关于“石墨烯/Co上MoS2单层磁邻近效应的直接光谱证据”的致编辑的信

IF 16 1区 材料科学 Q1 CHEMISTRY, MULTIDISCIPLINARY
ACS Nano Pub Date : 2025-02-25 DOI:10.1021/acsnano.3c09974
Elena Voloshina, Na Zhu, Jiaxin Zhang, Beate Paulus, Yuriy Dedkov
{"title":"关于“石墨烯/Co上MoS2单层磁邻近效应的直接光谱证据”的致编辑的信","authors":"Elena Voloshina, Na Zhu, Jiaxin Zhang, Beate Paulus, Yuriy Dedkov","doi":"10.1021/acsnano.3c09974","DOIUrl":null,"url":null,"abstract":"Let us first compare ARPES and spin-resolved photoemission data presented in two figures from Voroshnin et al.: (27) Figure 2a and Figure 3, respectively. As it is well known and clearly stated in ref (27), “The band structure of MoS<sub>2</sub> depends on the number of layers: in a few-layer stack, the valence-band maximum is located at the Γ̅ point, while in a single-layer it is at K̅. Figure 2a shows that the valence-band maximum is at the K̅ point, demonstrating that the MoS<sub>2</sub> film is one monolayer thick.” This is true for Figure 2a of ref (27), and one can see that the position of the band at the Γ̅ point is by ≈250 meV lower compared to the band position of the upper spin–orbit-split band at the K̅ point. However, if we compare the positions of these bands in Figure 3 of ref (27), then we can see that these bands have the same binding energies, thus contradicting Figure 2a and the statement in the paper. According to Voroshnin et al., (27) the coverage of MoS<sub>2</sub> in the synthesized trilayer is about 0.4 mL. Therefore, the apparent “spin-splitting of MoS<sub>2</sub> states” may actually be the spin-polarized signal, which comes from the graphene/Co(0001) support underneath MoS<sub>2</sub>. Particularly, it can happen for the photon energy of 20 eV, which was used for the spin-resolved photoemission experiments. At this photon energy, the photoemission cross section for the Mo 4<i>d</i> and S 3<i>p</i> valence band states is larger compared to the value for Co 3<i>d</i> by a factor of ≈6 and ≈1.5, respectively. However, in the photoemission experiments, this difference is partly compensated by the noncomplete coverage for the MoS<sub>2</sub> layer, that leaves some parts of the gr/Co(0001) support naked to the light. In this case, the contribution of the spin-polarized photoemission signal, which originates from the gr/Co(0001) support, to the total photoemission picture is expected to be very significant. The evidence that the background photoemission signal from gr/Co(0001) is spin-polarized is the shift of two curves, spin-up and spin-down, in the vertical direction in Figure 3a, c, and e of ref (27), and the spin-polarized (or spin-split) intensity “bump” is clearly visible at 0.9 eV in Figure 3a ref (27). Moreover, the previous spin-resolved photoemission data for gr/Co(0001) measured at the Γ point clearly demonstrate the strong variation of the spin polarization (in value and in sign) in the range of 2 eV below the Fermi level, (33) i.e., exactly in the energy range where spin-resolved experiments for MoS<sub>2</sub> on gr/Co(0001) are presented in ref (27). [The photon energy used in ref (33) is different from the one used in the discussed work. (27) However, taking into account the band structure of gr/Co(0001), a similar strong variation of the spin-polarization is expected.] Unfortunately, such reference spin-resolved photoemissions at a photon energy of 20 eV for the gr/Co(0001) system are not presented in ref (27). Therefore, without such reference data, one cannot unequivocally claim that presented spin-splitting observed for the MoS<sub>2</sub>-derived states is due to the intrinsic spin-polarization of the MoS<sub>2</sub> states. Moreover, using the parameters which can be considered as very close to the real ones used in the discussed experiment, (27) we present a very rough example of how the spin-splitting in the background signal (with spin-splitting of 1 eV) can introduce the “spin-splitting” of 30 meV for the band which is not originally spin-polarized (Figure 1). Here, spin-up and spin-down Lorentzians simulate the photoemission intensity from the respective exchange-split states of the ferromagnetic substrate. If we compare data in Figure 3a of ref (27) and Figure 1 of the present work, we can clearly see that the claimed effect is clearly reproduced, however, without intrinsic spin-polarization for the initially non-spin-polarized emission line. These simulations do not pretend on the completeness and cannot be considered as an attempt to simulate the experimental data presented in ref (27), but they point out the importance of preliminary reference data for gr/Co(0001) (used as a support for the MoS<sub>2</sub> growth), which are unfortunately missed in the original work. Here, we also would like to note that in ref (27) the energy resolutions of 10 and 45 meV are claimed for ARPES and spin-resolved ARPES experiments at room temperature, respectively. However, the dominant factor in such experiments is the thermal broadening caused by the sample’s temperature, which amounts to Δ<i>E</i> ≈ 4<i>k</i><sub>B</sub><i>T</i> ≈ 120 meV, (34) which is much large compared to the claimed exchange spin-splitting of 20 meV for the MoS<sub>2</sub>-derived