Phase Transformations in Arc-Evaporated Ti-Si-N Thin Films Axel Flink1, Manfred Beckers1, Jacob Sjölén2, Tommy Larsson2, Slavomir Braun3, Lennart Karlsson2, and Lars Hultman1 1 Thin Film Physics Division, Department of Physics, Chemistry, and Biology, IFM, Linköping University, SE-581 83 Linköping, Sweden 2 3 Seco Tools AB, SE-737 82 Fagersta, Sweden Division of Surface Physics and Chemistry, Department of Physics, Chemistry, and Biology, IFM, Linköping University, SE-581 83 Linköping, Sweden Abstract (Ti1-xSix)Ny (0≤x≤0.20) thin solid films have been deposited by arc evaporation onto cemented carbide (WC-Co) and sintered c-BN substrates. X-ray diffraction and TEM analyses show that low-Si content films up to x=0.09 exhibit a dense columnar singlephase cubic (Ti,Si)N solid solution while 0.14≤x≤0.20 films assumes a defect-rich, feather-like nanostructure consisting of cubic nanometer size (Ti,Si)N crystallites and amorphous SiNz:Ti phases. Correspondingly, the N content in the films measured by elastic recoil detection analysis increases close to linear with increasing Si content from y=0.99 (x=0) to y=1.13 (x=0.20). X-ray photo-electron spectroscopy reveals tetrahedral SiNz binding configuration. The nanoindentation hardness of as-deposited films increases with increasing Si content from 30 GPa (x=0) to 42 GPa (x=0.14). For higher Si contents, up to x=0.20, the hardness decreases again to 38 GPa. Annealing experiments show that films retain composition and hardness up to 1000 °C for 0.04≤x≤0.09 due to a thermodynamically driven phase segregation to residual (Ti,Si)N and a coherent SiNz grain boundary phase. For x<0.04, the films soften by thermally-induced recovery effects 1 within the film. For x>0.09, Si and N diffuse out of the films along boundaries accompanied by Co and W interdiffusion from the substrate, yielding recrystallization, grain boundary weakening and a corresponding decrease of hardness to <28 GPa. Sidepletion is also observed during annealing of films with x=0.17 and x=0.19 on thermally more stable c-BN and Ta substrates, respectively. This is again accompanied by domain recrystallization; the hardness is, however, almost retained at 38-40 GPa. At 1200 °C, the films have fully recrystallized into nanocrystallites of TiN and porous grain boundaries where Si and N out-diffusion took place. A residual Si content of ?? is still present in the film. Introduction Materials science and advanced surface engineering are employed to develop wearresistant coatings for metal cutting tools with superior thermal properties, chemical inertness, and mechanical strength [1,2] with the objective to enable higher cutting speeds with correspondingly higher working temperatures. Such combination of material properties is sought for in ternary or quaternary ceramic coatings deposited by physical vapor deposition. In particular, the Ti-Si-N system exhibits interesting properties for metal cutting applications. Adding Si to TiN results in hardening for TiN-Si3N4 nanocomposites [3,4,5], TiN/SiNx multilayers [6,7,8], and metastable (Ti1-xSix)N solid solutions [9,10,11]. There is, however, no stable ternary phase reported in the Ti-Si-N phase diagram [12]. The cubic (Ti1-xSix)N solid solutions are the least explored of the Ti-Si-N structures mentioned above. Yet, the solid solution hardening is substantial. We previously showed 2 that (Ti1-xSix)N films deposited by arc evaporation at 500 °C exhibit an essentially linear hardness increase with increasing Si from ~31 GPa in pure TiN to ~45 GPa for Ti0.86Si0.14N [9]. Moreover, the hardening of the solid solutions is retained during isothermal annealing at 900 °C in Ar for 2 h. By contrast, TiN softens significantly to ~25 GPa during such annealing because of recrystallization and residual stress recovery. The upper limit of Si supersaturation in a cubic alloy with TiN is difficult to assess for analysis reasons. For the possibility of a spinodal decomposition reaction, the range of NaCl-structure Ti1-xSixN alloy compositions was shown by ab initio calculations to have a lattice parameter which deviates less than 0.5 % from that calculated for TiN [13,14]. This makes it difficult to detect such phase separation and solid solution alloying by x-ray diffraction. The strong segregation tendency of the species in a nitride solid solution, however, will eventually lead to phase transformation into TiN and SiNx. In such a case, the analysis challenge becomes one of detecting the smallest volumes of SiNx in a crystalline matrix. Here, we present a combination of high-resolution imaging and analytical techniques to investigate both the details of phase transformations for different Si contents, and the actual nitrogen content in the films, which we hereafter denote as (Ti1-xSix)Ny. It is found that the forced solid solubility limit for Si in cubic (Ti1-xSix)Ny thin films synthesized by arc evaporation is x≈0.1 (~5 at.%). As-deposited films with higher Si content exhibit Si segregation and N uptake in the range 1.09≤y≤1.13 with a concomitant tendency for the formation of an amorphous SiNz:Ti phase. Nanoindentation experiments 3 show that the hardness of as-deposited films reaches a maximum of 41.8±2.0 GPa for a Si content of x=0.14. The solid solution films (0.04≤x≤0.09) are structurally stable with retained hardness after annealing at 1000 °C in Ar for 2 h. Films with x≥0.14 in the asdeposited state, however, exhibit pronounced Si and N loss by out-diffusion and desorption together with simultaneous recrystallization within the grains in the cubic state together with Co and W interdiffusion from the cemented carbide (WC-Co) substrates. Correspondingly, the post-annealing hardness decreases to <28 GPa. On the contrary, the hardness of films with x=0.17 on thermally more stable sintered c-BN substrates is, however, more or less retained at 38-40 GPa up to 1100 °C, despite local Si out-diffusion and segregation, which results in local recrystallized areas. Experimental details (Ti1-xSix)Ny coatings were deposited by arc evaporation in a Metaplas MZR323 system with a base pressure of 5x10-6 mbar. 12x12x4 mm3 cemented carbide (WC-Co(6 wt.%)), 5x5x1 mm3 sintered c-BN-(50 vol.% TiC), and 15x15x1 mm3 metallic Ta were used as substrates. The WC-Co substrates were ground and polished to a mirror-like finish with a roughness Ra ≈ 0.01 µm. Both WC-Co and Ta were cleaned ultrasonically in an alkaline degreasing agent prior to deposition. Nine samples were placed along three vertically mounted 63 mm diameter targets of composition Ti, Ti0.8Si0.2, and Ti0.75Si0.25, respectively, to obtain a Ti to Si film composition gradient. For the case of c-BN, the deposition experiments were performed using 63 mm diameter Ti0.80Si0.20 targets in order to obtain films of a constant high Si content. In both series, the arc evaporation was operated in a reactive N2 atmosphere. The substrates were negatively biased to –50 V and 4 mounted on a rotating cylindrical fixture. The substrate temperature was kept at ~500 C using a combination of plasma heating and a resistive heater. The film compositions were analyzed by time-of-flight energy and elastic recoil detection analysis (TOF-E ERDA). The measurements were performed using a 40 MeV 127 9+ I ion beam. The TOF-E setup, described in detail elsewhere [15], consists of a 437.5 mm long telescope with two carbon foil time detectors, which is followed by a ion implanted silicon charged energy detector with 10x10 mm² active area. The recoiled atoms are collected at an angle of 45° relative to the incoming beam direction. The incidence angle of the primary ions as well as the exit angle of the recoils is 67.5° with respect to the substrate normal. The resulting time-of-flight over recoil energy spectra are transformed to elemental depth profiles using the newly developed CONTES code [16]. The average film compositions and statistical errors are obtained by normalizing over the measured depth profiles over 100-300 nm sampling depth. The statistical error of the measurement is 1-2 at.