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填充因子ν = 3/4时的偶数分母分数量子霍尔态

Even-Denominator Fractional Quantum Hall State at Filling Factor ν=3/4.

作者信息

Wang Chengyu, Gupta A, Singh S K, Chung Y J, Pfeiffer L N, West K W, Baldwin K W, Winkler R, Shayegan M

机构信息

Department of Electrical and Computer Engineering, Princeton University, Princeton, New Jersey 08544, USA.

Department of Physics, Northern Illinois University, DeKalb, Illinois 60115, USA.

出版信息

Phys Rev Lett. 2022 Oct 7;129(15):156801. doi: 10.1103/PhysRevLett.129.156801.

Abstract

Fractional quantum Hall states (FQHSs) exemplify exotic phases of low-disorder two-dimensional (2D) electron systems when electron-electron interaction dominates over the thermal and kinetic energies. Particularly intriguing among the FQHSs are those observed at even-denominator Landau level filling factors, as their quasiparticles are generally believed to obey non-Abelian statistics and be of potential use in topological quantum computing. Such states, however, are very rare and fragile, and are typically observed in the excited Landau level of 2D electron systems with the lowest amount of disorder. Here we report the observation of a new and unexpected even-denominator FQHS at filling factor ν=3/4 in a GaAs 2D hole system with an exceptionally high quality (mobility). Our magnetotransport measurements reveal a strong minimum in the longitudinal resistance at ν=3/4, accompanied by a developing Hall plateau centered at (h/e^{2})/(3/4). This even-denominator FQHS is very unusual as it is observed in the lowest Landau level and in a 2D hole system. While its origin is unclear, it is likely a non-Abelian state, emerging from the residual interaction between composite fermions.

摘要

当电子 - 电子相互作用在热能和动能中占主导地位时,分数量子霍尔态(FQHSs)体现了低无序二维(2D)电子系统的奇异相。在FQHSs中,特别引人注目的是那些在偶数分母朗道能级填充因子下观察到的态,因为人们普遍认为它们的准粒子遵循非阿贝尔统计,并且在拓扑量子计算中具有潜在用途。然而,这样的态非常罕见且脆弱,通常在具有最低无序量的2D电子系统的激发朗道能级中观察到。在这里,我们报告在具有极高质量(迁移率)的GaAs二维空穴系统中,在填充因子ν = 3/4处观察到一种新的、意想不到的偶数分母FQHS。我们的磁输运测量揭示了在ν = 3/4处纵向电阻有一个强烈的最小值,同时伴随着一个以(h/e²)/(3/4)为中心发展的霍尔平台。这种偶数分母FQHS非常不寻常,因为它是在最低朗道能级和二维空穴系统中观察到的。虽然其起源尚不清楚,但它可能是一种非阿贝尔态,由复合费米子之间的残余相互作用产生。

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