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arXiv:2602.03323·v2·Nuclear Theory

Neutron skin thickness and its volume and surface contributions in berkelium isotopes

Peng Wang · Zi-Dan Huang · Shuang-Quan Zhang · Ting-Ting Sun

Abstract

Accurate determination of the neutron skin thickness () in finite nuclei is essential for constraining the density dependence of the nuclear symmetry energy. This work presents a systematic investigation of for the transuranium berkelium (Bk) isotopes within the framework of the deformed relativistic Hartree-Bogoliubov theory in continuum (DRHBc). The results indicate an overall increase in neutron skin thickness with , which exhibits antikinks at the shell closures due to the shell effects. A decomposition of into volume and surface terms, based on two-parameter Fermi (2pF) fits to angle-averaged DRHBc densities, demonstrates that the volume term dominates as much as -- in most nuclei, consistent with the found in Pb, thereby validating the volume-surface decomposition for deformed nuclei and confirming its correlation with the symmetry energy slope . The surface term prevails only near the proton drip line, where the volume fraction drops below due to the reduced neutron-to-proton ratio. Deformation is found to slightly reduce the central radius but markedly enhance the surface diffuseness , leading to a notable increase in , primarily driven by the surface term. Furthermore, we extend the decomposition to a directional analysis by extracting 2pF parameters along the symmetry axis () and perpendicular to it (). In prolate deformed nuclei, a strong directional dependence is observed: although the nucleus is elongated along the symmetry axis, is significantly larger in the perpendicular direction. This anisotropy is weak for oblate nuclei around the shell closures.

Comments: 11 figures, 13 pages

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