Open Access Article
Peter Frenzela,
Andrea Preußa,
Jörn Bankwitzb,
Colin Georgib,
Fabian Ganssd,
Lutz Mertensf,
Stefan E. Schulzbc,
Olav Hellwigde,
Michael Mehring
f and
Heinrich Lang
*a
aTechnische Universität Chemnitz, Faculty of Natural Sciences, Institute of Chemistry, Inorganic Chemistry, D-09107 Chemnitz, Germany. E-mail: heinrich.lang@chemie.tu-chemnitz.de; Fax: +49(0)371-531-21219; Tel: +49(0)371-531-21210
bFraunhofer Institute for Electronic Nano Systems (ENAS), Technologie-Campus 3, D-09126 Chemnitz, Germany
cTechnische Universität Chemnitz, Center for Microtechnologies, D-09107 Chemnitz, Germany
dTechnische Universität Chemnitz, Faculty of Natural Sciences, Institute of Physics, D-09107 Chemnitz, Germany
eHelmholtz-Zentrum Dresden-Rossendorf, Institute of Ion Beam Physics and Materials Research, D-01328 Dresden, Germany
fTechnische Universität Chemnitz, Faculty of Natural Sciences, Institute of Chemistry, Coordination Chemistry, D-09107 Chemnitz, Germany
First published on 5th April 2019
The synthesis of complexes [M(OCHMeCH2NMeCH2)2] (5, M = Mg; 7, M = Zn) is described. Treatment of MeHNCH2CH2NMeH (1) with 2-methyloxirane (2) gave diol (HOCHMeCH2NMeCH2)2 (3), which upon reaction with equimolar amounts of MR2 (4, M = Mg, R = Bu; 6, M = Zn, R = Et) gave 5 and 7. The thermal behavior and vapor pressure of 5 and 7 were investigated to show whether they are suited as CVD (= chemical vapor deposition) and/or spin-coating precursors for MgO or ZnO layer formation. Thermogravimetric (TG) studies revealed that 5 and 7 decompose between 80–530 °C forming MgO and ZnO as evidenced by PXRD studies. In addition, TG-MS-coupled experiments were carried out with 7 proving that decomposition occurs by M–O, C–O, C–N and C–C bond cleavages, as evidenced from the detection of fragments such as CH4N+, C2H4N+, C2H5N+, CH2O+, C2H2O+ and C2H3O+. The vapor pressure of 7 was measured at 10.4 mbar at 160 °C, while 5 is non-volatile. The layers obtained by CVD are dense and conformal with a somewhat granulated surface morphology as evidenced by SEM studies. In addition, spin–coating experiments using 5 and 7 as precursors were applied. The corresponding MO layer thicknesses are between 7–140 nm (CVD) or 80 nm and 65 nm (5, 7; spin-coating). EDX and XPS measurements confirm the formation of MgO and ZnO films, however, containing 12–24 mol% (CVD) or 5–9 mol% (spin-coating) carbon. GIXRD studies verify the crystalline character of the deposited layers obtained by CVD and the spin-coating processes.
