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Large Band Gap in a Quantum Spin Hall Insulator with Weak Spin–Orbit Coupling
Author(s) -
Wu Zhigang
Publication year - 2018
Publication title -
physica status solidi (rrl) – rapid research letters
Language(s) - English
Resource type - Journals
SCImago Journal Rank - 0.786
H-Index - 68
eISSN - 1862-6270
pISSN - 1862-6254
DOI - 10.1002/pssr.201800141
Subject(s) - condensed matter physics , band gap , physics , spin–orbit interaction , insulator (electricity) , scattering , coupling (piping) , topological insulator , spin (aerodynamics) , materials science , quantum mechanics , optoelectronics , metallurgy , thermodynamics
The typical quantum spin Hall (QSH) insulator acquires its band gap through spin–orbit coupling (SOC). However, the intrinsic SOC in most materials is rather weak and creates small band gaps comparable to k B T . Here, we present a method to open a giant band gap (>1 eV) in a QSH phase with a weak SOC, employing the tight‐binding (TB) Kane–Mele model for the QSH insulator with the additional feature of periodic defects. By tuning the periodicity of structural defects, one can induce the intervalley scattering to open a large band gap, and we show that the characteristic metallic edge modes of a QSH phase persist even with the inclusion of such periodic defects. Our TB calculations show the existence of a Z 2 odd QSH phase in a Kane–Mele model modified to include periodic defects, demonstrating the coexistence of a giant band gap and the QSH effect with weak SOC.