InSb岩心空穴电子筛选

IF 1.8 4区 物理与天体物理 Q2 SPECTROSCOPY
A. Alsawi , C.R.J. Sait , D. Hesp , P. Unsworth , M.J. Ashwin , V.R. Dhanak , T.D. Veal , P. Weightman
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引用次数: 0

摘要

应用电位模型分析InSb的螺旋参数与元素材料之间的差异,得出InSb的岩心孔筛分距离为1.82±0.07Å。它也产生了0.22±0.49 e的值在InSb中的电荷转移。利用一种基于量子化原子核心势的新方法,解释了化合物半导体中元素在金属态和原子核心空穴数之间的俄歇参数的变化。原子核心势是一种量子力学观测,它依赖于价荷和原子核心空穴数。岩心孔的筛选距离比最近邻原子间相互作用距离的一半大~ 30%,根据等效岩心模型,预计将是InSb中Sn和Te杂质的筛选半径。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
Core hole electron screening in InSb

The application of a potential model to the analysis of differences between the Auger parameters of InSb and the elemental materials yields a value 1.82±0.07Å for the core hole screening distance in InSb. It also yields a value of 0.22 ± 0.49 e for the charge transfer in InSb. Shifts in the Auger parameters of elements between their metallic states and in a compound semiconductor are interpreted using a novel method based on quantifying atomic core potential, as a quantum mechanical observable, in terms of its dependence on the valence charge and the number of atomic core holes. The core hole screening distance is 30% larger than half the interatomic distance between the nearest neighbors and, by the equivalent cores model, is expected to be the screening radius of Sn and Te impurities in InSb.

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来源期刊
CiteScore
3.30
自引率
5.30%
发文量
64
审稿时长
60 days
期刊介绍: The Journal of Electron Spectroscopy and Related Phenomena publishes experimental, theoretical and applied work in the field of electron spectroscopy and electronic structure, involving techniques which use high energy photons (>10 eV) or electrons as probes or detected particles in the investigation.
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