band at the Γ point and claimed energy resolutions. In Voroshnin et al., (27) the crystallographic structures of the resulting system for which ARPES and spin-resolved photoemission data are presented do not correspond to the crystallographic structures which were used for the interpretation of spin-resolved photoemission data and in the DFT calculations. Moreover, only one model was used in the DFT calculations ignoring other possibilities as discussed below in Results and Discussion. Figure 1. Formation of the “artificial” spin-polarization in the initially non-spin-polarized peak by the spin-polarized photoemission background signal (for details, see the text). The authors of ref (27) use a very thin Co slab of only 4 monolayers (ML). This is an insufficient thickness, in general, which is also very critical when working with magnetic systems. However, even more serious is the lack of passivation of the bottom layer of the slab by adatoms. The approach where the bottom layer of the thin metallic slab is passivated with adatoms, such as H or Al, is a common practice in computation materials modeling. This is especially important for consideration of spin–orbit-related and exchange-splitting effects because of the inversion-symmetry breaking necessary in this case. (35,36) Also such layers protect the magnetic exchange interaction between slabs which can cause artifacts in the calculations. In our work, we have performed the calculations for (4 × 4)MoS<sub>2</sub>/(5 × 5)graphene/Co(0001) with the distances reported by Voroshnin et al. (27) with and without Al passivation. The results of these calculations allow us to conclude that the claimed ref (27) spin-splitting of the MoS<sub>2</sub>-derived states at the Γ point is an artifact due to the wrong computational approach (see discussion below and in Methods). We are considering a supercell that has the periodicity that was observed in the experiment, namely, a (9 × 9) lateral periodicity with respect to graphene and Co(0001) and a (7 × 7) lateral periodicity with respect to MoS<sub>2</sub> (the resulting structure in our paper is approximately four times larger as compared to the model used in Voroshnin et al.). This way, the lattice mismatch of both two-dimensional materials, graphene and MoS<sub>2</sub>, is less than 1%. In our work, the slabs have sufficient thickness with the bottom side of each slab protected by a layer of adatoms. Taking into account the synthesis conditions and experimental observations, we take into account the possible intercalation of S and the formation of CoS<sub><i>x</i></sub>. This results in the consideration of six possible structures (instead of one random structure, which does not correspond to the experimental situation, investigated by Voroshnin et al. (27)). We use the same code (see Methods) for the structure optimization and for calculating the band structures. For each structure, all calculated parameters are extracted from the same output file. Furthermore, we present all computational details so that the results can be clearly reproduced by any qualified reader. We disclose all our results: We present the optimized structures (see all Supporting Information) .txt files: S1, S2, S3, S4, S5, and S6), optimized distances (see Results and Discussion), and calculated band structures in the ranges where graphene- and MoS<sub>2</sub>-valence band states are visible (see Results and Discussion). Figure 2. Optimized crystallographic structures (top and side views) of the MoS<sub>2</sub>-graphene heterostructures on ferromagnetic Co(0001) considered in this work. The red rhombus marks the unit cell. Figure 3. (a, b) Crystallographic structure of the lattice-matched graphene/Co(0001) interface: top (a) and side (b) views. (c) Spin-resolved band structure of graphene/Co(0001) in the vicinity of the K point. (d) Spin-resolved band structure of free-standing MoS<sub>2</sub>. All visible spin-splittings are due to the spin–orbit interaction. Total energy (<i>E</i><sub>tot</sub>, in eV per unit cell), mean distances between different layers in the optimized structures (for details, see Figure 2: <i>d</i>(gr-S1), <i>d</i>(gr-Co), <i>d</i>(S1–Co), <i>d</i>(Mo-Co), <i>d</i>(gr-S<sup>int</sup>), <i>d</i>(S1–S<sup>int</sup>), in Å), corrugation of the graphene layer (gr-corr., in Å), average magnetic moments of Mo, S, C, and Co (<i>m</i>(Mo), <i>m</i>(S1), <i>m</i>(S2), <i>m</i>(S<sup>int</sup>), <i>m</i>(C1), <i>m</i>(C2), <i>m</i>(Co1), <i>m</i>(Co2), <i>m</i>(Co3), in μ<sub>B</sub> per atom). Figure 4. Spin-resolved band structures of the MoS<sub>2</sub>-graphene heterostructures on ferromagnetic Co(0001) obtained after the unfolding procedure for the graphene (1 × 1) primitive cell (left) and MoS<sub>2</sub> (1 × 1) primitive cell (right). Size of the filled circles gives the number of primitive cell bands crossing particular (<i>k</i>, <i>E</i>) in the unfolding procedure, that is, the partial density of states at (<i>k</i>, <i>E</i>) for graphene (left) and MoS<sub>2</sub> (right), respectively. √, experimental observable is reproduced in calculations; x, experimental observable is not