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. Author manuscript; available in PMC: 2018 Aug 8.
Published in final edited form as: Chem Mater. 2017 Jul 12;29(15):6279–6288. doi: 10.1021/acs.chemmater.7b01367

Rapid Wafer-Scale Growth of Polycrystalline 2H-MoS2 by Pulsed Metalorganic Chemical Vapor Deposition

Berc Kalanyan †,*, William A Kimes , Ryan Beams , Stephan J Stranick , Elias Garratt , Irina Kalish , Albert V Davydov , Ravindra K Kanjolia , James E Maslar
PMCID: PMC5846631  NIHMSID: NIHMS943719  PMID: 29545674

Abstract

High volume manufacturing of devices based on transition metal dichalcogenide (TMD) ultra-thin films will require deposition techniques that are capable of reproducible wafer-scale growth with monolayer control. To date, TMD growth efforts have largely relied upon sublimation and transport of solid precursors with minimal control over vapor phase flux and gas-phase chemistry, which are critical for scaling up laboratory processes to manufacturing settings. To address these issues, we report a new pulsed metalorganic chemical vapor deposition (MOCVD) route for MoS2 film growth in a research-grade single-wafer reactor. Using bis(tert-butylimido)-bis(dimethylamido)molybdenum and diethyl disulfide we deposit MoS2 films from ≈ 1 nm to ≈ 25 nm in thickness on SiO2/Si substrates. We show that layered 2H-MoS2 can be produced at comparatively low reaction temperatures of 591 °C at short deposition times, approximately 90 s for few-layer films. In addition to the growth studies performed on SiO2/Si, films with wafer-level uniformity are demonstrated on 50 mm quartz wafers. Process chemistry and impurity incorporation from precursors are also discussed. This low-temperature and fast process highlights the opportunities presented by metalorganic reagents in the controlled synthesis of TMDs.

Keywords: MoS2, MOCVD, CVD, transition metal dichalcogenides, metalorganic chemistry

1. INTRODUCTION

Layered two-dimensional (2D) transition-metal dichalcogenides (TMDs), e.g., MoS2, WSe2, ReS2, are of increasing interest for next-generation nanoelectronic and optoelectronic devices due to their unique thickness modulated electronic properties1. When structured into single or few atomic layers, some TMDs develop a direct band gap due to quantum confinement2, which enables their use in low-power field effect transistor (FET) devices35. In addition to traditional logic devices, structures consisting of TMDs are also being investigated for use in valleytronics6, memory applications7, chemical sensing8,9, optoelectonics1012, energy devices13, and life sciences14,15. When assembled into van der Waals heterostructures with TMDs or other 2D materials (e.g., graphene, hexagonal BN, etc.) novel and unique device arrangements16,17 become realizable without the need for epitaxial matching between the layers. Furthermore, incorporation of dopants into TMDs1821, alloying of various layered compounds22, and heterojunction assemblies2325 highlight the immense level of tunability afforded by layered 2D systems. Despite their tremendous potential for new applications, synthetic routes available for 2D TMDs have been largely limited to growth techniques that are difficult to scale, have low throughput, or do not offer sufficient control over the process chemistry to achieve reproducible material properties. Additionally, commonly employed powder vaporization routes, e.g., MoS2 from MoO3 and S, require high growth temperatures and are not suitable for downstream integration with existing electronic manufacturing process flows.

Synthetic high-quality bulk TMD crystals are commonly produced using the chemical vapor transport method26. After growth, individual layers held together by van der Waals forces can be separated from the bulk by mechanical exfoliation and transferred onto device substrates. Although this approach is successful for small scale device development and fundamental studies, large-area growth of TMDs requires vapor-phase deposition routes. The simplest approach that employs vapor-phase reagents is direct chalcogenization of metal foils27,28 or thin films29. These approaches pose several challenges, particularly in terms of compatibility with semiconductor process flows and 3D integration. For instance, growth on sacrificial substrates requires the mechanical transfer of TMDs onto a target substrate and metal chalcogenization requires a separate metal deposition step. Among other growth techniques, powder vaporization in flow tube reactors using inorganic sources such as transition metal oxides and elemental chalcogens have been widely used to produce a variety of 2D TMDs3034. While high-quality films are routinely produced in this manner, the inherent lack of control over precursor flux and process variability associated with the flow tube geometry severely limit the scalability of powder vaporization. Even with high vapor pressure precursors, hot-walled flow tube reactors present problems with parasitic wall reactions, i.e., partial conversion of precursors before they reach the substrate.

