The full exploration of the potential, which graphene offers to nanoelectronics requires its integration into semiconductor technology. So far the real-world applications are limited by the ability to concomitantly achieve large single-crystalline domains on dielectrics and semiconductors and to tailor the interfaces between them. Here we show a new direct bottom-up method for the fabrication of high-quality atomically precise interfaces between 2D materials, like graphene and hexagonal boron nitride (hBN), and classical semiconductor via Ge intercalation. Using angle-resolved photoemission spectroscopy and complementary DFT modelling we observed for the first time that epitaxially grown graphene with the Ge monolayer underneath demonstrates Dirac Fermions unaffected by the substrate as well as an unperturbed electronic band structure of hBN. This approach provides the intrinsic relativistic 2D electron gas towards integration in semiconductor technology. Hence, these new interfaces are a promising path for the integration of graphene and hBN into state-of-the-art semiconductor technology.
In the recent years graphene attracted attention from researchers all over the world and was studied intensively because of its unique electronic properties showing promise for usage in next-generation electronics1. However, for commercial applications, implementation on a large scale into classical semiconductor technology is still missing2. Among other methods to grow graphene, chemical vapour deposition (CVD) on metallic substrates is known to achieve the highest quality of graphene sheets on a large scale3,4. Unfortunately, the electronic properties of epitaxially grown graphene are complicated by charge puddles, charge transfer, corrugation, and hybridization, modifying its unique relativistic two-dimensional (2D) electron gas5,6,7,8, while the post-growth transfer procedure inevitably leads to corrugation, contamination and breakage of graphene sheets9. Thus, many efforts were put to reduce the impact of the substrate on the electronic structure of graphene resulting in intercalation of metals6,7,10,11,12,13,14, semiconductors15,16,17,18, oxygen19,20,21 and hydrogen22,23 under epitaxially grown graphene. It has been shown that graphene can be grown on Ge by molecular beam epitaxy (MBE)24 or chemical vapor deposition (CVD)25 and that graphene on H-terminated Ge4 and on Ge oxide surface26 have superb electronic properties that can even exceed the mobilities of free-standing graphene membranes26. Up to now the best devices were obtained for graphene grown epitaxially on hexagonal boron nitride (hBN)27,28, i.e. achieving a novel van der Waals solid. Clearly, the electronic properties of such devices will be strongly influenced by the interface structure. So far these real-world applications are limited by the ability to concomitantly achieve large single-crystalline domains on dielectrics and semiconductors and to tailor the interfaces between the 2D material and the substrate. Even less is known about how to tailor interfaces between 2D materials, such as graphene and hBN, and classical semiconductors, such as Si and Ge, and especially about scalable growth of high-quality graphene and hBN sheets on semiconductors. Previous works on Ge intercalation were done for graphene on SiC for which the intercalated Ge is amorphous and no precise interface structures was reported19,17. In these works it was reported that Ge intercalation under graphene on SiC leads to ambipolar doping of ±0.3 eV16,17. Here we demonstrate a new bottom-up method for fabrication high-quality large-scale graphene Ge and hBN Ge heterostructures and a crucial pathway how to achieve an atomistic control on these interfaces while avoiding the post-growth transfer process. We experimentally prove the conditions how the Ge intercalation results in atomically precise interfaces between 2D material and atomically thin semiconductor layer and study the stability limits of these planar structures. Using state-of-art electronic structure characterization methods such as angle-resolved photoemission spectroscopy (ARPES) and complementary DFT modelling we observed that graphene with a Ge monolayer underneath demonstrates Dirac Fermions unaffected by the Ni substrate. Comprehensive studies also revealed an unperturbed electronic band structure of hBN after Ge intercalation. These results can have a huge implication for tailoring such interfaces and achieving devices based on relativistic 2D electron gas.
Epitaxially grown graphene and hBN on Ni(111) have a very well-known hexagonal p(1 × 1) low-energy electron diffraction (LEED) pattern7,29,30. Intercalation of Ge leads to a surface reconstruction which can be observed in LEED as a diffraction pattern as shown in Fig. 1(a). The LEED pattern of hBN after Ge intercalation is similar (Supplementary Figure S1). The diffraction spots are very sharp, showing the excellent crystallinity of the interface pointing towards a well-ordered Ge layer. The observed LEED pattern is consistent with a supercell with 6 C and 1 Ge atom per unit cell as shown in Fig. 1(b). This type of LEED pattern is also observed e.g. in LiC6 intercalated graphene31 and graphene/Co(0001), intercalated with silicon32. To explore further the structure and interaction with the substrate in Ge-intercalated graphene and hBN we employ near edge X-ray absorption fine structure (NEXAFS), X-ray photoemission (XPS), angle-resolved photoemission (ARPES) spectroscopies and ab-initio calculations.
