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2015
DOI: 10.1038/srep17044
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Spin splitting in 2D monochalcogenide semiconductors

Abstract: We report ab initio calculations of the spin splitting of the uppermost valence band (UVB) and the lowermost conduction band (LCB) in bulk and atomically thin GaS, GaSe, GaTe, and InSe. These layered monochalcogenides appear in four major polytypes depending on the stacking order, except for the monoclinic GaTe. Bulk and few-layer ε-and γ -type, and odd-number β-type GaS, GaSe, and InSe crystals are noncentrosymmetric. The spin splittings of the UVB and the LCB near the Γ-point in the Brillouin zone are finite… Show more

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Cited by 61 publications
(64 citation statements)
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References 56 publications
(100 reference statements)
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“…This feature cannot be explained by the spin-orbit splitting of the topmost band since the predicted value is in the range of only a few meV. 12,29 It is more likely that the subband is arising from the mixed signals of the Γ 1 + band of exposed monolayer GaSe in the examined region, since the energy difference is in line with theoretical calculations. 6,12 It is worth noting that the second topmost band, (Γ 3 − ) lies below the Γ 1 + bands with an energy difference of~1.1 eV at the Γ point, a value which is also comparable with the reported calculations for both the monolayer and bilayer cases making further distinction difficult.…”
Section: Resultssupporting
confidence: 61%
“…This feature cannot be explained by the spin-orbit splitting of the topmost band since the predicted value is in the range of only a few meV. 12,29 It is more likely that the subband is arising from the mixed signals of the Γ 1 + band of exposed monolayer GaSe in the examined region, since the energy difference is in line with theoretical calculations. 6,12 It is worth noting that the second topmost band, (Γ 3 − ) lies below the Γ 1 + bands with an energy difference of~1.1 eV at the Γ point, a value which is also comparable with the reported calculations for both the monolayer and bilayer cases making further distinction difficult.…”
Section: Resultssupporting
confidence: 61%
“…Going on from the monolayer [32][33][34][35][36][37][38][39][40][41][42][43][44][45][46][47][48] to N -layer films, interlayer hopping between successive layers of InSe splits each band into N subbands, as studied earlier using DFT and tight-binding calculations 31,33,39 . At the Γ-point, v 1 and v 2 split very weakly, whereas c and v, which are dominated by s and p z orbitals on In and Se, exhibit a much stronger splitting.…”
Section: Multilayersmentioning
confidence: 99%
“…The values of the k · p parameters listed in Table II are determined 39 from fitting to DFT dispersions without SOC near Γ. The dispersions of these bands coincide with the DFT-calculated Γ-point dispersion of InSe bands [32][33][34][35][36][37][38][39][40][41][42][43][44][45][46][47][48] , but with the band gap corrected by a 'scissor correction' adjustment to the bands 39 . The factors eβ 1 (2) cm e , are couplings of the spin-conserving v 1 → c interband transition (B-line), and of the transition between bands v and v 2 49 , respectively, to in-plane polarized light described by vector potential A = (A x , A y ), with β 1(2) = | c(v)| P |v 1 (v 2 ) | the magnitude of the interband matrix element of the momentum operator.…”
Section: Monolayermentioning
confidence: 99%
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“…22 Additionally we considered other 2D materials such as GaSe. 27 Again, we only consider cases where the energy difference ∆ECV = EC (2) -EV (1) is relatively small, with ∆ECV deduced from the DFT computations (We note that DFT is well known to underestimate experimental band gap values. 28 An approximate correction to the band gaps will cause a right-shift of our results in Fig.…”
Section: Resultsmentioning
confidence: 99%