reproduced in calculations. Figure 5. Effect of the bottom passivation of the MoS<sub>2</sub>/gr/Co(0001) slab by Al atoms: (a) no passivation by Al, with exchange splitting of the MoS<sub>2</sub>-derived states and (b) bottom is passivated by Al, without exchange splitting of the MoS<sub>2</sub>-derived states. The area of interest is marked by the green rectangle. The Supporting Information is available free of charge at https://pubs.acs.org/doi/10.1021/acsnano.3c09974. S1: Structural data for MoS<sub>2</sub>/gr/Co(0001) (TXT) S2: Structural data for gr/MoS<sub>2</sub>/Co(0001) (TXT) S3: Structural data for MoS<sub>2</sub>/gr/CoS<sub><i>x</i></sub>/Co(0001) (TXT) S4: Structural data for gr/MoS<sub>2</sub>/CoS<sub><i>x</i></sub>/Co(0001) (TXT) S5: Structural data for MoS<sub>2</sub>/gr/S<sup>int</sup>/Co(0001) (TXT) S6: Structural data for gr/MoS<sub>2</sub>/S<sup>int</sup>/Co(0001) (TXT) Letter to the Editor\nConcerning “Direct Spectroscopic\nEvidence of Magnetic Proximity Effect in MoS<sub>2</sub> Monolayer\non Graphene/Co” <span> 3 </span><span> views </span> <span> 0 </span><span> shares </span> <span> 0 </span><span> downloads </span> Most electronic Supporting Information files are available without a subscription to ACS Web Editions. Such files may be downloaded by article for research use (if there is a public use license linked to the relevant article, that license may permit other uses). Permission may be obtained from ACS for other uses through requests via the RightsLink permission system: http://pubs.acs.org/page/copyright/permissions.html. The authors thank the National Natural Science Foundation of China (Grant No. 22272104) for financial support. E.V. and B.P. gratefully acknowledge the computing time granted by the Resource Allocation Board and provided on the supercomputer Lise and Emmy at NHR@ZIB and NHR@Göttingen as part of the NHR infrastructure. The calculations for this research were conducted with computing resources under the project bec00256. This article references 53 other publications. This article has not yet been cited by other publications.","PeriodicalId":21,"journal":{"name":"ACS Nano","volume":"26 1","pages":""},"PeriodicalIF":16.0000,"publicationDate":"2025-02-25","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"0","resultStr":"{\"title\":\"Letter to the Editor Concerning “Direct Spectroscopic Evidence of Magnetic Proximity Effect in MoS2 Monolayer on Graphene/Co”\",\"authors\":\"Elena Voloshina, Na Zhu, Jiaxin Zhang, Beate Paulus, Yuriy Dedkov\",\"doi\":\"10.1021/acsnano.3c09974\",\"DOIUrl\":null,\"url\":null,\"abstract\":\"Let us first compare ARPES and spin-resolved photoemission data presented in two figures from Voroshnin et al.: (27) Figure 2a and Figure 3, respectively. As it is well known and clearly stated in ref (27), “The band structure of MoS<sub>2</sub> depends on the number of layers: in a few-layer stack, the valence-band maximum is located at the Γ̅ point, while in a single-layer it is at K̅. Figure 2a shows that the valence-band maximum is at the K̅ point, demonstrating that the MoS<sub>2</sub> film is one monolayer thick.” This is true for Figure 2a of ref (27), and one can see that the position of the band at the Γ̅ point is by ≈250 meV lower compared to the band position of the upper spin–orbit-split band at the K̅ point. However, if we compare the positions of these bands in Figure 3 of ref (27), then we can see that these bands have the same binding energies, thus contradicting Figure 2a and the statement in the paper. According to Voroshnin et al., (27) the coverage of MoS<sub>2</sub> in the synthesized trilayer is about 0.4 mL. Therefore, the apparent “spin-splitting of MoS<sub>2</sub> states” may actually be the spin-polarized signal, which comes from the graphene/Co(0001) support underneath MoS<sub>2</sub>. Particularly, it can happen for the photon energy of 20 eV, which was used for the spin-resolved photoemission experiments. At this photon energy, the photoemission cross section for the Mo 4<i>d</i> and S 3<i>p</i> valence band states is larger compared to the value for Co 3<i>d</i> by a factor of ≈6 and ≈1.5, respectively. However, in the photoemission experiments, this difference is partly compensated by the noncomplete coverage for the MoS<sub>2</sub> layer, that leaves some parts of the gr/Co(0001) support naked to the light. In this case, the contribution of the spin-polarized photoemission signal, which originates from the gr/Co(0001) support, to the total photoemission picture is expected to be very significant. The evidence that the background photoemission signal from gr/Co(0001) is spin-polarized is the shift of two curves, spin-up and spin-down, in the vertical direction in Figure 3a, c, and e of ref (27), and the spin-polarized (or spin-split) intensity “bump” is clearly visible at 0.9 eV in Figure 3a ref (27). Moreover, the previous spin-resolved photoemission data for gr/Co(0001) measured at the Γ point clearly demonstrate the strong variation of the spin polarization (in value and in sign) in the range of 2 eV below the Fermi level, (33) i.e., exactly in the energy range where spin-resolved