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A study of the effect of deformation and pairing on the development of halo nuclei is presented. Exploratory three-body calculations show that both the NN interaction and the deformation/excitation of the core hinder the formation of the halo. Preliminary self-consistent mean-field calculations are used to search for regions in the nuclear chart where halos could potentially develop. These are also briefly discussed.

生成讲解博客的中文版本

生成AI智能校验的中文版本