Center for Nuclear Study, The University of Tokyo, Tokyo, Japan.
Department of Physics, The University of Tokyo, Tokyo, Japan.
Nature. 2020 Nov;587(7832):66-71. doi: 10.1038/s41586-020-2848-x. Epub 2020 Nov 4.
Atomic nuclei are composed of a certain number of protons Z and neutrons N. A natural question is how large Z and N can be. The study of superheavy elements explores the large Z limit, and we are still looking for a comprehensive theoretical explanation of the largest possible N for a given Z-the existence limit for the neutron-rich isotopes of a given atomic species, known as the neutron dripline. The neutron dripline of oxygen (Z = 8) can be understood theoretically as the result of single nucleons filling single-particle orbits confined by a mean potential, and experiments confirm this interpretation. However, recent experiments on heavier elements are at odds with this description. Here we show that the neutron dripline from fluorine (Z = 9) to magnesium (Z = 12) can be predicted using a mechanism that goes beyond the single-particle picture: as the number of neutrons increases, the nuclear shape assumes an increasingly ellipsoidal deformation, leading to a higher binding energy. The saturation of this effect (when the nucleus cannot be further deformed) yields the neutron dripline: beyond this maximum N, the isotope is unbound and further neutrons 'drip' out when added. Our calculations are based on a recently developed effective nucleon-nucleon interaction, for which large-scale eigenvalue problems are solved using configuration-interaction simulations. The results obtained show good agreement with experiments, even for excitation energies of low-lying states, up to the nucleus of magnesium-40 (which has 28 neutrons). The proposed mechanism for the formation of the neutron dripline has the potential to stimulate further thinking in the field towards explaining nucleosynthesis with neutron-rich nuclei.
原子核由一定数量的质子 Z 和中子 N 组成。一个自然的问题是 Z 和 N 可以有多大。超重元素的研究探索了 Z 的极限,我们仍在寻找一个综合的理论解释,说明对于给定的 Z,最大可能的 N 是多少——这就是给定原子种类的富中子同位素的存在极限,也被称为中子滴线。氧(Z=8)的中子滴线可以从理论上理解为单个核子填充由平均势限制的单粒子轨道的结果,实验证实了这一解释。然而,最近对较重元素的实验与这一描述不符。在这里,我们表明,从氟(Z=9)到镁(Z=12)的中子滴线可以用一种超越单粒子图像的机制来预测:随着中子数的增加,核形状呈现出越来越椭圆的变形,导致结合能增加。当这种效应达到饱和(当原子核不能进一步变形时),就会得到中子滴线:在这个最大 N 之后,同位素是无束缚的,当添加更多的中子时,它们会“滴落”出来。我们的计算是基于最近开发的有效核子-核子相互作用,对于这个相互作用,我们使用组态相互作用模拟来解决大规模本征值问题。得到的结果与实验很好地吻合,即使对于低激发能的低能态,直到镁-40 核(有 28 个中子)。提出的形成中子滴线的机制有可能激发该领域进一步思考,以解释富中子核的核合成。