NEXAFS spectroscopy allows one to probe unoccupied states and gives information about the hybridisation of electronic states. The angle dependence of NEXAFS K-edge spectra shows the orientation of the π-system with respect to the substrate and thus can be used to characterise the possible corrugation or flatness of the 2D film33,34. In Fig. 1(c–e) we show NEXAFS spectra of the graphene and the hBN K-edges before and after Ge intercalation. The absorption spectrum of graphene on Ni(111) is characterised by the presence of π*- and σ*-resonances and a feature A* between them which is due to strong hybridisation between C2pz and Ni3d orbitals of graphene and Ni substrate35. After Ge intercalation significant changes in the absorption spectra taken at θ = 45° can be observed–the A* peak disappears, π*- and σ*-resonances become sharper and the lineshape of the spectrum becomes similar to quasi-free-standing graphene36. This points towards the decrease of hybridisation and decoupling of graphene from Ni substrate. The abscence of Ge3d states in the close vicinity of the Fermi level, as compared to Ni, leads to the abscence of hybridization between Ge and C, as compared to Ni. Another reason for such behaviour is the abscence of compounds or solubility at the intercalation temperature in Ge-C phase diagram, contrary to Ni-C phase diagram, where there are solid solution region and carbides. CK-edge NEXAFS spectra show a strong angular dependence with highest intensity of π*-resonance at grazing incidence and σ*-resonance at normal incidence, which shows that graphene on Ge is indeed very flat, as expected for quasi-free-standing graphene layer36. As can be seen in Fig. 1(d,e) both B and NK-edges of hBN acquired at θ = 45° change significantly after Ge intercalation. The spectral features A′, A″ and A1 significantly decrease. The main peak A of the π*-resonance becomes very intense, both π*- and σ*-resonances become more sharp and the spectra become similar to quasi-free-standing hBN30. These changes show the decrease of Ni3d–hBNπ hybridisation as a result of Ge intercalation37,38. π*- and σ*-resonances show strong angular dependence with maximum intensity of π* at grazing incidence and minimum at normal incidence, contrary to σ*, pointing towards a flat and decoupled hBN monolayer. Thus we can conclude that Ge intercalation leads to decoupling of graphene and hBN from metallic substrate and formation of quasi-free-standing graphene and hBN monolayers on Ge.
To study the bonding environment and the stoichiometry in Ge-intercalated graphene and hBN we performed XPS measurements. In Fig. 2(a), the evolution of the C1s core level during Ge intercalation is depicted. It can be seen that after the first intercalation step the second component CGe appears in C1s line at lower binding energy. During further Ge intercalation the intensity of initial CNi component decreases while the intensity of CGe increases, pointing towards a liberation of graphene from the substrate. The fully intercalated sample is characterised by a single component CGe in the C1s line which is shifted by −0.41 eV as compared to graphene/Ni. The C1s binding energy of fully Ge-intercalated graphene is equal to that of quasi-free-standing graphene on Au(111)39. The same behaviour can be observed for the B1s and N1s core-level energies of hBN in Fig. 2(b). Here, Ge intercalation also leads to the shift of core-level photoemission peaks to a lower binding energy, indicative of the decoupling of hBN monolayer from the Ni substrate. N1s peak is shifted by −0.75 eV and B1s by −0.3 eV. This behaviour is similar to that of epitaxial hBN for Au intercalation30. According to the interface stoichiometry of GeC6 and GeB3N3, only 0.17 ML of Ge (with respect to graphene or hBN) are needed to form the interface. However, since part of Ge alloys with Ni, a larger amount of Ge is actually needed to form a complete GeC6 interface (according to quartz micro-balance). As we will show below, the Ge XPS spectrum also consists of a surface and a bulk component. Therefore, the ratio of the Ge surface component to the CGe component of the C1s spectrum is a measure of the interface stoichiometry. This stoichiometry, measured by XPS, rapidly approaches GeC6 in fully Ge-intercalated graphene, which is in a perfect agreement with LEED and our structural model. Further increasing the amount of deposited Ge leads to excessive surface coverage. This is observed as a reduction of the C1s photoemission intensity. To show the mechanism of Ge intercalation, we recorded the evolution of the Ge3d core-level spectrum during intercalation. As it can be seen in Fig. 2(c), as-deposited Ge has a broad and weakly resolved doublet corresponding to clusters adsorbed on the graphene surface [Fig. 2(d)]. During heating, the Ge atoms start to intercalate under the graphene (or the hBN) layer and the Ge3d line splits into two doublets – GeB and GeS (bulk and surface, correspondingly), separated by 0.4 eV. This is consistent with recent calculations, showing that a 2D layer of Ge is energetically preferred to small clusters40. Samples annealed to 450 °C represent the maximum intensity of the GeS component and correspond to fully Ge-intercalated graphene and hBN. Further annealing leads to the disappearance of the low-energy GeS component and is accompanied by shifting of the graphene and hBN core-levels back to the initial higher binding energy [see Fig. 2(a,b)].