To overcome scalability and process control issues, recent reports on TMD synthesis have focused on using alternative metal precursors, primarily transition metal halides35 such as MoCl5 or metal carbonyls36 such as Mo(CO)6. Halides have also been used in low-temperature processes, with several examples of atomic layer deposition (ALD)37,38 reported to date. At low growth temperatures, ALD TMD routes do not produce crystalline material and corrosive reaction products are generally undesirable. Recently, a new CVD route was proposed by Robinson et al.39 using W(CO)6, (CH3)2Se, and H2, to produce large-grain WSe2. Using an analogous chemistry, Kang et al.36 found that layer-by-layer or 2D growth of MoS2 occurred in a tube reactor under sufficiently low Mo(CO)6 flux, which necessitated extremely long growth times of 26 hours per monolayer MoS2. Metal carbonyls are typically used for low-temperature metal CVD reactions due to their zerovalent state40. However, high reaction temperatures (typically 800 °C to 900 °C) needed to produce large grain TMDs pose unique challenges for transition metal carbonyl sources. Iron and nickel carbonyls are known to form41 readily upon reaction of CO and H2 with exposed stainless steel surfaces (e.g., reactor walls). These conditions are met in CVD reactions that liberate CO from metal carbonyls and often employ H2 as a reducing agent. In situ formation of Fe and Ni carbonyls could become a source of downstream Fe and Ni contamination for metal carbonyl based chemical vapor deposition (CVD) routes. In contrast to the inorganic42 metal sources in use today, metalorganic precursors are expected to offer greater flexibility and a higher degree of controllability for processing in conventional CVD reactor hardware.

In this article we report a new MOCVD process that addresses some of the challenges encountered in the state of the art vapor-phase TMD growth. Here, we present a new MOCVD process that uses metalorganic and organosulfur precursors and produces wafer-scale 2H-MoS2 films at short deposition times from tens of seconds to several minutes. We use a pulsed injection strategy to discretize the growth process, which, to our knowledge, is the first reported pulsed MOCVD process for 2D TMD growth. The relatively low growth temperature of 591 °C employed in this work makes our process thermally compatible with a variety of substrates, including flexible glasses used in consumer electronics43. Through extensive post-deposition characterization, we relate film properties to process conditions. We show that few-layer MoS2 can be readily produced on 50 mm diameter substrates, with sub-monolayer control over aggregate film thickness. Chemical analyses show impurity incorporation and ligand removal steps, which suggests that precursor chemistry impacts the film deposition process and that exploration of additional metalorganic precursors may provide new vapor-phase synthetic routes for TMD growth.

2. EXPERIMENTAL METHODS

a. Surface preparation

Surfaces used for growth characterization consisted of 90 nm thermal SiO2 on Si(100). For each growth run, 32 mm × 32 mm coupons were cleaved from a 300 mm wafer and degreased using acetone and methanol, and subsequently dried using a stream of nitrogen. X-ray photoelectron spectra from as-cleaned substrates showed only Si, O, and C species, the latter being ascribed to adventitious carbon.

b. MOCVD growth

Films were grown in a single-wafer perpendicular flow reactor described elsewhere44. Briefly, the reactor consisted of a resistively heated thin-walled stainless steel pedestal, independently heated aluminum walls, and o-ring sealed flanges. Gas flow direction was normal to the plane of the receiving substrate. Walls were maintained at 160 °C and upstream lines were heated to prevent precursor condensation. Substrates were placed on the steel pedestal and heated to a surface temperature of approximately 591 °C ± 1 °C, measured using a type-K thin-wire thermocouple embedded on a test wafer. Substrates were allowed to thermally equilibrate for 10 minutes once the heater setpoint was reached. Reactions were run at 160 Pa using 400 mL/min (standard cubic centimeters per minute, SCCM) of argon (99.999 %) at standard temperature and pressure (STP) with the carrier gas distributed among four delivery lines. Here, STP is defined as 0 °C and 101.33 kPa. The reactor was pumped using a twin-screw pump with an ultimate pressure of approximately 0.01 Pa. The metal precursor was electronic grade bis(tert-butylimido)-bis(dimethylamido)molybdenum, (NtBu)2(NMe2)2Mo, installed in a 300 mL stainless steel ampoule, heated to 28 °C in an oven, and delivered by flowing 25 SCCM of carrier gas over the ampoule head space (vapor draw). Electronic grade diethyl disulfide (Et2S2, >98 %) was used as the sulfur source and was delivered out of a 100 mL single-port ampoule heated to 60 °C. Carrier flow rate in the Et2S2 line was 100 SCCM, with two auxiliary lines delivering the balance. In order to limit the amount of Et2S2 delivered, a 250 μm diameter steel orifice was installed between the ampoule and the injection valve. After deposition, the wafer heater was allowed to cool to ≈160 °C, at which point the reactor was back filled with Ar and the wafer immediately removed and placed on a cold surface. As a result of this procedure, all deposited films were briefly exposed to laboratory ambient at ≈160 °C upon removal from the reactor.