Magnesium oxide is a promising candidate for the generation of thin films of inorganic high-κ metal oxide dielectrics, due to its wide band gap (7.8 eV), low refractive index (1.72), low dielectric constant (9.8), high melting point (2900 °C), chemical and thermal stability, as well as its outstanding diffusion barrier properties.12–16 Moreover, MgO thin films can be used for the protection of plasma display panels from erosion by ion bombardment.17
Several deposition methodologies for MgO and ZnO layer formation exist, including the sol–gel process in combination with spin-coating,18,19 spray pyrolysis,20,21 pulsed laser deposition,22,23 molecular beam epitaxy,24 as well as metal–organic gas phase deposition techniques such as CVD (= chemical vapor deposition)25–27 and ALD (= atomic layer deposition).28,29 Among them, CVD and spin-coating provide convincing alternatives owing to their simplicity of processing control, covering of large areas and their capability to allow adherent and reproduceable films at low cost.30–33
For ZnO film formation diverse zinc complexes such as diethylzinc,34–36 zinc acetates,37,38 alkylzinc alkoxides,39 zinc β-ketoiminates,27,40 zinc β-iminoesterates32,40 and zinc acetylacetonates41,42 are used as CVD precursors. While zinc acetate,37,38 alkylzinc alkoxide39 and zinc β-ketoiminate40 complexes give ZnO without any addition of a co-reactant, ZnEt2 requires, however, oxygen as reactive gas to produce ZnO.34–36 However, the pyrophoric nature and reactivity impedes its easy handling. In addition, ZnEt2 shows undesired pre-reactions and hence decomposition by the deposition of particulates, upstream from the heating element may occur during the precursor delivery.32,39,43
For MgO film formation, bis(cyclopentadienyl) magnesium,25,44 alkylmagnesium alkoxides,45,46 magnesium carboxylates,47,48 magnesium β-ketoiminates,49 magnesium β-diketonates26 and their diamine adducts12,50,51 are usually used as CVD precursors of which the latter ones are promising CVD candidates, due to their high volatility, good stability in the condensed and gas phase, and their straightforward synthetic procedure.12,50,51
In contrast, as spin-coating precursors mainly magnesium acetate tetrahydrate or zinc acetate dihydrate were used for the formation of the respective metal oxide layers.52,53 In addition, also MgO/ZnO composite materials are accessible.54 In combination with copper(II) acetate monohydrate CuO/ZnO layers can be obtained.55
Herein, we describe the synthesis of magnesium and zinc diolates [M(OCHMeCH2NMeCH2)2] (M = Mg, Zn). Their thermal decomposition behavior and their use as spin-coating (Mg, Zn) and CVD (Zn) precursors for metal oxide deposition on Si/SiO2 substrates is discussed.
cos
θ, where τ is the volume weighted crystallite size, K is the Scherrer constant (here taken as 1.0), λ is the X-ray wavelength, θ is the Bragg angle in °. Theta, and β is the full width of the diffraction line at half of the maximum intensity (fwhm, background subtracted). The fwhm is corrected for instrumental broadening using a LaB6 standard (SRM 660) purchased from NIST. The value of β was corrected from (β2measured and β2instrument are the fwhm's of measured and standard profiles): β2 = β2measured − β2instrument. Spin-coating experiments were carried out with a spin coater system WS-650MZ-23NPP/A1/AR1. For CVD experiments a home-built vertical cold-wall CVD reactor with heater dimension of 20 × 20 mm (BACH Resistor Ceramics GmbH) was used (for more details see ref. 56). Heating could be adjusted up to 500 °C and was controlled by a Gefran 600 module connected with a Pt100 thermosensor. The flow rates of carrier gas (N2) and the reactive gas (O2) were controlled by MKS type 247 mass flow controllers connected to the reactor by heated copper lines. The CVD system was attached to a rotary vane pump RZ 6 (Vacuubrand). The pressure of the reactor system was controlled by a Vacuubrand vacuum controller (CVC 3000) in combination with an external Pirani vacuum sensor (VSP 3000).
The surface morphology was investigated by field-emission scanning electron microscopy using a ZEISS Supra60 SEM with an accelerating voltage of 2 or 3 kV. Cross-sectional SEM investigations were carried out to determine the film thickness. Energy-dispersive X-ray analysis using a Bruker Quantax 400 system attached to a SEM was applied to determine the chemical composition of the films. The composition of the samples were investigated using a PREVAC XPS system. Monochromatic aluminum Kα radiation (1486.6 eV) was provided by a VG Scienta MX 650 X-ray source and a monochromator. The energy distribution of the photoelectrons was measured using a VG Scienta EW3000 analyzer. This analyzer was operated at 200 eV pass energy with a step size of 200 meV and a measurement time of 2.0 s for each data point for detailed spectra, and 1 eV step size and 1.0 s measurement time at each point for survey spectra. The Casa XPS 2.3.16 Pre-rel 1.4 software was used for the deconvolution of the XPS peaks. For the calculation of the atomic concentration, Scofield relative sensitivity factors (RSFs) were used. These RSFs were corrected for a monochromator-analyzer angle of 52.55°. For the escape depth correction in Casa XPS, a value of −0.75 was applied. GIXRD (= grazing incidence X-ray diffraction) measurements of the CVD and spin-coated films have been carried out with a Rigaku SmartLab 9 kW diffractometer using a parallel beam of Cu Kα radiation. The source was operated at 45 kV and 200 mA. The incidence angle was set to 0.32° for the ZnO films and to 0.25° for the MgO layer in order to maximize the reflex intensity of the thin films and only the detector axis was moved to perform the 2θ scans. The samples have been rotated within the film plane to an offset of approximately 5° so that any reflexes from the single-crystalline silicon substrate were mostly suppressed. The incident beam was limited to 5 mm × 0.1 mm and the detector was equipped with a parallel slit analyzer. The integration time per data point was set to 1.5 s for the layers C and D, 6 s for the other layers.