To study the structure of the interface at fully Ge-intercalated graphene we measured the Ge3d core-level spectrum at different photoelectron emission angles to the sample surface and normalised it to the intensity of graphene’s (hBN’s) core-levels. As it can be seen in Fig. 2(e,f), the intensity of the Ge3d spectrum is lower at grazing emission, showing that after intercalation all Ge atoms are below the graphene or hBN layer. Also the relative intensity of GeB component is reduced with increasing emission angle which indicates that the corresponding Ge atoms are buried deeper under the surface. Thus we can conclude that the GeS doublet corresponds to intercalated Ge atoms in between graphene (hBN) and the Ni substrate and the GeB doublet correspond to Ni2Ge alloy, where Ge atoms are incorporated in topmost Ni layer. This conclusion is also supported by our simulations, the difference in Ge3d binding energy for intercalated and alloyed Ge atoms is 0.4 eV, which is in a perfect agreement with XPS data (see supplementary details for further information). The relative intensity of GeS component for different emission angles can be fitted with a Beer-Lambert law [see inset of Fig. 2(f)]. From this analysis we estimated the thickness of intercalated and alloyed Ge layers as 4.1 Å and 2.9 Å, correspondingly (A detailed description of the analysis procedure is given in Supplementary Note 1). The remarkably narrow spin-orbit split components in the Ge3d line show that Ge atoms after intercalation form a well defined structure, like it was observed for germanene41 and Ag2Ge surface alloy42. Interestingly, these samples are the first where the Ge doublet can be clearly observed, while previous attempts of Ge intercalation under graphene yielded only one Ge line and lacked a LEED pattern16,17. This information allows us to assume that Ge intercalation leads to formation of a well-ordered Ge layer in between graphene (hBN) [Fig. 2(d)] and the Ni(111) substrate at 450 °C and some amount of Ge atoms alloyed with Ni. Further annealing leads to alloying of all Ge intercalated with the Ni substrate and brings graphene (hBN) to the initial state with a higher binding energy [Fig. 2(a,b)]. Such transitions from the adsorbed state to a surface alloy have been observed before in Sn/Ni(111) system and resulted in the formation of an ordered surface alloy with the same structure43,44,45.
To study the impact of Ge intercalation on the electronic band structure of graphene and hBN we performed ARPES measurements which directly probe the electron energy dispersion in solids. In Fig. 3(a,b) we show ARPES spectra in the vicinity of the K point of the graphene Brillouin zone before and after Ge intercalation. Figure 3(a) shows the well-known band structure of graphene on Ni(111). It can be characterised by a large shift of the graphene π band due to the strong hybridisation with Ni3d states, which brings the Dirac point to almost 3 eV binding energy. Ni3d states can be clearly observed at the Fermi level. Intercalation of Ge leads to drastic changes in the band dispersion of graphene. As we can see in Fig. 3(b), Ge intercalation restores the Dirac cone, shifting the Dirac point to the Fermi level, the intensity of Ni3d states decreases and the band structure of graphene becomes similar to that of quasi-free-standing graphene6. In Fig. 3(c) we show the high-resolution ARPES data measured at 20 K together with the momentum distribution curve (MDC) fit with two Lorentzian peak functions. It should be noted that because of matrix element effects in the photoemission cross section, the π* graphene states are invisible with p polarization in the first Brillouin zone. Hence, we performed our photoemission studies in both, p and s polarization and then added them39,46. As it can be seen graphene on Ge is indeed quasi-free-standing – the Dirac point is at the Fermi level. This behaviour is different when compared to graphene on SiC intercalated with Ge16,17 and is attributed to the facts that (i) in the present case Ge is ordered and (ii) the substrate is different (Ni instead of SiC).
