the kink through their contribution to the proton central potential. In particular, the significant differences between the radial parts of the small components of spin-orbit partner states make neutrons with j=l−1/2 more efficient in increasing the nuclear charge radius than those with j=l+1/2. However, the effect induced by the small components alone does not fully account for the magnitude of the kink observed in Sn isotopes.

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