Geometry and electronic structure of monolayer, bilayer, and multilayer Janus WSSe

Newly synthesized Janus transition-metal dichalcogenides MXY ( M = Mo , W; X ≠ Y = S , Se, Te) possess intrinsic Rashba spin splitting and out-of-plane dipole moment due to the breaking of mirror symmetry. Taking WSSe as an example, we present a first-principles investigation of the structural stabi...

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Veröffentlicht in:Physical review. B 2019-02, Vol.99 (7), p.075160, Article 075160
Hauptverfasser: Zhou, Wenzhe, Chen, Jianyong, Yang, Zhixiong, Liu, Junwei, Ouyang, Fangping
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Sprache:eng
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Zusammenfassung:Newly synthesized Janus transition-metal dichalcogenides MXY ( M = Mo , W; X ≠ Y = S , Se, Te) possess intrinsic Rashba spin splitting and out-of-plane dipole moment due to the breaking of mirror symmetry. Taking WSSe as an example, we present a first-principles investigation of the structural stability and electronic properties of mono-, bi-, and multilayer MXY. Results show that S atoms contribute more than Se atoms in the valence-band maximum at the Γ point, which can be greatly affected by interlayer interactions. The high-symmetry AA′ stacking is still the most stable pattern, but there are various orders of chalcogen atomic layers in each stacking. The most preferred order of two adjacent layers is S-Se-Se-S, followed by Se-S-Se-S. The Se-S-Se-S–ordered WSSe bilayer is found to have significant layer splitting due to the net dipole moment, which has great potential for solar cells. Layer-dependent Rashba splittings exist in asymmetry-ordered WSSe bilayers, that can be tuned by changing the interlayer distance, originating from the regulation of interlayer electrostatic interaction. However, there is not layer splitting in a symmetrically stacked WSSe bilayer and opposite Rashba splitting appears in the two layers at a sufficiently large interlayer distance. The electronic structures and spin splittings can be easily modulated by controlling the chalcogen atomic-layer order, so that we can obtain the desired properties from mono-, bi-, and multilayer MXY.
ISSN:2469-9950
2469-9969
DOI:10.1103/PhysRevB.99.075160