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
“…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.…”
Atomically thin GaSe has been predicted to have a non-parabolic, Mexican hat-like valence band structure due to the shift of the valence band maximum (VBM) near the Γ point which is expected to give rise to novel, unique properties such as tunable magnetism, high effective mass suppressing direct tunneling in scaled transistors, and an improved thermoelectric figure of merit. However, the synthesis of atomically thin GaSe remains challenging. Here, we report on the growth of atomically thin GaSe by molecular beam epitaxy (MBE) and demonstrate the high quality of the resulting van der Waals epitaxial films. The full valence band structure of nominal bilayer GaSe is revealed by photoemission electron momentum microscopy (k-PEEM), confirming the presence of a distorted valence band near the Γ point. Our results open the way to demonstrating interesting new physical phenomena based on MBE-grown GaSe films and atomically thin monochalcogenides in general.
“…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.…”
Atomically thin GaSe has been predicted to have a non-parabolic, Mexican hat-like valence band structure due to the shift of the valence band maximum (VBM) near the Γ point which is expected to give rise to novel, unique properties such as tunable magnetism, high effective mass suppressing direct tunneling in scaled transistors, and an improved thermoelectric figure of merit. However, the synthesis of atomically thin GaSe remains challenging. Here, we report on the growth of atomically thin GaSe by molecular beam epitaxy (MBE) and demonstrate the high quality of the resulting van der Waals epitaxial films. The full valence band structure of nominal bilayer GaSe is revealed by photoemission electron momentum microscopy (k-PEEM), confirming the presence of a distorted valence band near the Γ point. Our results open the way to demonstrating interesting new physical phenomena based on MBE-grown GaSe films and atomically thin monochalcogenides in general.
“…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%
“…These experiments have identified two main photoluminescence lines, interpreted 30 as a lower energy transition between bands dominated by s and p z orbitals (A-line) and hot luminescence, involving holes in a deeper valence band based on p x and p y orbitals (B-line). The band structure analysis of mono-and few-layer InSe [32][33][34][35][36][37][38][39][40][41][42][43][44][45][46][47][48] has revealed that the conduction and valence band edges near the Γ-point are non-degenerate, being dominated by s and p z orbitals of both metal and chalcogen atoms. Combined with the opposite z → −z (mirror reflection) symmetry of conduction and valence bands, this determines that the transition across the principal band gap has a dominantly electric dipole-like character, coupled to out-of-plane polarized photons.…”
We show that spin-orbit coupling (SOC) in InSe enables the optical transition across the principal band gap to couple with in-plane polarized light. This transition, enabled by px,y ↔ pz hybridization due to intra-atomic SOC in both In and Se, can be viewed as a transition between two dominantly s-and pz-orbital based bands, accompanied by an electron spin-flip. Having parametrized k · p theory using first principles density functional theory we estimate the absorption for σ ± circularly polarized photons in the monolayer as ∼ 1.5%, which saturates to ∼ 0.3% in thicker films (3 − 5 layers). Circularly polarized light can be used to selectively excite electrons into spin-polarized states in the conduction band, which permits optical pumping of the spin polarization of In nuclei through the hyperfine interaction.
“…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.…”
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