experiments for MoS<sub>2</sub> on gr/Co(0001) are presented in ref (27). [The photon energy used in ref (33) is different from the one used in the discussed work. (27) However, taking into account the band structure of gr/Co(0001), a similar strong variation of the spin-polarization is expected.] Unfortunately, such reference spin-resolved photoemissions at a photon energy of 20 eV for the gr/Co(0001) system are not presented in ref (27). Therefore, without such reference data, one cannot unequivocally claim that presented spin-splitting observed for the MoS<sub>2</sub>-derived states is due to the intrinsic spin-polarization of the MoS<sub>2</sub> states. Moreover, using the parameters which can be considered as very close to the real ones used in the discussed experiment, (27) we present a very rough example of how the spin-splitting in the background signal (with spin-splitting of 1 eV) can introduce the “spin-splitting” of 30 meV for the band which is not originally spin-polarized (Figure 1). Here, spin-up and spin-down Lorentzians simulate the photoemission intensity from the respective exchange-split states of the ferromagnetic substrate. If we compare data in Figure 3a of ref (27) and Figure 1 of the present work, we can clearly see that the claimed effect is clearly reproduced, however, without intrinsic spin-polarization for the initially non-spin-polarized emission line. These simulations do not pretend on the completeness and cannot be considered as an attempt to simulate the experimental data presented in ref (27), but they point out the importance of preliminary reference data for gr/Co(0001) (used as a support for the MoS<sub>2</sub> growth), which are unfortunately missed in the original work. Here, we also would like to note that in ref (27) the energy resolutions of 10 and 45 meV are claimed for ARPES and spin-resolved ARPES experiments at room temperature, respectively. However, the dominant factor in such experiments is the thermal broadening caused by the sample’s temperature, which amounts to Δ<i>E</i> ≈ 4<i>k</i><sub>B</sub><i>T</i> ≈ 120 meV, (34) which is much large compared to the claimed exchange spin-splitting of 20 meV for the MoS<sub>2</sub>-derived band at the Γ point and claimed energy resolutions. In Voroshnin et al., (27) the crystallographic structures of the resulting system for which ARPES and spin-resolved photoemission data are presented do not correspond to the crystallographic structures which were used for the interpretation of spin-resolved photoemission data and in the DFT calculations. Moreover, only one model was used in the DFT calculations ignoring other possibilities as discussed below in Results and Discussion. Figure 1. Formation of the “artificial” spin-polarization in the initially non-spin-polarized peak by the spin-polarized photoemission background signal (for details, see the text). The authors of ref (27) use a very thin Co slab of only 4 monolayers (ML). This is an insufficient thickness, in general, which is also very critical when working with magnetic systems. However, even more serious is the lack of passivation of the bottom layer of the slab by adatoms. The approach where the bottom layer of the thin metallic slab is passivated with adatoms, such as H or Al, is a common practice in computation materials modeling. This is especially important for consideration of spin–orbit-related and exchange-splitting effects because of the inversion-symmetry breaking necessary in this case. (35,36) Also such layers protect the magnetic exchange interaction between slabs which can cause artifacts in the calculations. In our work, we have performed the calculations for (4 × 4)MoS<sub>2</sub>/(5 × 5)graphene/Co(0001) with the distances reported by Voroshnin et al. (27) with and without Al passivation. The results of these calculations allow us to conclude that the claimed ref (27) spin-splitting of the MoS<sub>2</sub>-derived states at the Γ point is an artifact due to the wrong computational approach (see discussion below and in Methods). We are considering a supercell that has the periodicity that was observed in the experiment, namely, a (9 × 9) lateral periodicity with respect to graphene and Co(0001) and a (7 × 7) lateral periodicity with respect to MoS<sub>2</sub> (the resulting structure in our paper is approximately four times larger as compared to the model used in Voroshnin et al.). This way, the lattice mismatch of both two-dimensional materials, graphene and MoS<sub>2</sub>, is less than 1%. In our work, the slabs have sufficient thickness with the bottom side of each slab protected by a layer of adatoms. Taking into account the synthesis conditions and experimental observations, we take into account the possible intercalation of S and the formation of CoS<sub><i>x</i></sub>. This results in the consideration of six possible structures (instead of one random structure, which does not correspond to the experimental situation, investigated by Voroshnin et al. (27)). We use the same code (see Methods) for the structure optimization and for calculating the band structures. For each structure, all calculated parameters