Anal. calcd for C10H24N2O2 (204.31 g mol−1): C, 58.79; H, 11.84; N, 13.71. Found: C, 58.70; H 11.65; N, 13.70. Bp: 85 °C at 5 × 10−2 mbar. IR (CHCl3, NaCl; cm−1): 3400 (br), 2974 (vs), 2849 (vs), 2804 (vs), 1455 (vs), 1413 (m), 1377 (m), 1356 (m), 1331 (s), 1299 (s), 1136 (s), 1067 (vs), 1034 (vs), 956 (s), 843 (s), 772 (vs). 1H NMR§ (CDCl3, δ): 4.79 (s, br, 4H, OH), 3.75–3.83 (m, 4H, CH), 2.61–2.68 (m, 2H, CH2), 2.44–2.55 (m, 4H, CH2), 2.20–2.32 (m, 22H, CH3, CH2), 1.06 (d, 3JHH = 6.20 Hz, 6H, CH3), 1.05 (d, 3JHH = 6.20 Hz, 6H, CH3). 13C{1H} NMR§ (CDCl3, δ): 65.29 (CH2), 64.86 (CH2), 64.29 (CH), 64.17 (CH), 55.82 (CH2), 54.70 (CH2), 43.77 (CH3), 43.11 (CH3), 20.07 (CH3), 20.01 (CH3). HRMS (ESI-TOF, m/z): calcd for C10H25N2O2 [M + H]+: 205.1911, found 205.1954.
Anal. calcd for C10H22MgN2O2 (226.60 g mol−1): C, 53.00; H, 9.79; N, 12.36. Found: C, 53.11; H 10.05; N, 12.30. Mp: 100 °C decomposition. IR (KBr; cm−1): 2965 (vs), 2848 (vs), 2803 (vs), 2652 (w), 2595 (w), 1459 (s), 1421 (w), 1359 (m), 1315 (m), 1296 (m), 1209 (w), 1165 (s), 1135 (s), 1094 (s), 1065 (vs), 1031 (s), 985 (s), 962 (m), 943 (m), 864 (w), 806 (w), 618 (m), 572 (s), 514 (m). 1H NMR (CDCl3, δ): 4.3–0.7 (m, CH, CH2, CH3). 13C{1H} NMR (CDCl3, δ): see the ESI. HRMS (ESI-TOF, m/z): calcd for C10H23MgN2O2 [M + H]+: 227.1604, found 227.1690.
Anal. calcd for C10H22N2O2Zn (267.67 g mol−1): C, 44.87; H, 8.28; N, 10.47. Found: C, 44.46; H 8.55; N, 10.15. Mp: 160 °C decomposition. IR (KBr; cm−1): 2965 (vs), 2911 (vs), 2847 (vs), 2571 (m), 1467 (s), 1457 (s), 1355 (s), 1338 (m), 1328 (m), 1312 (s), 1272 (w), 1206 (w), 1187 (w), 1136 (vs), 1088 (vs), 1073 (vs), 1048 (s), 978 (vs), 964 (s), 923 (s), 853 (s), 826 (m), 794 (m), 608 (m), 581 (s), 513 (s). 1H NMR (C6D6, δ): 4.5–0.6 (m, CH, CH2, CH3). 13C{1H} NMR (C6D6, δ): see the ESI. HRMS (ESI-TOF, m/z): calcd for C10H23N2O2Zn [M + H]+: 267.1046, found 267.1045.
