在铁电半导体中推进巨型拉什巴效应的厚度极限
Boris Croes1, Alexandre Llopez1, Calvin Tagne-Kaegom2
1Aix Marseille Univ, CNRS, CINAM, AMUtech, 13288 Marseille, France.
Nano letters
|October 14, 2024
概括
铁电Rashba半导体 (FERSCs) 呈现出一个巨大的Rashba效应,直至1nm厚度. 这种持久性是由于这些自旋轨道电子材料中的介面反补偿空缺.
科学领域:
- 材料科学 材料科学 材料科学
- 凝聚物质物理学 凝聚物质物理学
- 量子力学就是量子力学.
背景情况:
- 铁电Rashba半导体 (FERSCs) 是节能自旋轨道电子的关键.
- 了解这些效应的厚度极限对于设备应用至关重要.
研究的目的:
- 在α-GeTe薄膜中研究Rashba-Spin-Orbit Coupling (SOC) 效应的最小厚度.
- 探索Rashba效应在减少厚度时持续存在的潜在机制.
主要方法:
- 角度分辨率光辐射光谱学 (ARPES) 探测电子带结构.
- 第一个原则计算用于对原始GeTe的理论分析.
- 射线光辐射光谱学 (XPS) 用于分析薄膜组成和缺陷.
主要成果:
- α-GeTe(111) 薄膜在覆盖着Sb的Si(111) 基板上表现出一个巨大的Rashba效应,厚度低至1纳米.
- 拉什巴常数即使在1nm时也仍然显著 (5.2±0.5 eV·Å).
- XPS揭示了接口Sb原子补偿Ge空位,从而保持Rashba效应.
结论:
- 在α-GeTe中的巨大的Rashba效应是强大的,并持续到超薄膜 (1纳米).
- 使用Sb的接口工程是一种可行的策略,可以在FERSC中保持旋转轨道合效应.
- 这些发现为开发下一代节能自旋轨道电子设备铺平了道路.
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