%. The microstructure of the samples was investigated by x-ray diffraction (XRD), transmission electron microscopy (TEM), scanning transmission electron microscopy (STEM), and scanning electron microscopy (SEM). XRD was performed using a Bruker AXS D8-advanced x-ray diffractometer with a line-focus Cu Kα x-ray source. -2 scans were performed in the 2 range from 20 to 80. The residual stress was calculated using the sin2ψ method based on the (Ti1-xSix)Ny 422 peak in the as-deposited films with x≤0.14 and all annealed films. For as-deposited films with x≥0.14, the stress was calculated based on the 002 peak due to dominant 002 preferred off-plane orientation. For 5 all calculations a The Poisson’s ratio (ν) of 0.22 and a Young’s modulus (E) of 450 GPa was used, as were determined for TiN [17]. The indicated error bars originate from linear fitting of the measured data points. The SEM analysis was performed on a LEO 1550 FEG-SEM. An analytical FEI Technai G2 UT FEG microscope equipped with an energy dispersive x-ray spectrometer (EDX) operating at 200 kV was used for TEM, STEM, and EDX elemental mapping. For the STEM analysis, a high angle annular dark field detector (HAADF) was used and a camera length of 220 nm. The mapping was performed with a pixel resolution of 2 nm over 150x150 nm2 for as-deposited (Ti0.81Si0.19)N1.13 and 1 nm over 50x50 nm2 for (Ti0.81Si0.19)N1.13 annealed at 1000 °C for 2 h, respectively. Crosssectional TEM/STEM specimens of films deposited on WC-Co substrates were made by clamping two small sample pieces film to film into a Ti-grid, followed by mechanical grinding and polishing. Electron transparency was achieved by ion milling using a Gatan Precision Ion Polishing System. The corresponding plan-view TEM specimens were made by cutting out a disc followed by the similar steps of mechanical grinding, polishing, and ion milling. Cross-sectional TEM/STEM specimens of films deposited on c-BN and Ta substrates were prepared using a Zeiss 1540 EsB CrossBeam focused ion beam with the so-called lift-out technique [18]. X-ray photoelectron spectroscopy (XPS) measurements were conducted using a Scienta ESCA 200 with a monochromated Al (1486.6 eV) Kα beam. Survey scans were recorded in the 0-800 eV energy range with a step size of 0.5 eV for each sample. For accurate determination of the N1s, Si2p, Ti2p, O1s, C1s, Co2p, and W4f peak shapes, respectively, local region scans were recorded with a step size of 0.1 eV. In order to maintain sufficient charge neutralization for samples containing silicon, the use of a flood 6 gun was necessary. The binding energy scale of the narrow scans was calibrated by the C1s line at 284.7 eV. Scans were recorded both prior to Ar-sputtering in order to avoid sputter-induced chemical shifts, and after 20 min of Ar-sputtering at PAr =2.5x10-7 mbar in order to rule out surface-oxide contaminations. The analysis of the spectra obtained before and after sputtering, however, revealed the presence of sputter-induced chemical shifts. Hence only scans before Ar-sputtering are discussed in the paper. Isothermal annealing of the as-deposited films was carried out in a Sintevac Furnace from GCA Vacuum Industries for a duration of 120 min in Ar at atmospheric pressure in order to prevent oxidation of the sample surfaces. The individual annealing temperatures (Ta) were 1000C (WC-Co and c-BN), 1100C (c-BN), and 1200C (c-BN), respectively. The initial heating rate was 7 °C/min, which was reduced to 5 °C/min at 40 °C below the respective Ta. After the annealing the samples were cooled in the furnace with typical cooing times of 1.5 h from 1100 °C down to 500 °C and 4 h from 500 °C down to 100 °C. The film hardness was determined by nanoindentation using a Nanoindenter XP equipped with a Berkovich diamond tip. Mechanical polishing on taper sections was performed prior to the indents in order to reduce the surface roughness influence. 