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探测锕系元素5f态自旋轨道分裂能级的粒子数。

Probing the population of the spin-orbit split levels in the actinide 5f states.

作者信息

Moore K T, van der Laan G, Tobin J G, Chung B W, Wall M A, Schwartz A J

机构信息

Lawrence Livermore National Laboratory, Livermore, CA 94550, USA.

出版信息

Ultramicroscopy. 2006 Mar;106(4-5):261-8. doi: 10.1016/j.ultramic.2005.08.002. Epub 2005 Nov 4.

Abstract

Spin-orbit interaction in the 5f states is believed to strongly influence exotic behaviors observed in actinide metals and compounds. Understanding these interactions and how they relate to the actinide series is of considerable importance. To address this issue, the branching ratio of the white-line peaks of the N4,5 edge for the light actinide metals, alpha-Th, alpha-U, and alpha-Pu were recorded using electron energy-loss spectroscopy (EELS) in a transmission electron microscope (TEM) and synchrotron-radiation-based X-ray absorption spectroscopy (XAS). Using the spin-orbit sum rule and the branching ratios from both experimental spectra and many-electron atomic spectral calculations, accurate values of the spin-orbit interaction, and thus the relative occupation of the j = 5/2 and 7/2 levels, are determined for the actinide 5f states. Results show that the spin-orbit sum rule works very well with both EELS and XAS spectra, needing little or no correction. This is important, since the high spatial resolution of a TEM can be used to overcome the problems of single-crystal growth often encountered with actinide metals, allowing acquisition of EELS spectra, and subsequent spin-orbit analysis, from nm-sized regions. The relative occupation numbers obtained by our method have been compared with recent theoretical results and they show a good agreement in their trend.

摘要

5f态中的自旋轨道相互作用被认为对锕系金属和化合物中观察到的奇异行为有强烈影响。理解这些相互作用以及它们与锕系元素系列的关系具有相当重要的意义。为了解决这个问题,利用透射电子显微镜(TEM)中的电子能量损失谱(EELS)和基于同步辐射的X射线吸收谱(XAS),记录了轻锕系金属α-Th、α-U和α-Pu的N4,5边白线峰的分支比。利用自旋轨道求和规则以及实验光谱和多电子原子光谱计算得到的分支比,确定了锕系5f态自旋轨道相互作用的精确值,从而确定了j = 5/2和7/2能级的相对占据情况。结果表明,自旋轨道求和规则在EELS和XAS光谱中都能很好地适用,几乎不需要校正。这很重要,因为TEM的高空间分辨率可用于克服锕系金属单晶生长中经常遇到的问题,从而能够从纳米尺寸区域获取EELS光谱并进行后续的自旋轨道分析。通过我们的方法获得的相对占据数已与最近的理论结果进行了比较,它们在趋势上显示出良好的一致性。

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