Each reaction cycle consisted of 1.5 s long co-injections of (NtBu)2(NMe2)2Mo centered on 2.0 s long injections of Et2S2. Pulse duration for the Et2S2 was kept slightly longer than the Mo source in order to preclude reactions of (NtBu)2(NMe2)2Mo in the absence of sulfur. After each co-injection of Mo and S reagents, the reactor was purged with 400 SCCM of Ar for 4.0 s, resulting in a 6.0 s cycle time. A graphical representation of the reaction chamber and the pulse valve timing scheme are shown in Figure 1. High precision pulse timing and repeatability was incorporated into the injection system using low-jitter digital delay generators. In this fashion, reaction cycles were iterated n number of times to vary the thicknesses of MoS2 deposited. For example, we will write n=15 to mean 15 injections of ((NtBu)2(NMe2)2Mo+ Et2S2). By employing pulsed injections, we effectively regulated the amount of material delivered to the growth surface and arbitrarily discretized the time coordinate of the growth process.

Figure 1.

Figure 1

Overview of the pulsed MOCVD process. A schematic of the reactor geometry is shown on the right and the injection sequence of the Mo and S precursors in a 6 s period is shown on the left.

c. Characterization

Raman and photoluminescence (PL) spectra were obtained with 532 nm excitation in a back-scattering configuration using a custom-built Raman microprobe system. The incident laser was spatially filtered and sent into the microscope after passing through a linear polarizer to define the excitation polarization. Radiation was introduced into the microscope optical path using an angled dielectric edge filter in an injection-rejection configuration. A 40×, 0.75 numerical aperture infinity-corrected microscope objective was used for focusing incident radiation and collecting scattered/emitted radiation. Power levels at the sample were less than about 1 mW and 0.1 mW for Raman and photoluminescence spectroscopy, respectively. Collected scattered/emitted radiation was coupled to a multimode optical fiber and delivered to a 0.5 m focal length and 0.3 m focal length imaging, single spectrograph for Raman and photoluminescence spectroscopy, respectively. Light was detected with a back-illuminated, charge coupled device (CCD) camera system operating at −70 °C and −75 °C for the Raman and PL CCD cameras, respectively. The instrumental bandpass full width at half maximum (FWHM) was approximately 2.2 cm−1 at 347 cm−1 and 18.3 cm−1 at 1700cm−1 for Raman and photoluminescence spectroscopy, respectively. Laser wavelength was determined using a commercial wavemeter.

Cross sectioning for high resolution transmission electron microscopy (HRTEM) was performed using an FEI Nova Nanolab instrument (FEI Company, Hillsboro, OR). To protect sample integrity, thin layers of C (10 nm) and Pt (250 nm) were deposited using an electron beam operating at 5 keV. The final Pt cap was deposited using the ion beam operating at 30 keV. Samples were extracted and thinned using standard lift-out techniques. HRTEM was performed using an FEI Titan 80-300 AEM (FEI Company, Hillsboro, OR). Images were obtained with a multi-scan CCD camera with a single 1024×1024 pixel detector using 300 keV electrons through a 60 μm aperture at 1 nA of current for 1 s acquisition times. Sample thickness was nominally 100 nm or less for all images obtained. Fourier transformations were calculated using Gatan DigitalMicrograph (v3.10) (Gatan Inc., Pleasanton, CA).

X-ray photoelectron spectroscopy (XPS) was carried out using a Kratos Axis Ultra DLD instrument from Kratos Analytical (Chestnut Ridge, NY), which incorporated a monochromated Al Kα source operated at 104 W (8 mA; 13 kV) and a hemispherical analyzer. Spectra were acquired at an analyzer pass energy of 40 eV and the analysis area was approximately 1 mm by 0.5 mm. Spectra were charge calibrated against S 2p3/2 (S-Mo, 162.0 eV) assigned to MoS245. A low energy electron gun was used for charge neutralization. Elemental percentages were calculated by taking the average of at least three non-overlapping measurements, with the uncertainty given as ± one standard deviation of the mean. Film thickness was estimated based on the inelastic scattering of Si 2p photoelectrons by an MoS2 overlayer. The inelastic mean free path (IMFP) for Si 2p at a kinetic energy of 1383 eV was estimated to be 2.537 nm using the TPP-2M formula as implemented in the NIST Electron Inelastic-Mean-Free-Path Database46. Parameters used for the IMFP calculation were ρMoS2=5.06gcm3 (for bulk molybdenite47), Eg,MoS2=1.8eV (monolayer2), and 18 valence electrons, where ρ is the mass density and Eg is the band gap. Peak fitting was done using the CasaXPS software package (v2.3.17) (Teignmouth, U.K.). Sputter depth profiling was done using 4 keV Ar+ ions delivered to the surface at a 70° angle of incidence. The ion beam was rastered over an area of 3 mm × 3 mm at a current density of approximately 0.5 mA/cm2. The analysis area was within the plateau of the sputter crater.

