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InSb(111)B 表面上铋薄膜中的谢尔宾斯基结构与电子拓扑

Sierpiński Structure and Electronic Topology in Bi Thin Films on InSb(111)B Surfaces.

作者信息

Liu Chen, Zhou Yinong, Wang Guanyong, Yin Yin, Li Can, Huang Haili, Guan Dandan, Li Yaoyi, Wang Shiyong, Zheng Hao, Liu Canhua, Han Yong, Evans James W, Liu Feng, Jia Jinfeng

机构信息

Key Laboratory of Artificial Structures and Quantum Control (Ministry of Education), Shenyang National Laboratory for Materials Science, School of Physics and Astronomy, Shanghai Jiao Tong University, Shanghai 200240, China.

Department of Materials Science and Engineering, University of Utah, Salt Lake City, Utah 84112, USA.

出版信息

Phys Rev Lett. 2021 Apr 30;126(17):176102. doi: 10.1103/PhysRevLett.126.176102.

Abstract

Deposition of Bi on InSb(111)B reveals a striking Sierpiński-triangle (ST)-like structure in Bi thin films. Such a fractal geometric topology is further shown to turn off the intrinsic electronic topology in a thin film. Relaxation of a huge misfit strain of about 30% to 40% between Bi adlayer and substrate is revealed to drive the ST-like island formation. A Frenkel-Kontrova model is developed to illustrate the enhanced strain relief in the ST islands offsetting the additional step energy cost. Besides a sufficiently large tensile strain, forming ST-like structures also requires larger adlayer-substrate and intra-adlayer elastic stiffnesses, and weaker intra-adlayer interatomic interactions.

摘要

铋在InSb(111)B上的沉积在铋薄膜中揭示了一种惊人的类似谢尔宾斯基三角形(ST)的结构。这种分形几何拓扑结构进一步表明会关闭薄膜中的固有电子拓扑结构。据揭示,铋吸附层与衬底之间约30%至40%的巨大失配应变的弛豫驱动了类似ST岛的形成。开发了一个弗伦克尔-康托罗娃模型来说明ST岛中增强的应变弛豫抵消了额外的台阶能量成本。除了足够大的拉伸应变外,形成类似ST的结构还需要更大的吸附层-衬底和层内弹性刚度,以及较弱的层内原子间相互作用。

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