Disentangling Orbital and Valley Hall Effects in Bilayers of Transition Metal Dichalcogenides

被引:91
作者
Cysne, Tarik P. [1 ]
Costa, Marcio [1 ]
Canonico, Luis M. [2 ,3 ]
Nardelli, M. Buongiorno [4 ,5 ]
Muniz, R. B. [1 ]
Rappoport, Tatiana G. [6 ,7 ]
机构
[1] Univ Fed Fluminense, Inst Fis, BR-24210346 Niteroi, RJ, Brazil
[2] CSIC, Catalan Inst Nanosci & Nanotechnol ICN2, Campus UAB, Barcelona 08193, Spain
[3] BIST, Campus UAB, Barcelona 08193, Spain
[4] Univ North Texas, Dept Phys, Denton, TX 76203 USA
[5] Univ North Texas, Dept Chem, Denton, TX 76203 USA
[6] Univ Lisbon, Inst Super Tecn, Inst Telecomunicacoes, Ave Rovisco Pais 1, P-1049001 Lisbon, Portugal
[7] Univ Fed Rio de Janeiro, Inst Fis, CP 68528, BR-21941972 Rio De Janeiro, RJ, Brazil
关键词
D O I
10.1103/PhysRevLett.126.056601
中图分类号
O4 [物理学];
学科分类号
0702 ;
摘要
It has been recently shown that monolayers of transition metal dichalcogenides (TMDs) in the 2H structural phase exhibit relatively large orbital Hall conductivity plateaus within their energy band gaps, where their spin Hall conductivities vanish [Canonico et al., Phys. Rev. B 101, 161409 (2020); Bhowal and Satpathy, Phys. Rev. B 102, 035409 (2020)]. However, since the valley Hall effect (VHE) in these systems also generates a transverse flow of orbital angular momentum, it becomes experimentally challenging to distinguish between the two effects in these materials. The VHE requires inversion symmetry breaking to occur, which takes place in the TMD monolayers but not in the bilayers. We show that a bilayer of 2H-MoS2 is an orbital Hall insulator that exhibits a sizeable orbital Hall effect in the absence of both spin and valley Hall effects. This phase can be characterized by an orbital Chern number that assumes the value C-L = 2 for the 2H-MoS2 bilayer and C-L = 1 for the monolayer, confirming the topological nature of these orbital-Hall insulator systems. Our results are based on density functional theory and low-energy effective model calculations and strongly suggest that bilayers of TMDs are highly suitable platforms for direct observation of the orbital Hall insulating phase in two-dimensional materials. Implications of our findings for attempts to observe the VHE in TMD bilayers are also discussed.
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页数:7
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