These experimental data are in good agreement with ab-initio calculations performed for Ge-intercalated graphene on Ni(111). We started from the optimised top − fcc geometry, which is known to be the most stable for graphene/Ni(111) theoretically47 and observed experimentally5. Then Ge was added in the right stoichiometry in between graphene and the topmost Ni layer in correspondence of the hollow site of graphene (lowest energy) and the structure was optimised. Atomic relaxation induced by the presence of Ge breaks the bonds between the surface Ni and C atoms. This produces a detaching of graphene from Ni(111) surface bringing it to about 3.8 Å, without any corrugation. The final geometry is characterised by a surface reconstruction of Ni which move away from the Ge adatom eventually sitting in correspondence of the middle of the C–C bond [Fig. 3(e,f)]. In the band structure linear Dirac bands belonging to the graphene lattice are restored and a Dirac point is present at about 0.3 eV from the Fermi level [Fig. 3(d)]. We summarised in Table 1 the calculated structural properties of the considered systems in terms of distances from substrate to graphene, corrugations and presence of the Dirac bands.
Figure 3(g,h) show the band dispersion of pristine hBN/Ni(111) and fully Ge-intercalated hBN. First, the intensity of Ni3d states at the Fermi level decreases significantly upon Ge intercalation. Second, the intercalation of Ge atoms leads to the shift of π-and σ-bands by 1.29 eV towards the Fermi level, bringing the π band at the K point to a binding energy of 2.9 eV. Such changes in the band structure point towards decoupling from Ni substrate and the formation of quasi-free-standing hBN monolayer30. We now discuss the effects of further annealing of Ge intercalated graphene and hBN on the electronic band structure. As it was mentioned in the discussion of the XPS data, further annealing of Ge intercalated graphene and hBN leads to alloying of all Ge atoms with the Ni substrate and diffusion of Ge into the bulk Ni. Figure 3(i,j) show the band dispersion of hBN/Ge in the vicinity of K point after annealing at elevated temperature (∼600 °C). It can be seen that such treatment leads to the appearance of a second band π2, whose intensity increases with the annealing time. Also the intensity of Ni3d states increases. This restores the initial electronic band structure of graphene and hBN with a higher binding energy.
Now we discuss a theoretical suggestion of an alternative structural model and provide reasons, based on our measurements, to exclude it. We performed ab-initio calculations for a structure with the same amount of Ge atoms (1 per unit cell) substituting Ni atoms in topmost layer, yielding the Ni2Ge alloy [Fig. 4(a,b)]. Incorporating of Ge in the topmost Ni layer produces a slight increase of the graphene–substrate distance up to 2.2 Å, as compared to graphene/Ni(111) (see Table 1), but the hybridisation between the Ni3d states and Cpz is still relevant and the Dirac cone is not restored [Fig. 4(c)]. Also graphene on the Ni2Ge layer shows a slight corrugation of 0.15 Å. This perfectly correlates with our experimental results and show that intercalation of Ge atoms leads to the formation of quasi-free-standing graphene and hBN, while formation of surface alloy with the same symmetry and stoichiometry does not lead to the decoupling of graphene (hBN) from the Ni substrate.
The calculated formation energy of graphene/Ni2Ge/Ni(111) is 1.4 eV lower than that of graphene/Ge/Ni(111) structure, which means that the formation of an alloy is more favorable and the driving force of Ge intercalation is the reduction of the total energy if Ge alloys with Ni. This explains the fact that at elevated temperatures the intercalated Ge layer overcomes the diffusion barrier and incorporates into the topmost Ni layer resulting in a Ni2Ge alloy.
In this work we carried out a bottom-up approach to synthesize atomically precise graphene–Ge and hBN–Ge interfaces with GeC6 and GeB3N3 stoichiometry. Starting from epitaxial graphene/Ni(111) and hBN/Ni(111) we performed Ge intercalation which resulted in well-defined interfaces between the 2D layer and Ge. The reconstruction was observed for both graphene–Ge and hBN–Ge systems after intercalation. Using XPS and LEED we have characterized the structure, stoichiometry and stability of these interfaces. Further NEXAFS and ARPES measurements and ab-initio calculations corroborated this structural assignment and showed that intercalation of Ge restores the graphene and hBN band structure making them quasi-free-standing. It was shown that intercalation leads to formation of atomically thin Ge layer, while further annealing leads to alloying of Ge with Ni and does not result in quasi-free-standing graphene or hBN. We have also shown that further annealing causes the reversal of the band structure changes since Ge diffuses inside the bulk Ni. Given the current interest in Ge nanostructures such as germanene and the promising transport properties of graphene on Ge, we believe that a well-defined interface with its electronic properties fully characterized can pave the way for future progress in this research direction.