are extracted from the same output file. Furthermore, we present all computational details so that the results can be clearly reproduced by any qualified reader. We disclose all our results: We present the optimized structures (see all Supporting Information) .txt files: S1, S2, S3, S4, S5, and S6), optimized distances (see Results and Discussion), and calculated band structures in the ranges where graphene- and MoS<sub>2</sub>-valence band states are visible (see Results and Discussion). Figure 2. Optimized crystallographic structures (top and side views) of the MoS<sub>2</sub>-graphene heterostructures on ferromagnetic Co(0001) considered in this work. The red rhombus marks the unit cell. Figure 3. (a, b) Crystallographic structure of the lattice-matched graphene/Co(0001) interface: top (a) and side (b) views. (c) Spin-resolved band structure of graphene/Co(0001) in the vicinity of the K point. (d) Spin-resolved band structure of free-standing MoS<sub>2</sub>. All visible spin-splittings are due to the spin–orbit interaction. Total energy (<i>E</i><sub>tot</sub>, in eV per unit cell), mean distances between different layers in the optimized structures (for details, see Figure 2: <i>d</i>(gr-S1), <i>d</i>(gr-Co), <i>d</i>(S1–Co), <i>d</i>(Mo-Co), <i>d</i>(gr-S<sup>int</sup>), <i>d</i>(S1–S<sup>int</sup>), in Å), corrugation of the graphene layer (gr-corr., in Å), average magnetic moments of Mo, S, C, and Co (<i>m</i>(Mo), <i>m</i>(S1), <i>m</i>(S2), <i>m</i>(S<sup>int</sup>), <i>m</i>(C1), <i>m</i>(C2), <i>m</i>(Co1), <i>m</i>(Co2), <i>m</i>(Co3), in μ<sub>B</sub> per atom). Figure 4. Spin-resolved band structures of the MoS<sub>2</sub>-graphene heterostructures on ferromagnetic Co(0001) obtained after the unfolding procedure for the graphene (1 × 1) primitive cell (left) and MoS<sub>2</sub> (1 × 1) primitive cell (right). Size of the filled circles gives the number of primitive cell bands crossing particular (<i>k</i>, <i>E</i>) in the unfolding procedure, that is, the partial density of states at (<i>k</i>, <i>E</i>) for graphene (left) and MoS<sub>2</sub> (right), respectively. √, experimental observable is reproduced in calculations; x, experimental observable is not reproduced in calculations. Figure 5. Effect of the bottom passivation of the MoS<sub>2</sub>/gr/Co(0001) slab by Al atoms: (a) no passivation by Al, with exchange splitting of the MoS<sub>2</sub>-derived states and (b) bottom is passivated by Al, without exchange splitting of the MoS<sub>2</sub>-derived states. The area of interest is marked by the green rectangle. The Supporting Information is available free of charge at https://pubs.acs.org/doi/10.1021/acsnano.3c09974. S1: Structural data for MoS<sub>2</sub>/gr/Co(0001) (TXT) S2: Structural data for gr/MoS<sub>2</sub>/Co(0001) (TXT) S3: Structural data for MoS<sub>2</sub>/gr/CoS<sub><i>x</i></sub>/Co(0001) (TXT) S4: Structural data for gr/MoS<sub>2</sub>/CoS<sub><i>x</i></sub>/Co(0001) (TXT) S5: Structural data for MoS<sub>2</sub>/gr/S<sup>int</sup>/Co(0001) (TXT) S6: Structural data for gr/MoS<sub>2</sub>/S<sup>int</sup>/Co(0001) (TXT) Letter to the Editor\\nConcerning “Direct Spectroscopic\\nEvidence of Magnetic Proximity Effect in MoS<sub>2</sub> Monolayer\\non Graphene/Co” <span> 3 </span><span> views </span> <span> 0 </span><span> shares </span> <span> 0 </span><span> downloads </span> Most electronic Supporting Information files are available without a subscription to ACS Web Editions. Such files may be downloaded by article for research use (if there is a public use license linked to the relevant article, that license may permit other uses). Permission may be obtained from ACS for other uses through requests via the RightsLink permission system: http://pubs.acs.org/page/copyright/permissions.html. The authors thank the National Natural Science Foundation of China (Grant No. 22272104) for financial support. E.V. and B.P. gratefully acknowledge the computing time granted by the Resource Allocation Board and provided on the supercomputer Lise and Emmy at NHR@ZIB and NHR@Göttingen as part of the NHR infrastructure. The calculations for this research were conducted with computing resources under the project bec00256. This article references 53 other publications. 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摘要

让我们首先比较Voroshnin等人提供的两张图中的ARPES和自旋分辨光电发射数据:(27)分别图2a和图3。众所周知,在文献(27)中明确指出,“二硫化钼的能带结构取决于层数:在几层堆叠中,价带最大值位于Γ′s点,而在单层中,价带最大值位于K′s点。”图2a显示,价带最大值出现在K′s点,表明二硫化钼薄膜厚度为一层。在文献(27)的图2a中也是如此,我们可以看到,与K′s点上的自旋轨道分裂带的能带位置相比,Γ′s点处的能带位置要低约250 meV。但是,如果我们比较ref(27)的图3中这些带的位置,我们可以看到这些带具有相同的结合能,这与图2a和文中的陈述相矛盾。根据Voroshnin等人的研究,(27)在合成的三层中MoS2的覆盖率约为0.4 mL。因此,表面上的“MoS2状态的自旋分裂”实际上可能是自旋极化信号,它来自于MoS2下面的石墨烯/Co(0001)支撑体。特别是对于用于自旋分辨光发射实验的光子能量为20 eV时,可以发生这种情况。在此光子能量下,mo4d和s3p价带态的光发射截面分别比co3d的值大约6倍和约1.5倍。然而,在光电发射实验中,这种差异部分地被MoS2层的不完全覆盖所补偿,这使得gr/Co(0001)支架的某些部分裸露在光下。在这种情况下,来自gr/Co(0001)支撑体的自旋极化光发射信号对总光发射图像的贡献预计是非常显著的。gr/Co(0001)的背景光发射信号是自旋极化的证据是参考文献(27)的图3a、c和e在垂直方向上的自旋向上和自旋向下两条曲线的位移,并且在图3a参考文献(27)的0.9 eV处可以清楚地看到自旋极化(或自旋分裂)强度“凸起”。此外,先前在Γ点测量的gr/Co(0001)的自旋分辨光发射数据清楚地表明,在费米能级(33)以下的2ev范围内,自旋极化(在值和符号上)发生了强烈变化,即,正好在参考文献(27)中提出的gr/Co(0001)上的MoS2自旋分辨实验的能量范围内。