Compounds 3, 5 and 7 were characterized by elemental analysis, IR and NMR (1H, 13C{1H}) spectroscopy and high-resolution ESI-TOF mass-spectrometry (Experimental). Additionally, the thermal behavior of 5 and 7 was studied by thermogravimetry (TG) and TG-coupled mass-spectrometry (TG-MS) (7). In addition, the vapor pressure of 7 was determined.
In the 13C{1H} NMR spectrum of 3 two sets of resonance signals can be observed due to its diastereomeric character (Experimental). Upon the reaction of 3 with 4 and 6, respectively, the 1H and 13C{1H} NMR spectra become more complex due to the formation of different isomers (see the ESI‡), an assignment of signals was not possible.
Characteristic in the IR spectrum of 3 is the appearance of the
(OH) vibration at 3400 cm−1, which disappears upon complexation to M (M = Mg, Zn). Hence, IR spectroscopy is suitable to monitor the reaction of 3 with 4 and 6 to give 5 and 7.
In the ESI-TOF mass-spectra the protonated molecular ion peaks [M + H]+ could be detected at m/z = 205.1954 for 3, 227.1690 for 5 and 267.1045 for 7.
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| Fig. 1 TG traces of 5 and 7 under an atmosphere of oxygen (left) and argon (right) (gas flow 20 mL min−1, heating rate 10 °C min−1). | ||
| Compd. | Decomp. range (Ar) [°C] | Decomp. range (O2) [°C] | Calcd MO content [%] | TG residue (Ar) [%] | TG residue (O2) [%] |
|---|---|---|---|---|---|
| a Decomp. = decomposition; MO = metal oxide. | |||||
| 5 | 100–480 | 80–530 | 17.8 | 17.4 | 18.2 |
| 7 | 160–400 | 120–490 | 30.4 | 22.1 | 30.1 |
Powder X-ray diffraction (PXRD) measurements of the residues obtained after TG confirmed the formation of crystalline MgO (complex 5) [ICDD 00-045-0946] and ZnO (7) [ICDD 01-070-8070], respectively (Fig. 2). The related crystallite sizes were calculated by using the Scherrer equation (Experimental). The estimation reveals crystallite sizes of 11 ± 1 nm for 5 and 43 ± 5 for 7, respectively.
In addition, TG-MS studies were carried out on the example of 7 in order to get a deeper insight into the decomposition behavior of this species. The appropriate TG-MS traces including the TG trace, its first derivative and the respective mass-to-charge ratios (m/z) are depicted in Fig. 3. It is concluded that between 120 °C and 230 °C a partial evaporation and decomposition of 7 occurs, resulting in a weight loss of 25.3%. The fragments detected are of low intensity. The 2nd decomposition step (230–400 °C) illustrates an overall weight loss of 52.8% with m/z fragments of higher intensity (Fig. 3). As characteristic ions, CH3+ (m/z = 15), C2H2+/CN+ (26), C2H3+/HCN+ (27), C2H5+/CHO+ (29), CH4N+/CH2O+ (30), C2H4N+/C2H2O+ (42) and C2H5N+/C2H3O+ (43) could be detected, indicating the cleavage of Zn–O, N–C and C–C bonds.
log p = A − B/T
| (1) |
To compare the volatility of 7 with literature known systems, zinc chelate complexes such as the fluorinated zinc acetylacetonate [Zn{CF3C(O)CHC(O)CH3}2]57 and the zinc β-ketoiminate [Zn{CF3C(O)CHC(NH(CH2)2OMe)Me}2]58 have been used as reference compounds. It should be noticed that there is a lack of vapor pressure measurements for the zinc chelate compounds, despite of their wide use in the numerous applications for deposition of ZnO. Complex 7 possesses a vapor pressure of 10.4 mbar at 160 °C (Fig. 4). This value is comparable with the one for [Zn{CF3C(O)CHC(O)CH3}2] (140 °C of 11.1 mbar)57 but significantly higher than the vapor pressure for [Zn{CF3C(O)CHC(NH(CH2)2OMe)Me}2] (0.53 mbar at 160 °C).58 Hence, complex 7 was investigated for its applicability in the low pressure CVD process (see below).