X-ray diffraction (XRD) data were collected using a conventional powder diffractometer by Phillips in the θ–2θ configuration using CuKα radiation (λ=0.15418 nm). The XRD scans were analyzed using the MDI-JADE 6.5 software package (Jade 6.5, Materials Data, Inc. Livermore, CA., 2015). MoS2 c-lattice parameter was calculated by cell refinement. Complimentary two-dimensional X-ray diffraction (XRD2) patterns were collected on a Bruker-AXS D8 Discover diffractometer (Bruker Corporation, Billerica, MA), equipped with an area detector (Hi-star), using CuKα radiation. Intensity of the 0002 reflection from the XRD2 pattern was angle-integrated along the χ direction, which is equivalent to sample tilting in a conventional diffractometer, to produce a “rocking curve”-like plot (see inset in Figure 6) to assess the degree of texture in the film. The angle integrated patterns were examined using Bruker AXS Diffracplus EVA software.

Figure 6.

Figure 6

θ-2θ XRD scans from a thick MoS2 films (≈25 nm, n=200) grown at 591 °C. Absence of the hkl reflections other than from the {0002} family is evidence for 0002 texture in the film. A high degree of texture is also evident from a relatively narrow rocking curve shown in the inset, which shows an integrated intensity for the 0002 reflection vs χ-angle produced from the XRD2 diffraction (not shown). Reflections identified with a star (★) on the θ-2θ scan are from the Si (100) substrate. The lattice parameter is calculated as c = 1.2306(5) nm.

Atomic force microscope (AFM) topographic images were collected using an Asylum Research MFP-3D instrument (Asylym Research, Goleta, CA). The measurements were done in tapping mode using a stiff cantilever (Si, 42 N/m) with a large driving aplitude and setpoint. Surface roughness values are calculated as the root mean square (RMS) of the height data.

Scanning electron microcopy (SEM) characterization was done using Hitachi S-4700 (Hitachi High-Technologies Europe GmbH, Krefeld, Germany) and JEOL JSM-7100 (JEOL Ltd., Tokyo, Japan) field emission instruments operated at 20 kV accelerating voltage with the sample stage tilted to 70° in order to assess the film’s morphology.

3. RESULTS AND DISCUSSION

Films were grown on wafer substrates using pulsed injections of (NtBu)2(NMe2)2Mo and Et2S2 as described in the Experimental section. We varied the number of pulses to scale the thickness of the MoS2 films deposited. The flow distribution in this reactor geometry has been previously modeled44 using computational fluid dynamics and results in visually uniform coatings on large-area substrates. To demonstrate uniform and large-area deposition of MoS2, we grew films of various thicknesses on 50 mm diameter fused quartz wafers. Photographs of wafers with n=0, 15, 50, and 100 injections of (NtBu)2(NMe2)2Mo and Et2S2 are shown in Figure 1 (b). The coatings are uniform to the eye over the diameter of the wafers and show decreasing optical transmission with increasing film thickness.

Few-layer MoS2 films were grown and subsequently characterized using cross-sectional HRTEM, Raman spectroscopy, PL spectroscopy, XRD, and XPS. We found that growth on thermal SiO2 exhibited gross inhomogeneities at n<10, associated with nucleation or incomplete surface coverage. In order to characterize the properties of coalesced and continuous films, we focused our attention on films growth with 25 pulses. Cross-sectional HRTEM images from a film deposited using n=25 are shown in Figure 3 (a) through (c). In Figure 3 (a), MoS2 can be identified by the dark contrast between the SiO2 layer and the protective carbon coating. The film is continuous within the field of view, with some areas showing non-uniformities in thickness. Regions of the film that appear to be out of focus may be a result of sample preparation. These regions could be the topmost MoS2 sheet that has come loose during cross sectioning and is projecting away from the plane of the image. The higher magnification image in Figure 3 (b) is from the dashed area in Figure 3 (a). Here, a layered structure is clearly discernable, with some layers exhibiting non-planar stacking. A higher magnification view in Figure 3 (c) shows approximately 6 layers present with a total thickness of 4.08 nm ± 0.20 nm, taken as the average of ten line measurements in Figure 3 (b). Interplane spacing was measured to be 0.68 nm ± 0.05 nm, in agreement with the expected separation between stacked MoS2 layers48.

Figure 3.

Figure 3

HRTEM cross sections from MOCVD grown MoS2 on SiO2/Si shown at (a) low, (b) medium, and (c) high magnification.

