论文标题

富含中子的核中的壳演化:单个粒子透视

Shell evolution in neutron-rich nuclei: the single particle perspective

论文作者

Ma, Weiqiang, Qian, Yibin

论文摘要

在相互作用的壳模型的框架内广泛研究了壳的演化,而从单个粒子角度进行的研究相对缺乏或忽略。特别是,随着$ N/z $的增加,自旋轨道分裂的同胞依赖性变得越来越重要。遵循最初的独立粒子策略来解释魔术数量的发生,我们系统地研究了同胞素对木材 - 萨克森(WS)平均场势势和旋转轨道项中富含中子核的壳演变的影响。发现新的魔术数量$ n = 14 $和$ n = 16 $可能会在中子富含中子的核中出现,如果一个人在自旋轨道耦合中更改了依赖isospin的术语的符号,而传统的魔术数字$ n = 20 $可能会消失。尽管在旋转轨道分裂中选择了ISOSPIN部分,但魔术数量$ n = 28 $预计将被破坏,而$ n = 50 $可能会消失,$ n = 82 $仍然存在于单个粒子方案中。此外,在中子富含中子的Ca同位素中,出现明显的能量差距为$ n = 32 $和34个。当WS电位的Isospin项的符号与相应的自旋轨耦合部分的符号不同时,所有这些结果与相互作用的壳模型的结果更加一致。本研究不仅可以为相互作用的外壳,而且针对中子二光线的其他核多体计算提供更合理的起点。

The shell evolution has been studied extensively within the framework of interacting shell model, while the studies from the single particle viewpoint is relatively lacking or neglected. In particular, the isospin dependence of spin-orbit splitting has become increasingly important as $N/Z$ increases in neutron-rich nuclei. Following the initial independent-particle strategy towards explaining the occurrence of magic numbers, we have systematically investigated the isospin effect on the shell evolution of neutron-rich nuclei within the Woods-Saxon (WS) mean-field potential plus the spin-orbit term. It is found that new magic numbers $N = 14$ and $N =16$ may emerge in neutron-rich nuclei if one changes the sign of the isospin-dependent term in the spin-orbit coupling while the traditional magic number $N = 20$ may disappear. The magic number $N = 28$ is expected to be destroyed despite the sign choice of the isospin part in spin-orbit splitting, while $N = 50$ may disappear and $N = 82$ persists within the single particle scheme. Besides, an appreciable amount of energy gap appears at $N = 32$ and 34 in neutron-rich Ca isotopes. All these results are more consistent with those of the interacting shell model, when the sign of the isospin term of the WS potential is different from that of the corresponding spin-orbit coupling part. The present study may provide a more reasonable starting point for not only the interacting shell but also other nuclear many-body calculations towards the neutron-dripline.

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