In a typical deposition experiment, precursor 7 was heated to 165 °C in the CVD vaporizer unit under a pressure of 1.1–1.7 mbar (Table 3). The reactor walls were additionally heated (100 °C) to achieve a continuous precursor flow rate. According to TG studies (Fig. 1) the substrate temperature was set to 250 °C and thereafter was increased stepwise up to 450 °C producing layers A–D (Table S1, see the ESI‡). For all CVD studies the deposition time was adjusted to 45 min for a better comparison of evaporation and growth rates. To the carrier gas different ratios of the reactive gas oxygen (N2
:
O2 = 1
:
1, 3
:
1) were added (Table 3). Under all applied deposition conditions, the formation of thin zinc oxide layers was observed. The morphology and layer thicknesses of the as-deposited films were determined by Scanning Electron Microscopy (SEM). It was found that the reactive gas flow rate and the substrate temperature strongly influence the growth rate and hence the layer formation. The obtained layers are dense and conformal with a granulated surface morphology with layer thicknesses up to 140 nm (Table 3). The thinner films are metallic silver colored, whereas thicker films possess a golden or bluish metallic appearance.
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| Fig. 5 SEM images of as-deposited layers A–D and a cross-sectional image (bottom right) of layer D using 7 as CVD precursor, deposited on Si/SiO2 substrates (for layer composition see Table 4). | ||
The layer thicknesses of the respective films were determined to 7 nm (A), 8 nm (B), 65 nm (C) and 140 nm (D) from cross-sectional SEM images (Table 3). Exemplary, the cross sectional view of layer D is shown in Fig. 5, whereas all other images are presented in Fig. S1–S4 (see the ESI‡). Layers A and B show similar film thicknesses and hence equal growth rates, though the deposition temperature for the formation of layer B is 80 °C higher than for A, but the higher applied temperature effects more granulated surface morphologies (layer B). A significant increase of the growth rate was achieved, when the gas flow rate of oxygen was enhanced from 20 mL min−1 to 60 mL min−1 as evidenced for layer C (1.5 nm min−1; for comparison 0.2 nm min−1 B). The deposition rate of 7 could be further increased to 3.1 nm min−1 by applying a higher substrate temperature of 450 °C.
The film composition of the as-deposited layers A–D was analysed by EDX spectroscopy using different electron beam energies, showing a similar pattern of zinc and oxygen signals for all films. Representative, the EDX spectrum of layer A is depicted in Fig. 6, whereas all other EDX spectra of the layers A–D (Fig. S5–S8) are shown in the ESI.‡
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| Fig. 6 EDX spectra of layer A obtained from 7 by CVD showing the characteristic pattern of zinc and the presence of oxygen, carbon and silicon by using an electron beam energy of 3 keV. | ||
Moreover, carbon and silicon could be detected. In spite of low electron beam energy (3 keV) the signal intensity for Si of the A and B films is very high, ascribing to excitation of the substrate material, due to the thin film thickness of the as-deposited layers. Contrastingly, EDX spectra of thicker layers (C and D) show no or signals of rather low intensity.
In order to determine the film composition without penetration of the underlying native SiO2 layer and silicon wafer, surface sensitive ex situ XPS measurements were performed. All XPS measurements were carried out on the respective ZnO surfaces and in the layers (Fig. 7 and S11–S14 (ESI); Tables 4 and S1 (ESI)‡). Since XPS is a surface sensitive measurement method, contaminations on the surface may be overestimated, therefore, the airborne hydrocarbon impurities and carbon surface contaminations of precursor molecules on the topmost layer have been removed by argon ion sputtering (4 keV, 5 mA current at an angle of 60° with respect to the sample plane, 5 min, 2 × 2 mm2 sputtering field). Concentration quantification was achieved by using standard single element sensitivity factors.59 The Zn 2p3/2, O 1s and C 1s peaks appearing at 1021.2 eV, 529.6 eV and 284.6 eV were used to calculate the chemical composition.