The orientation of the first few MoS2 layers with respect to the amorphous substrate may give some insights into the initial nucleation mechanism. Several layers in Figure 3 (b) emerge from the substrate and terminate back at the substrate a short distance away, ca. 10 nm. Second, third, and subsequent MoS2 planes show significantly longer continuity, with some layers extending beyond 50 nm without interruption. Also in Figure 3 (b), some regions of the image show branching and merging MoS2 planes. One growth model that would account for these observations is island nucleation. In this model, the anchor points at which the MoS2 originates out of the substrate could be the initial nucleation sites. Surface-limited reaction of (NtBu)2(NMe2)2Mo with hydroxyl groups was reported for ALD of MoO349 and MoN50,51 at <325 °C. Assuming a similar interaction with surface hydroxyls, the initial formation of Si-O-Mo bonds may also play a role in MoS2 nucleation. Accordingly, the formation of the first MoS2 layer may be influenced by the substrate chemistry, whereas subsequent layers could form based on interactions with existing MoS2 surfaces. Differences in layer continuity between the first and subsequent MoS2 layers gives some validity to this distinction. Since the reaction temperatures in this study are low (<600 °C) relative to furnace grown TMDs, the Mo adatoms are expected to have limited surface mobility and, therefore, rearrangements at the MoS2/SiO2 interface are less likely. Under such conditions, grain size could be dependent on the initial nucleation process. The interface shown in Figure 3 (b) and (c) is remarkably similar to that produced by pulsed laser deposition (PLD)52 at 700 °C, showing that surface rearrangement may not be favorable even at higher substrate temperatures for fast deposition processes. While we focused this work on wafer-scale growth and pulse modulated thickness control, deposition at a higher reaction temperature and on crystalline substrates is expected to promote better long range ordering of MoS2 basal planes. Further discussion of growth temperature is provided in the Supporting Information (Figure S1).

In addition to comparatively low deposition temperatures afforded by this MOCVD chemistry, controlled and reproducible growth of TMDs is also highly desirable. By employing pulsed injections of precursor, we can impose digital control over film thickness, which is otherwise difficult to achieve with a continuous deposition process. Although a continuous process could have been used, we implemented pulsed injections to mitigate transient effects associated with the depletion of precursor vapor in a vapor draw configuration, as employed in this work. To illustrate thickness scaling that is achievable by our pulsed MOCVD scheme, we systematically varied the number of (NtBu)2(NMe2)2Mo and Et2S2 injections at a wafer temperature of 591 °C and studied the resultant films by XPS. By measuring the attenuation of the Si 2p photoelectrons originating in the SiO2 layer, we were able to estimate the average thickness of the MoS2 overlayer over the sampled area (see Supplemental Information for details). Given the large analysis area of XPS (≈ 0.5 mm2) compared to the MoS2 crystallite size, film thicknesses calculated from XPS are representative of the amount of material on the surface without accounting for the growth mode. Figure 4 (a) shows the results of this analysis. We found that film thickness increases linearly with n and the MOCVD process gives rise to Mo 3d signal after a single injection of the reactants (Figure S2). Since the reactivity of (NtBu)2(NMe2)2Mo with hydroxylated surfaces is known, the lack of a chemisorption delay is not surprising. Interestingly, the thickness intercept in Figure 4 (a) is non-zero, which could indicate the presence of an interfacial layer that develops during nucleation or a surface contamination layer that exists prior to deposition. These would be reasonable possibilities since the substrates do not undergo in situ cleaning before growth. While the origin of this offset is not clear, the linear trend in Figure 4 (a) demonstrates the level of thickness control afforded by the pulsed injection strategy. The aggregate growth rate is determined to be 0.12 nm/pulse, which is equivalent to < 1 ML of MoS2 deposited per injection, when considered on a planar basis. Given that 2H-MoS2 is a layered crystal with a fixed d spacing, an aggregate growth rate less than d suggests that surface coverage is less than unity per pulse. The aggregate thickness control achieved using our MOCVD approach demonstrates that a pulsed-metering of the precursor delivered to the substrate can provide fine control over film thickness for a fast TMD deposition process. For further analysis of the way in which growth proceeds we turn to AFM.

Figure 4.

Figure 4

In (a), film thickness estimated from Si 2p photoelectron attenuation is plotted as a function of pulse count. Error bars represent one standard deviation of the mean. (b) Shows root mean square surface roughness as determined by AFM. Inset panels in (b) show perspective view (70° tilt) SEM images for 25 and 50 pulses.

