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The energies of the POMO spin up and down orbitais relative to the Dirac points predicted by LDA are -0.5eV and -1.4eV, respectively, i.e, in almost quantitative agreement with the GGA results
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The energies of the POMO spin up and down orbitais relative to the Dirac points predicted by LDA are -0.5eV and -1.4eV, respectively, i.e., in almost quantitative agreement with the GGA results.
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38749107145
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LDA locates these LUMOs between 2 meV and 210 meV above the Dirac point.
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LDA locates these LUMOs between 2 meV and 210 meV above the Dirac point.
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G) was observed when visiting large gate voltages (above 40 V) For the sweep rates used in our experiments (15 V/min), the typical hysteresis was 1.5 V; however, it could be as high as 5 V if the time spent at high voltages was too long. Such hysteresis has been discussed in refs 23 and 24, but the exact cause of this effect is beyond the scope of this paper. Here, we always present the data obtained during sweeps from negative to positive voltages (-45 V → +45 V), and we always made sure that the time spent at -45 V was kept at a minimum.
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G) was observed when visiting large gate voltages (above 40 V) For the sweep rates used in our experiments (15 V/min), the typical hysteresis was 1.5 V; however, it could be as high as 5 V if the time spent at high voltages was too long. Such hysteresis has been discussed in refs 23 and 24, but the exact cause of this effect is beyond the scope of this paper. Here, we always present the data obtained during sweeps from negative to positive voltages (-45 V → +45 V), and we always made sure that the time spent at -45 V was kept at a minimum.
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38749125665
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The broadness of the impurity levels does not strongly influence the simulations
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The broadness of the impurity levels does not strongly influence the simulations.
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