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| Fig. 7 Ex situ XPS spectra of the ZnO layer C obtained from 7 at 400 °C (N2, 60 mL min−1, O2, 60 mL min−1, after 5 min sputtering, Ar+, 4 keV). | ||
The XPS measurements of the layers confirm the presence of zinc, oxygen and carbon in the deposited films. The typical XPS spectrum of the ZnO layer C deposited at 400 °C and the corresponding detailed XPS spectra of Zn 2p3/2, O 1s and C 1s after the sputtering process (5 min, Ar+, 4 keV) are shown in Fig. 7 and 8. Detailed XPS spectra of layers A, B and D are depicted in the ESI (Fig. S17–S19‡).
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| Fig. 8 Ex situ detailed XPS spectra of Zn 2p3/2 (left), O 1s (middle) and C 1s (right) of layer C obtained from 7 by CVD. | ||
The XPS measurements of the layers confirm the presence of zinc, oxygen and carbon in the deposited films. The spectra of layers A–D show two main peaks located at 1044.2 eV and 1021.2 eV, which correlate with Zn 2p1/2 and Zn 2p3/2,60,61 respectively (Fig. 7, S11–S14 (see the ESI‡)). For all received films the binding energy difference between Zn 2p1/2 and Zn 2p3/2 is 23 eV, which is in good agreement for ZnO layers of different morphologies.61,62 This value together with the binding energy of Zn 2p1/2 and Zn 2p3/2 confirms the +2 oxidation state of Zn in the ZnO layers.61,62 Also, the position of O 1s at 529.6 eV verifies the formation of ZnO.61,62 Table 4 shows the composition of layers A–D after 5 min Ar ion sputtering, whereas the configuration of the surface is summarized in Table S1 (see the ESI‡).
| Layer | Layer composition [mol%] | ||
|---|---|---|---|
| Zn | O | C | |
| A | 36.3 | 46.4 | 17.3 |
| B | 42.2 | 34.1 | 23.7 |
| C | 49.2 | 38.5 | 12.3 |
| D | 44.4 | 33.8 | 21.8 |
The gas flow of the reactive gas influences the amount of the carbon in the layers. The higher the gas flow of the reactive gas, the lower the carbon contamination is, as illustrated for layers B and C (Tables 3 and 4). Also, the deposition temperature has an effect on the layer element composition. It was found that higher substrate temperatures result in an increase of carbon as demonstrated for D in comparison to C. Similar results were reported for the ZnO layers deposited by using diethyl zinc in the MOCVD process.63 In this context it is understandable that the carbon content of layer A is placed between the ones of films C and D, which is attributed to the lowest applied substrate temperature for deposit A using identical gas flow conditions as characteristic for layer B formation (Table 4).
The reason for the carbon contamination most likely is based on an uncontrolled and incomplete decomposition of the precursor depending on the used deposition conditions. Hence, the carbon impurity is higher on the surface areas then in the respective layers A–D (Tables 4 and S1 (ESI‡)), which can be ascribed to adsorbed precursor molecules 7 and/or hydrocarbons on the layer surface.
GIXRD measurements were carried out to prove the crystallinity of the as-deposited films. Representative, the diffractogram of layer D is depicted in Fig. 9, whereas the XRD patterns of A–C are presented in Fig. S22–S24 (see the ESI‡). It was found that the crystalline part of layers A–D consist of hexagonal ZnO (31.76°, 34.44°, 36.25°, 47.55°, 56.57°, 62.88°, 66.35°, 67.94°, 69.06°; [ICDD 01-070-8070]).
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| Fig. 9 GIXRD spectra of layer D with reflections of ZnO (red), applied deposition parameters are given in Table 3. | ||
Also, from Fig. 9 and S22–S24 (see the ESI‡) it can be seen that layers B–D show relatively sharp reflections, whereas the ones of layer A are less intense and broad. This cannot be ascribed to the different film thicknesses, since layers A and B demonstrate approximately the same thickness (Table 3). Presumably, in the case of layer A the lower deposition temperature of 320 °C affords smaller crystallite sizes or a lower fraction of crystalline material compared to layer B, which was deposited at 400 °C. The relatively large reflection at ca. 54° of A can be assigned to the Si/SiO2 substrate (Fig. S22, see the ESI‡).