Figure 4 (b) shows the evolution of surface roughness for the same range of thicknesses analyzed by XPS. For n≤15, film roughness remains below 2 nm. Within this regime, films are relatively smooth and exhibit a uniform distribution of small features <20 nm in lateral dimensions, as shown in Figure S3. At n=25, roughness increases to 2.4 nm, and continues to rise, reaching 6 nm at n=50. Despite the large roughness factor, all MoS2 on the surface is accounted for by XPS since Si 2p photoelectrons have a finite escape probability through an MoS2 layer up to ≈8 nm thick. Contrasting the linear growth rate measured by XPS to the onset of surface roughening at n=25, we postulate that 3D or out-of-plane MoS2 growth takes place beyond ≈4 nm of growth. Indeed, we find that beyond 50 pulses, films continue to roughen. Accompanying SEM images show that the rough areas evident at n=25 take the form of randomly oriented features by n=50, and eventually grow into sharp platelets emerging from the surface at n=100 (Figure S4). Additional deposition (n=200) produces a continuous surface with rounded features. One potential explanation for this evolution in film morphology is a growth process with a distinct nucleation phase. At n≤15 the growth could be dominated by precursor-substrate interactions, as the initial few ML of MoS2 are formed. Subsequent deposition of MoS2 on existing MoS2 sites includes a 3D growth component, where out-of-plane crystallites can form alongside the layered structure confirmed by TEM and diffraction measurements (discussed below).

The complex evolution of MoS2 layering, surface coverage, and morphology is a confounding factor for spectroscopic measurements. For this reason we will limit spectroscopic analyses to few-layer MoS2 to confirm optical and optoelectronic characteristics. We found that PL yield for our MoS2 films was maximized around n=15, therefore we focused subsequent analysis on few-layer material produced with 15 pulses. The Raman spectrum in Figure 5 (a) exhibits in-plane (E2g1) and out-of-plane (A1g) modes associated with 2H-MoS2 at 384.7 cm−1 and 407.2 cm−1, respectively. The broad asymmetric feature at 454 cm−1 has been ascribed to a superposition of second-order zone-edge phonon 2LA(M) and the first-order optical phonon A2u53. These modes were previously observed in bilayer MoS2 from natural crystals. While the position and the separation of E2g1 and A1g are oftentimes correlated with the number of MoS2 layers53,54, quantitative relationships have only been established for exfoliated single crystal materials. Since line positions are influenced by the local electronic environment, an exact determination of film thickness for CVD films is complicated by factors such as local inhomogeneities (e.g., simultaneous sampling of multiple grains), rotational stacking faults, and grain size55. For these reasons, we rely on XPS and HRTEM for thickness measurements as described earlier.

Figure 5.

Figure 5

Raman (a) and PL (b) spectra for a few-layer MOCVD MoS2 film (n=15) deposited on SiO2. X-ray photoelectron spectra from the same surfaces are shown for the Mo 3d region in (c) and the S 2p region in (d).

To further assess the optoelectronic properties of our MOCVD films, we turn to photoluminescence (PL) spectroscopy. PL can often complement Raman spectroscopy, since large differences in PL yield can help discriminate between monolayer (ML) and few-layer MoS22. The PL spectrum of the same surface from Figure 5 (a) is shown in panel (b). The two broad features centered at 2.04 eV (656.0 nm) and 1.89 eV (607.6 nm) are assigned to the A and B excitons, respectively, originating from the direct gap transition at the K point. The energy of the A and B excitons are consistent with measurements from natural MoS2 samples, and the simultaneous presence of the two transitions generally suggests a multi-layer film2,56,57. As with Raman, existing literature on PL of MoS2 focuses on single-crystal measurements. Since our MOCVD films are polycrystalline and likely comprise an ensemble of layers (i.e. a mixture of different layer numbers), a reliable determination of thickness or layer number is left to other measurements.

Chemical analysis by XPS of the same films produced with n=15 is shown in Figure 5 (c) and (d). The high resolution spectrum in Figure 5 (c) shows Mo 3d and S 2s core-levels. Two types of Mo species are apparent due to the presence of two Mo 3d doublets. The lower binding energy (B.E.) doublet is ascribed to MoS2, with the 3d5/2 and 3d3/2 spin-orbit components positioned at 229.1 eV and 232.3 eV (Δ=3.15 eV), respectively, comparable to values reported for natural MoS2 crystals45. Oxidized Mo is observed as a higher B.E. doublet at 232.3 eV and 235.5 eV, likely from the oxidation of unsaturated Mo sites upon exposure to air. This thin oxide layer is typically described as MoO3 and is known to develop58 over time on both natural and synthetic MoS2. A broad S 2s transition is found at 226.4 eV, as expected for MoS2. Looking at the corresponding S 2p transition in (d), only one species of S is apparent, with the position of the S 2p doublet (162.2 eV and 163.3 eV) consistent with S-Mo bonding in MoS2. The presence of the Si 2s peak at 154.8 eV confirms that the MoS2 film is thin enough to transmit photoelectrons from the underlying SiO2/Si substrate (<8 nm). The main impurity found in the films is graphitic carbon, which will be discussed in more detail below.