[参考文献(33)中使用的光子能量与讨论工作中使用的光子能量不同。](27)然而,考虑到gr/Co(0001)的能带结构,预计自旋极化也会有类似的强烈变化。不幸的是,gr/Co(0001)系统在光子能量为20 eV时的参考自旋分辨光发射在文献(27)中没有给出。因此,如果没有这些参考数据,我们就不能明确地说,在MoS2衍生态中观察到的自旋分裂是由于MoS2态的固有自旋极化所致。此外,使用的参数可以被视为非常接近真正的讨论中使用的实验中,(27)我们提出一个非常粗糙的例子在后台spin-splitting信号(spin-splitting 1 eV)可以介绍30兆电子伏的“spin-splitting”乐队不是最初自旋极化(图1)。在这里,向上和向下的洛伦兹模拟各自的光电发射强度exchange-split铁磁衬底的州。如果我们比较文献(27)的图3a和本工作的图1中的数据,我们可以清楚地看到,所声称的效应被清楚地再现了,然而,对于最初非自旋极化的发射线,没有固有的自旋极化。这些模拟并没有假装完整性,也不能被认为是试图模拟参考文献(27)中提出的实验数据,但它们指出了gr/Co(0001)的初步参考数据的重要性(用于支持MoS2生长),不幸的是,这些数据在原始工作中被遗漏了。在这里,我们还想指出,在参考文献(27)中,室温下的ARPES和自旋分辨ARPES实验分别声称能量分辨率为10和45 meV。然而,这些实验中的主要因素是样品温度引起的热展宽,其值为ΔE≈4kBT≈120 meV,(34)与声称的在Γ点mos2衍生带的交换自旋分裂20 meV和声称的能量分辨率相比要大得多。在Voroshnin等人的(27)中,ARPES和自旋分辨光发射数据所呈现的结果系统的晶体结构与用于解释自旋分辨光发射数据和DFT计算的晶体结构并不对应。 此外,在DFT计算中只使用了一个模型,忽略了下面结果和讨论中讨论的其他可能性。图1所示。自旋极化光发射背景信号在初始非自旋极化峰形成“人工”自旋极化(详见正文)。参考文献(27)的作者使用了只有4层单层(ML)的非常薄的Co板。这是一个不足的厚度,在一般情况下,这也是非常关键的,当工作与磁性系统。然而,更严重的是缺乏对板坯底层的钝化。将薄金属板的底层用氢或铝等原子钝化的方法是计算材料建模中的常用方法。这对于考虑自旋轨道相关效应和交换分裂效应尤其重要,因为在这种情况下需要逆对称破缺。(35,36)此外,这些层保护板之间的磁交换相互作用,这可能导致计算中的伪像。在我们的工作中,我们对(4 × 4)MoS2/(5 × 5)石墨烯/Co(0001)进行了计算,其距离由Voroshnin等人(27)报道,有和没有铝钝化。这些计算的结果使我们可以得出结论,声称的参考文献(27)在Γ点的mos2衍生态的自旋分裂是由于错误的计算方法造成的伪产物(参见下面的讨论和方法)。我们正在考虑一个具有实验中观察到的周期性的超级单体,即石墨烯和Co(0001)的(9 × 9)横向周期性和MoS2的(7 × 7)横向周期性(我们论文中得到的结构与Voroshnin等人使用的模型相比大约大4倍)。这样,石墨烯和二硫化钼这两种二维材料的晶格错配小于1%。在我们的工作中,楼板有足够的厚度,每块楼板的底部都有一层硅原子保护。考虑到合成条件和实验观察,我们考虑了S的可能插层和CoSx的形成。这导致考虑了六种可能的结构(而不是Voroshnin等人(27)研究的一种随机结构,这与实验情况不相符)。我们使用相同的代码(见方法)进行结构优化和计算频带结构。对于每个结构,所有计算的参数都是从相同的输出文件中提取的。此外,我们提供了所有的计算细节,以便任何合格的读者都可以清楚地复制结果。我们公开了我们所有的结果:我们提出了优化的结构(见所有支持信息). txt文件:S1, S2, S3, S4, S5和S6),优化的距离(见结果和讨论),并计算了石墨烯和mos2价带态可见范围内的能带结构(见结果和讨论)。图2。本研究考虑了铁磁Co(0001)上mos2 -石墨烯异质结构的优化晶体结构(顶部和侧面视图)。红色菱形标志着单元格。图3。(a, b)晶格匹配石墨烯/Co(0001)界面的晶体结构:顶部(a)和侧面(b)视图。(c)石墨烯/Co(0001)在K点附近的自旋分辨能带结构。(d)独立MoS2的自旋分辨能带结构。所有可见的自旋分裂都是由于自旋轨道相互作用。总能量(Etot,单位为eV / cell),优化结构中不同层之间的平均距离(详细信息见图2:d(gr-S1), d(gr-Co), d(S1-Co), d(Mo-Co), d(gr-Sint), d(S1-Sint), Å),石墨烯层的波纹(gr-corr)。,参见Å), Mo、S、C和Co的平均磁矩(m(Mo)、m(S1)、m(S2)、m(Sint)、m(C1)、m(C2)、m(Co1)、m(Co2)、m(Co3),单位μB /原子)。图4。石墨烯(1 × 1)原始细胞(左)和MoS2 (1 × 1)原始细胞(右)展开后,在铁磁Co(0001)上得到了MoS2-石墨烯异质结构的自旋分辨带结构。填充圆的大小给出了展开过程中穿过特定(k, E)的原始细胞带的数量,即石墨烯(左)和MoS2(右)分别在(k, E)处的态偏密度。√,实验观测值在计算中重现;X,实验观察不能在计算中重现。图5。Al原子对MoS2/gr/Co(0001)板坯底部钝化的影响:(a)无Al钝化,MoS2衍生态发生交换分裂;(b)底部钝化,MoS2衍生态没有交换分裂。感兴趣的区域用绿色矩形标记。支持信息可在https://pubs.acs.org/doi/10.1021/acsnano.3c09974免费获取。 S1: MoS2/gr/Co(0001)结构数据(TXT) S2: gr/MoS2/Co(0001)结构数据(TXT) S3: MoS2/gr/CoSx/Co(0001)结构数据(TXT) S4: gr/MoS2/CoSx/Co(0001)结构数据(TXT) S5: MoS2/gr/Sint/Co(0001)结构数据(TXT) S6:gr/MoS2/Sint/Co的结构数据(0001)(TXT)致编辑的信关于“MoS2单层石墨烯/Co中磁邻近效应的直接光谱证据”3次浏览0次分享0次下载大多数电子支持信息文件无需订阅ACS网络版即可获得。这些文件可以通过文章下载用于研究用途(如果相关文章有公共使用许可链接,该许可可以允许其他用途)。如有其他用途,可通过RightsLink权限系统http://pubs.acs.org/page/copyright/permissions.html向ACS申请。作者感谢国家自然科学基金(资助号:22272104)的资助。E.V.和B.P.感谢资源分配委员会授予的计算时间,并在超级计算机Lise和Emmy (NHR@ZIB和NHR@Göttingen)上提供计算时间,作为NHR基础设施的一部分。本研究的计算使用bec00256项目下的计算资源进行。本文引用了53个其他出版物。这篇文章尚未被其他出版物引用。
本文章由计算机程序翻译,如有差异,请以英文原文为准。

Letter to the Editor Concerning “Direct Spectroscopic Evidence of Magnetic Proximity Effect in MoS2 Monolayer on Graphene/Co”

Letter to the Editor Concerning “Direct Spectroscopic Evidence of Magnetic Proximity Effect in MoS2 Monolayer on Graphene/Co”
Let us first compare ARPES and spin-resolved photoemission data presented in two figures from Voroshnin et al.: (27) Figure 2a and Figure 3, respectively. As it is well known and clearly stated in ref (27), “The band structure of MoS2 depends on the number of layers: in a few-layer stack, the valence-band maximum is located at the Γ̅ point, while in a single-layer it is at K̅. Figure 2a shows that the valence-band maximum is at the K̅ point, demonstrating that the MoS2 film is one monolayer thick.” This is true for Figure 2a of ref (27), and one can see that the position of the band at the Γ̅ point is by ≈250 meV lower compared to the band position of the upper spin–orbit-split band at the K̅ point. However, if we compare the positions of these bands in Figure 3 of ref (27), then we can see that these bands have the same binding energies, thus contradicting Figure 2a and the statement in the paper. According to Voroshnin et al., (27) the coverage of MoS2 in the synthesized trilayer is about 0.4 mL. Therefore, the apparent “spin-splitting of MoS2 states” may actually be the spin-polarized signal, which comes from the graphene/Co(0001) support underneath MoS2. Particularly, it can happen for the photon energy of 20 eV, which was used for the spin-resolved photoemission experiments. At this photon energy, the photoemission cross section for the Mo 4d and S 3p valence band states is larger compared to the value for Co 3d by a factor of ≈6 and ≈1.5, respectively. However, in the photoemission experiments, this difference is partly compensated by the noncomplete coverage for the MoS2 layer, that leaves some parts of the gr/Co(0001) support naked to the light. In this case, the contribution of the spin-polarized photoemission signal, which originates from the gr/Co(0001) support, to the total photoemission picture is expected to be very significant. The evidence that the background photoemission signal from