As it can be seen from the SEM images (Fig. 10), the respective deposits are dense. The MgO layer shows a grainy morphology as compared to the respective conformal ZnO coating. Cross-sectional SEM studies were carried out for all samples in order to determine layer thicknesses and growth rates, respectively (Fig. 10, Table 5). Layer thicknesses of 80 nm for MgO (layer E) and 65 nm for ZnO (layer F) were observed.
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| Fig. 10 SEM Images of the respective MgO (layer E) and ZnO (layer F) (top view, left) and cross-sectional images (right) deposited on Si substrates covered with a native SiO2 layer. | ||
The elemental composition of the as-deposited films was investigated by EDX, showing the typical zinc and magnesium pattern (Fig. S9 and S10, see the ESI‡). In addition, signals for Si and C were detected of which the Si signal most likely originates from the Si/SiO2 substrate. The carbon impurities may stem from airborne hydrocarbon.
Additionally, XPS measurements for the spin-coated layers were performed to determine the elemental composition of the surface and the layer (Tables 6 and S1 (ESI‡)). Argon sputtering was performed to remove the topmost layer. The survey spectra of layers E and F are depicted in Fig. 11, whereas the spectra of the corresponding surface areas are summarized in Fig. S15 and S16 (see the ESI‡).
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| Fig. 11 Ex situ XPS survey spectra of layer E (left, obtained from 5) and layer F (right, obtained from 7) by spin-coating (Table 5) (after 5 min sputtering, Ar+, 4keV). | ||
Detailed XPS spectra of the respective deposits are depicted in Fig. S20 and S21 (see the ESI‡). The Mg 2p, Zn 2p3/2, Zn 3d, O 1s and C 1s peaks were used to calculate the chemical composition of the deposits. In case of layers E and F the elemental composition of the surfaces and layers is quite similar (Table S1,‡ Table 6). In general, the layers themselves consists of 37 mol% Mg (layer E), 38 mol% Zn (layer F), 53 mol% O, and ca. 9 mol% impurities (ZnO: carbon; MgO: carbon and fluorine) (Table 6). As fluorine source the decomposed Teflon grease could be identified, which was used in the synthesis of 5 and 7 and in the preparation of the spin-coating solutions. The peak positions of Mg 2p (50.8 eV), Zn 2p3/2 (1021.4 eV), Zn 2p1/2 (1044.4 eV), O 1s (530.5 eV, MgO; 529.6 eV, ZnO) are in agreement with earlier reports on these elements, confirming the formation of metal oxide films.49,61,62,66,67 In the case of MgO this could also be confirmed by the XPS detailed spectra of the C 1s peak, where also the KLL auger line of Mg at 307.9 eV was detected (Fig. 12).68
The difference of surface and layer composition for elements Zn/Mg and C could be assigned to the impurities of the topmost layer.
To evaluate the crystallinity of the as-deposited films, GIXRD measurements were performed (Experimental). The respective diffractograms of layers E and F are depicted in Fig. 13.
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| Fig. 13 GIXRD spectra of layer E (left) with reflections of MgO (red) and F (right) with reflections of ZnO (red), applied deposition parameters are given in Table 5. | ||
According to Fig. 13 the crystalline part of layer E consists of cubic MgO [ICDD 00-045-0946] as evidenced by the reflections at 36.86°, 42.83°, 62.17°, 74.52° and 78.45° representing the respective (111), (200), (220), (311) and (222) planes of the crystal structure. The other peaks match the reflections characteristic for silicon. In the case of layer F GIXRD measurements confirmed the formation of hexagonal ZnO in analogy to the results obtained by the CVD experiments. The exceptional sharp peak at around 47° consist of a reflection of hexagonal ZnO (47.55°; ICDD 01-070-8070) as well as a reflection (47.30°) originating from the Si substrate.
Footnotes |
| † Dedicated to Prof. Dr Thomas F. Fässler on the occasion of his 60th birthday. |
| ‡ Electronic supplementary information (ESI) available: Fig. S1–S24, Table S1, NMR and IR spectra giving additional experimental data and spectroscopic details for all new compounds. See DOI: 10.1039/c9ra00585d |
| § NMR data are given for two diastereomers. |
| This journal is © The Royal Society of Chemistry 2019 |