To investigate the crystal structure of the MOCVD films, we grew ≈25 nm thick MoS2 using 200 pulses of Mo and S precursors and analyzed the XRD patterns generated therefrom. The XRD pattern in Figure 6 was obtained by measuring a θ-2θ scan from such a film. The as-grown film is crystallized into the single phase 2H-MoS2 hexagonal polytype with space group P63/mmc (D6h4 in Schönflies notation, or #194 in ITC59). In agreement with the layered structure apparent in the HRTEM images, strong (000l) texturing in the 2θ scan indicates c-plane oriented growth. Refined lattice parameter c = 1.2306(5) nm was obtained using PDF #01-073-1508 (ICCD, 2010) and is consistent with values reported in the literature60,61. Plane spacing of d=c2=0.612nm was also in excellent agreement with values reported elsewhere62. Since the XRD patterns were obtained from thick MoS2 specimens (n=200, ≈25 nm), reasonable agreement between the calculated d and HRTEM layer spacing for few-layer MoS2 (n=25) indicates that a considerable degree of crystallinity persists even for thick MoS2 films. The relatively narrow rocking curve shown in the inset to Figure 6 is further evidence to the high level of texturing in the MOCVD films.

To assess the bulk composition and stoichiometry of our MOCVD grown material, we used the same ≈25 nm thick MoS2 film (n=200) for XPS analysis. The main impurity in the film was found to be carbon, which is discussed in more detail below. We found that C accumulation in the film was correlated with the number of pulses used to grow the film. To exclude contributions from adventitious hydrocarbons, we sputtered the MoS2 surface prior to compositional analysis. The depth profile obtained from this analysis is shown in the Supporting Information (Figure S5). Elemental impurities left in the film after 60 s of Ar+ sputtering were carbon (5%) and oxygen (5%). The true internal composition of the film could not be measured by XPS, as longer ion milling suffers from preferential sputtering of sulfur63. Film stoichiometry near the surface was determined to be S:Mo = 1.95±0.01 as calculated from the Mo 3d and S 2p core levels. A small degree of sulfur deficiency due to undercoordinated Mo edge sites has also been noted for other synthetic MoS2 films and is likewise encountered in natural single crystals64.

In addition to process characteristics and optoelectronic properties, we also evaluated the growth chemistry of our MOCVD process. To assess the role of each precursor in the deposition process, we grew thick films at 591 °C with and without a sulfur source and compared the binding state of Mo, N, C, and S core electrons. Photoelectron spectra from these films are shown in Figure 7, where the lower spectra (black) represent films grown using (NtBu)2(NMe2)2Mo alone and the upper spectra (blue) denote those grown using the Mo source together with Et2S2. The Mo 3p region for the surface exposed to sulfur, in panel (a), shows evidence for a single Mo species that dominates the spectrum. Here, the doublet at 395.0 eV and 412.5 eV satisfies the 2:1 area ratio for spin-orbit splitting and is ascribed to MoS2. The broad feature at 417.4 eV is likely a surface plasmon peak, also observed in pristine MoS2 specimens45. While a small MoO3 component can be discerned in the spectrum, this contribution is more readily evident in the Mo 3d region. Looking at the spectrum from a surface exposed to the Mo precursor only (lower trace), two doublets are clearly resolved. However, the doublets alone do not fully account for the Mo 3p core spectrum, since the relative intensity relationship between the 3p3/2 and 3p1/2 peaks requires the presence of an additional component at 397.8 eV. This peak corresponds to the N 1s transition, likely a result of N-Mo bonding. The presence of the N KLL Auger transition in the survey spectrum further corroborates this hypothesis (Figure S6). The position of the lower B.E. Mo 3p3/2 component is consistent with either a sulfide or a nitride species. We discount the possibility of metallic Mo since Mo0 would be expected at a lower binding energy. Indeed, the Mo 3d and S 2s regions in Figure 7 (c) clearly indicate the presence of MoS2 when Et2S2 is used in the reaction, and show oxidized Mo in addition to the lower B.E. doublet when the reaction is run without Et2S2. The relatively large contribution from MoO3 in the Mo-only film indicates that a significant fraction of the deposited film consists of unsaturated Mo (possibly metallic) that is subsequently oxidized upon removal from the reactor (≈160 °C). The position of the lower B.E. Mo 3d doublet is consistent with either MoS2 or MoxNy, but the relative absence of sulfur (<3 %, from residual sulfur in the reactor) and the detection of N 1s favors the latter possibility. The peak shape of the Mo 3d5/2 transition at 228.9 eV is also consistent with Mo nitride, which is known to produce asymmetric peak shapes since MoN is a good electrical conductor65.