gr/Co(0001) is spin-polarized is the shift of two curves, spin-up and spin-down, in the vertical direction in Figure 3a, c, and e of ref (27), and the spin-polarized (or spin-split) intensity “bump” is clearly visible at 0.9 eV in Figure 3a ref (27). Moreover, the previous spin-resolved photoemission data for gr/Co(0001) measured at the Γ point clearly demonstrate the strong variation of the spin polarization (in value and in sign) in the range of 2 eV below the Fermi level, (33) i.e., exactly in the energy range where spin-resolved experiments for MoS2 on gr/Co(0001) are presented in ref (27). [The photon energy used in ref (33) is different from the one used in the discussed work. (27) However, taking into account the band structure of gr/Co(0001), a similar strong variation of the spin-polarization is expected.] Unfortunately, such reference spin-resolved photoemissions at a photon energy of 20 eV for the gr/Co(0001) system are not presented in ref (27). Therefore, without such reference data, one cannot unequivocally claim that presented spin-splitting observed for the MoS2-derived states is due to the intrinsic spin-polarization of the MoS2 states. Moreover, using the parameters which can be considered as very close to the real ones used in the discussed experiment, (27) we present a very rough example of how the spin-splitting in the background signal (with spin-splitting of 1 eV) can introduce the “spin-splitting” of 30 meV for the band which is not originally spin-polarized (Figure 1). Here, spin-up and spin-down Lorentzians simulate the photoemission intensity from the respective exchange-split states of the ferromagnetic substrate. If we compare data in Figure 3a of ref (27) and Figure 1 of the present work, we can clearly see that the claimed effect is clearly reproduced, however, without intrinsic spin-polarization for the initially non-spin-polarized emission line. These simulations do not pretend on the completeness and cannot be considered as an attempt to simulate the experimental data presented in ref (27), but they point out the importance of preliminary reference data for gr/Co(0001) (used as a support for the MoS2 growth), which are unfortunately missed in the original work. Here, we also would like to note that in ref (27) the energy resolutions of 10 and 45 meV are claimed for ARPES and spin-resolved ARPES experiments at room temperature, respectively. However, the dominant factor in such experiments is the thermal broadening caused by the sample’s temperature, which amounts to ΔE ≈ 4kBT ≈ 120 meV, (34) which is much large compared to the claimed exchange spin-splitting of 20 meV for the MoS2-derived band at the Γ point and claimed energy resolutions. In Voroshnin et al., (27) the crystallographic structures of the resulting system for which ARPES and spin-resolved photoemission data are presented do not correspond to the crystallographic structures which were used for the interpretation of spin-resolved photoemission data and in the DFT calculations. Moreover, only one model was used in the DFT calculations ignoring other possibilities as discussed below in Results and Discussion. Figure 1. Formation of the “artificial” spin-polarization in the initially non-spin-polarized peak by the spin-polarized photoemission background signal (for details, see the text). The authors of ref (27) use a very thin Co slab of only 4 monolayers (ML). This is an insufficient thickness, in general, which is also very critical when working with magnetic systems. However, even more serious is the lack of passivation of the bottom layer of the slab by adatoms. The approach where the bottom layer of the thin metallic slab is passivated with adatoms, such as H or Al, is a common practice in computation materials modeling. This is especially important for consideration of spin–orbit-related and exchange-splitting effects because of the inversion-symmetry breaking necessary in this case. (35,36) Also such layers protect the magnetic exchange interaction between slabs which can cause artifacts in the calculations. In our work, we have performed the calculations for (4 × 4)MoS2/(5 × 5)graphene/Co(0001) with the distances reported by Voroshnin et al. (27) with and without Al passivation. The results of these calculations allow us to conclude that the claimed ref (27) spin-splitting of the MoS2-derived states at the Γ point is an artifact due to the wrong computational approach (see discussion below and in Methods). We are considering a supercell that has the periodicity that was observed in the experiment, namely, a (9 × 9) lateral periodicity with respect to graphene and Co(0001) and a (7 × 7) lateral periodicity with respect to MoS2 (the resulting structure in our paper is approximately four times larger as compared to the model used in Voroshnin et al.). This way, the lattice mismatch of both two-dimensional materials, graphene and MoS2, is less than 1%. In our work, the slabs have sufficient thickness with the bottom side of each slab protected by a layer of adatoms. Taking into account the synthesis conditions and experimental observations, we take into account the possible intercalation