Graphene/Ni(111) and hBN/Ni(111) samples were prepared in situ under ultra-high vacuum (UHV) conditions by chemical vapour deposition on Ni(111) single crystalline film from propylene (C3H6)29 and borazine (B3H6N3)30, respectively. Then Ge (99.9999 + at.%, MaTecK) was evaporated from a Ta crucible and intercalation was achieved by further annealing to 450 °C according to pyrometer. The total amount deposited was controlled by quartz microbalance and XPS (the scheme of the experimental setup is shown in the Supplementary Figure S2). The quality of the samples was controlled for each step by LEED. The XPS and NEXAFS measurements were carried out at HESGM34 and the German-Russian (RGBL)48 beamlines at the Helmholtz-Zentrum Berlin (Germany). XPS spectra were acquired at various emission angles with respect to the sample surface. C1s and Ge3d core-level spectra were acquired with hv = 330 eV excitation energy, N1s and B1s core-level spectra were measured with hv = 450 eV excitation energy. NEXAFS spectra were acquired in total electron yield (TEY) and partial electron yield (PEY) modes at different incidence angles θ and then normalised to the intensity of incident radiation. ARPES scans through the K point perpendicular to the ΓKM high-symmetry direction were acquired at UE112_PGM-1 beamline with the RGBL-2 station at Helmholtz-Zentrum Berlin (Germany). Spectra were acquired at a photon energy of 40 eV with the sample held at room temperature and a base pressure better than 5 × 10−11 mbar. High-resolution ARPES scans through the K point along the ΓKM high-symmetry direction were acquired at BaDElPh beamline49 at Elettra synchrotron in Trieste (Italy). ARPES spectra were acquired at a photon energy of 29 eV with the sample held at 20 K and a base pressure better than 5 × 10−11 mbar. The total angular and energy resolution was determined to 0.15° and 15 meV, respectively. ARPES measurements of hBN were performed using a photoelectron spectrometer equipped with a Scienta SES-200 hemispherical electron energy analyzer and a high flux He resonance lamp (Gammadata VUV-5010) in combination with a grating monochromator. Spectra were acquired at room temperature and a photon energy of 40.8 eV (He IIα), with an angular resolution of 0.2° and a total energy resolution of 50 meV. Electron band dispersions were measured along the ΓKM direction of the Brillouin zone by varying the polar-emission angle.
The calculations were performed using the Vienna Ab-Initio Simulation Package (VASP)50,51 within the local density approximation (LDA)52. We used projected augmented-wave (PAW) pseudopotentials for all the atomic species involved with an energy cutoff up to 500 eV. Integration over the Brillouin Zone was performed considering an uniform 6 × 6 × 1 Monkhorst and Pack grid. The surfaces were simulated in the supercell approach with a vacuum space of 26 Å. Core-level shifts were calculated within the initial state approximation calculating the Kohn-Sham eigenvalues of the core states.
The formation energies (Ef) were calculated as:
where EX is the Kohn-Sham total energy of the X system. The chemical potentials of Ge and Ni (μGe and μNi, respectively) where considered equal to the total energy/atom of their stable bulk phases.
How to cite this article: Verbitskiy, N. I. et al. Atomically precise semiconductor—graphene and hBN interfaces by Ge intercalation. Sci. Rep. 5, 17700; doi: 10.1038/srep17700 (2015).
A.G. acknowledges the ERC Consolidator grant ‘SUPER-2D’ (grant agreement 648589) and funding from QM2 (Quantum Matter and Materials). N.I.V. and T.P. acknowledge Austrian Science Fund (FWF): projects No. I 377-N16 “Theory and Spectroscopy on functionalized Graphene” and No. P27769-N20 “Electron and Spin Correlation in Nano Carbon-Metal Hybrids”. A.G. and N.I.V. acknowledge funding from the 2EU MCA-IRSES project 612577 NanoCF. N.I.V. and A.A.E. acknowledge the Russian Science Foundation (No. 14-13-00747). G.P. acknowledges the FP7 European project SUPER-IRON (grant agreement No. 283204) and the Italian Ministry of University Research through the PRIN 2012 project. Computational resources were provided by CINECA award under the ISCRA initiative. D.Yu.U., A.V.F. and B.S. acknowledge RFBR (grant No. 14-02-31150). D.Yu.U., A.V.F. and D.V.V. acknowledge Saint Petersburg State University (grants No. 11.37.634.2013 and No. 18.104.22.1685). This work was partially supported by KIT Research Program Science and Technology of Nanosystems. The research leading to these results has received funding from the European Community’s Seventh Framework Programme (FP7/2007–2013) under grant agreement CALIPSO (n.312284). We thank HZB and Elettra for the allocation of synchrotron radiation beamtimes.
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