Figure 7.

Figure 7

High resolution XPS spectra and synthetic peak fitting in the Mo 3p (a), C 1s (b), and Mo 3d (c) core levels from films prepared using n=200 pulses with (X = Et2S2) and without (X = None) a sulfur co-reactant.

The interpretation of the Mo regions is corroborated by the C 1s spectra, shown in Figure 7 (b). For the films grown with and without a sulfur source, the salient differences in the C 1s region are the absence and presence of oxidized carbon species. For the surface exposed to Et2S2, the C 1s region shows a single asymmetric peak at 284.2 eV, which is ascribed to graphitic carbon due to its unique asymmetric peak shape66. In contrast, the surface that was only exposed to the Mo precursor produces a C 1s spectrum with two additional peaks at 286.6 eV and 288.6 eV. The former peak most likely stems from C-O bonding, with the latter peak position being high enough in B.E. to denote C=O or C-N. Since the Mo and S precursors do not possess any oxygen-containing functionality, the incorporation of O into the films is largely a result of atmospheric exposure, although a low background of oxygen in the reactor cannot be excluded. The notable absence of distinct C-O or C=O related peaks in the Et2S2-exposed surface makes it unlikely that adventitious carbon is the source of these oxygen-containing groups. A plausible explanation of the spectra is the generation of C-O and C=O functionality on the film surface upon expose to air, possibly by oxidation of unreacted ligands on the surface. This suggests that a ligand removal mechanism may play a part in the deposition process and Et2S2 is not simply a source of sulfur atoms, but rather a reactant that interacts with the growth surface or the metal precursor in the thermal boundary layer. This hypothesis is further supported by the observation that residual nitrogen remains in the films when the sulfur source is omitted, but N-containing ligands (amides and imides) are absent when Et2S2 is used during growth. Therefore, the chemistry behind our MOCVD MoS2 growth is not a simple case of Mo0 deposition followed by sulfurization. This apparent interaction between precursor ligands is also distinct from processes that use Mo(CO)6, which thermally decomposes67 into Mo0 and can be subsequently sulfurized68. Since reaction chemistry plays a part in growth, our MOCVD process highlights the opportunities in new precursor design and reaction schemes for scalable and controllable TMD growth processes.

4. CONCLUSION

Large area and controllable growth of TMDs require reaction chemistries that are compatible with industrially relevant growth techniques such as MOCVD. We have presented process characteristics and film properties for wafer-scale growth of 2H-MoS2 using metalorganic and organosulfur reagents in a pulsed MOCVD reactor. Polycrystalline few-layer films were produced at comparatively low temperatures (<600 °C) with fast deposition times on the order of seconds to minutes. Pulsed injections of precursor vapors facilitated excellent control over film thickness, producing films of <1 nm to 25 nm in thickness, with a growth rate of 0.12 nm/pulse. Our process demonstrates the feasibility of using low vapor pressure metalorganic sources as reagents for TMD growth and presents a viable alternative to various inorganic sources used up to this point. Moreover, the large library of metalorganic compounds offer process designers the flexibility in choosing reagents based on volatility, thermal stability, and reactivity. While the temperature of our process imposes limitations on TMD grain size, low temperature and fast processing could be advantageous for applications requiring thermal compatibility with flexible glass substrates and low cycle times for roll-to-roll processing.

Supplementary Material

Supp1

Figure 2.

Figure 2

Photographs of 50 mm diameter fused quartz wafers demonstrate wafer-scale growth of MoS2. Left to right: a blank wafer and wafers with MoS2 deposited with varying numbers of pulses. Logo that appears in the background used with permission of the National Institute of Standards and Technology (NIST).

Acknowledgments

We would like to thank SUNY Poly SEMATECH (formerly SEMATECH) for providing diethyl disulfide (Air Products) and EMD Performance Materials for supplying the (NtBu)2(NMe2)2Mo precursor.

Certain commercial equipment, instruments, and materials are identified in this publication to adequately specify the experimental procedure. Such identification in no way implies approval, recommendation, or endorsement by the National Institute of Standards and Technology, nor does it imply that the equipment, instruments, or materials identified are necessarily the best available for the purpose.

Footnotes

Notes

The authors declare no competing financial interest.

Supporting Information Available

Dependence of film crystallinity on substrate temperature, AFM and SEM images, XPS spectra of early nucleation, XPS depth profile and survey scans, thickness uniformity on quartz wafers. This material is available free of charge via the Internet at http://pubs.acs.org.

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