of S and the formation of CoSx. This results in the consideration of six possible structures (instead of one random structure, which does not correspond to the experimental situation, investigated by Voroshnin et al. (27)). We use the same code (see Methods) for the structure optimization and for calculating the band structures. For each structure, all calculated parameters are extracted from the same output file. Furthermore, we present all computational details so that the results can be clearly reproduced by any qualified reader. We disclose all our results: We present the optimized structures (see all Supporting Information) .txt files: S1, S2, S3, S4, S5, and S6), optimized distances (see Results and Discussion), and calculated band structures in the ranges where graphene- and MoS2-valence band states are visible (see Results and Discussion). Figure 2. Optimized crystallographic structures (top and side views) of the MoS2-graphene heterostructures on ferromagnetic Co(0001) considered in this work. The red rhombus marks the unit cell. Figure 3. (a, b) Crystallographic structure of the lattice-matched graphene/Co(0001) interface: top (a) and side (b) views. (c) Spin-resolved band structure of graphene/Co(0001) in the vicinity of the K point. (d) Spin-resolved band structure of free-standing MoS2. All visible spin-splittings are due to the spin–orbit interaction. Total energy (Etot, in eV per unit cell), mean distances between different layers in the optimized structures (for details, see Figure 2: d(gr-S1), d(gr-Co), d(S1–Co), d(Mo-Co), d(gr-Sint), d(S1–Sint), in Å), corrugation of the graphene layer (gr-corr., in Å), average magnetic moments of Mo, S, C, and Co (m(Mo), m(S1), m(S2), m(Sint), m(C1), m(C2), m(Co1), m(Co2), m(Co3), in μB per atom). Figure 4. Spin-resolved band structures of the MoS2-graphene heterostructures on ferromagnetic Co(0001) obtained after the unfolding procedure for the graphene (1 × 1) primitive cell (left) and MoS2 (1 × 1) primitive cell (right). Size of the filled circles gives the number of primitive cell bands crossing particular (k, E) in the unfolding procedure, that is, the partial density of states at (k, E) for graphene (left) and MoS2 (right), respectively. √, experimental observable is reproduced in calculations; x, experimental observable is not reproduced in calculations. Figure 5. Effect of the bottom passivation of the MoS2/gr/Co(0001) slab by Al atoms: (a) no passivation by Al, with exchange splitting of the MoS2-derived states and (b) bottom is passivated by Al, without exchange splitting of the MoS2-derived states. The area of interest is marked by the green rectangle. The Supporting Information is available free of charge at https://pubs.acs.org/doi/10.1021/acsnano.3c09974. S1: Structural data for MoS2/gr/Co(0001) (TXT) S2: Structural data for gr/MoS2/Co(0001) (TXT) S3: Structural data for MoS2/gr/CoSx/Co(0001) (TXT) S4: Structural data for gr/MoS2/CoSx/Co(0001) (TXT) S5: Structural data for MoS2/gr/Sint/Co(0001) (TXT) S6: Structural data for gr/MoS2/Sint/Co(0001) (TXT) Letter to the Editor Concerning “Direct Spectroscopic Evidence of Magnetic Proximity Effect in MoS2 Monolayer on Graphene/Co” 3 views 0 shares 0 downloads Most electronic Supporting Information files are available without a subscription to ACS Web Editions. Such files may be downloaded by article for research use (if there is a public use license linked to the relevant article, that license may permit other uses). Permission may be obtained from ACS for other uses through requests via the RightsLink permission system: http://pubs.acs.org/page/copyright/permissions.html. The authors thank the National Natural Science Foundation of China (Grant No. 22272104) for financial support. E.V. and B.P. gratefully acknowledge the computing time granted by the Resource Allocation Board and provided on the supercomputer Lise and Emmy at NHR@ZIB and NHR@Göttingen as part of the NHR infrastructure. The calculations for this research were conducted with computing resources under the project bec00256. This article references 53 other publications. This article has not yet been cited by other publications.
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来源期刊
ACS Nano
ACS Nano 工程技术-材料科学:综合
CiteScore
26.00
自引率
4.10%
发文量
1627
审稿时长
1.7 months
期刊介绍: ACS Nano, published monthly, serves as an international forum for comprehensive articles on nanoscience and nanotechnology research at the intersections of chemistry, biology, materials science, physics, and engineering. The journal fosters communication among scientists in these communities, facilitating collaboration, new research opportunities, and advancements through discoveries. ACS Nano covers synthesis, assembly, characterization, theory, and simulation of nanostructures, nanobiotechnology, nanofabrication, methods and tools for nanoscience and nanotechnology, and self- and directed-assembly. Alongside original research articles, it offers thorough reviews, perspectives on cutting-edge research, and discussions envisioning the future of nanoscience and nanotechnology.
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