Fig. 3: Quantised orbital Chern insulator at ν = 2 and possible Chern bands. | Nature Communications

Fig. 3: Quantised orbital Chern insulator at ν = 2 and possible Chern bands.

From: Spin-orbit coupling-enhanced valley ordering of malleable bands in twisted bilayer graphene on WSe2

Fig. 3: Quantised orbital Chern insulator at ν = 2 and possible Chern bands.The alternative text for this image may have been generated using AI.

a, b Landau fan diagram in longitudinal resistance Rxx and transverse resistance Rxy plotted as a function of ν for different B up to 10 T. c Fitting of the Diophantine equation along the minima in Rxx and wedge-like states in Rxy. The slopes of the straight lines give the Chern numbers C. d Rxy data at B = 10 T plotted for a small density range near ν = 2 marked by the blue colourbar on the top axis in panel 3c. Rxy is quantised to h/2e2 accompanied by a minima in Rxx at B = 10 T. e Schematic of flat bands with different Chern numbers via valley polarising \({{{{{{{\mathcal{T}}}}}}}}\)-symmetry breaking (TRS) and proximity-induced SOC. The dark and light colours represent each spin-valley flavour’s lower and upper bands, respectively. In the presence of SOC, the spin-valley flavour degeneracy can be completely lifted, leading to 8 isolated bands for appropriate system parameters. Blue(green) and red(yellow) indicate the up and down spin components for valley K(\({K}^{{\prime} }\)). The net Chern number Cnet obtained by adding the Chern numbers of the filled bands at ν = 2 (horizontal black dashed line) is +2 in both cases. f Schematic of valley Chern bands giving rise to Cnet = + 2 at ν = + 2. The band degeneracy can be lifted completely in the presence of SOC and a spin splitting exchange field that naturally accompanies a ferromagnetic spin polarised phase. We have used the SOC parameters for graphene on WSe2 following ref. 43 together with the exchange field λex = 0.5meV as summarised in the methods section. The degeneracy split Chern bands lead to finite orbital magnetism M(orb) that changes with the filling density ν, shown here from −4 to 4 in the right-most sub-panel. We note the changing signs in the total orbital magnetisation due to the relative filling of K(\({K}^{{\prime} }\uparrow\)) bands near ν = + 2, suggesting that delicate changes in level ordering with carrier density due to Coulomb interactions can strongly impact the net magnetisation.

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