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铋表面的自旋轨道劈裂的巨大各向异性。

Giant anisotropy of spin-orbit splitting at the bismuth surface.

机构信息

Synchrotron SOLEIL, L'Orme des Merisiers, Saint-Aubin-BP 48, F-91192 Gif sur Yvette, France.

出版信息

Phys Rev Lett. 2012 Nov 30;109(22):226404. doi: 10.1103/PhysRevLett.109.226404. Epub 2012 Nov 27.

Abstract

We investigate the bismuth (111) surface by means of time and angle resolved photoelectron spectroscopy. The parallel detection of the surface states below and above the Fermi level reveals a giant anisotropy of the spin-orbit spitting. These strong deviations from the Rashba-like coupling cannot be treated in k·p perturbation theory. Instead, first principles calculations could accurately reproduce the experimental dispersion of the electronic states. Our analysis shows that the giant anisotropy of the spin-orbit splitting is due to a large out-of plane buckling of the spin and orbital texture.

摘要

我们通过时间和角度分辨光电子能谱研究了铋(111)表面。费米能级上下表面态的平行探测揭示了自旋轨道劈裂的巨大各向异性。这种强烈偏离拉什巴耦合的现象不能用 k·p 微扰理论来处理。相反,第一性原理计算可以准确地再现电子态的实验色散。我们的分析表明,自旋轨道劈裂的巨大各向异性归因于自旋和轨道织构的大的面外翘曲。

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