20 indents were made in each sample with a maximum load of Pmax=25 mN. The indentation procedure consisted of 5 segments: 1) load to Pmax, 2) hold 10 s, 3) unload to 10% of Pmax, 4) hold 60 s, and 5) unload. Any thermal drift was corrected for at hold segment 4. The average hardness and its standard deviation were determined from the obtained data following the method of Oliver and Pharr [19] by fitting 50% of the unloading curve with an 7 exponential function. The reference SiO2 sample hardness was 9.6±0.3 GPa and 9.89±0.3 GPa for the (Ti1-xSix)Ny films deposited onto WC-Co and c-BN substrates, respectively. Results and Discussion Composition of the as-deposited films Table 1 shows the composition of the nine as-deposited of the as-deposited (Ti1-xSix)Ny films on WC-Co substrates as determined by ERDA. The Si content ranges from x=0 (0.1 at.%) for the sample facing the Ti target, to x=0.20 (9.1 at.%) for the film facing the Ti0.75Si0.25 target. The corresponding N content increases close to linear with increasing Si content from y=0.99 to y=1.13. The impurity levels for all as-deposited films were below 1 at.% with a small [O] increase from ~0.45 at.% to ~0.8 at.% with increasing Si content. Table 1 reveals a substantial reduction of Si content in the films compared to the composition of the targets for the geometry of the deposition experiments. For example, the film facing the Ti0.75Si0.25 target shows a Si content of only x=0.20. This can be explained by the different average ionization for the Ti and Si species during arc evaporation, which are typically +2.1 and +1.4, respectively [20]. Using a substrate bias of -50 V, the Ti ions will hence impinge on the sample surface with a correspondingly higher energy causing persisting Ti sub-plantation, while the comparably surface-near Si will be preferentially resputtered. Hence, the film will have a reduced concentration of Si. Microstructure of the as-deposited thin films 8 Error! Reference source not found. shows x-ray diffractograms obtained from the asdeposited films on WC-Co substrates. All films have a single-phase NaCl-structure with a lattice parameter of ~4.24 Å, i.e., more or less identical to stoichiometric TiN (4.24 Å [21]). For the pure TiN film (x=0), a random crystallographic orientation is observed. The uptake of Si induces peak broadening and a <002> out-of-plane preferred orientation, which is nearly complete for x≥0.09. The residual stress (σ) of films deposited on WC-Co substrates is presented in Error! Reference source not found.(a). All as-deposited films are under substantial compressive stress, which gradually increases from x=0 at σ=-2.7±0.2 GPa, up to σ≈-5.5 GPa for x=0.19. One has to keep in mind that a linear fit of sin2ψ method data is only exact for isotropic materials. The strong preferred orientation in films with x≥0.09 may therefore reduce the accuracy of the given stress values. The same applies to the use of the low angle 002 peak, for which ψ-tilt induces smaller peak shifts compared to the high angle 422 peak. A direct comparison between the 200 and 422 peaks for the as-deposited x=0.14 film, however, resulted in similar stress values, σ=-4.83±0.28 GPa and σ=4.55±0.53 GPa, respectively, which implies that the results obtained from 002 and 422 are comparable. The residual stress values for the annealed samples will be presented below. Error! Reference source not found.(a,b) shows detailed x-ray diffractograms around the 002 peak of the as-deposited and annealed films on WC-Co. In the as-deposited state, the full width at half maximum (FWHM) values remain close to constant at ~0.5° from x=0 up to x=0.04 (Error! Reference source not found.a). Also the peak positions of 9 films with 0.01≤x≤0.09 show no peak shift when compared to TiN (x=0). Recent calculations by Alling et al. [14] predict a lattice parameter change from 4.255 Å for x=0 to 4.250 Å for x=0.125 when the Si atoms are fixed at NaCl-lattice Ti positions. If the atoms within the unit cell are allowed to relax, however, the lattice parameter for x=0.125 is predicted to be 4.231 Å. Similar results were obtained with other ab initio methods in, e.g., [14,22]. These lattice parameter changes correspond to a shift of 0.25° and 0.05° to higher angles. As the observed FWHMs are bigger than the predicted peak shifts, any alloying of Si and TiN will be virtually impossible to detect, and hence, no conclusion whether Si is dissolved in a solid solution or segregated into a-SiNz or other grain boundary tissue phases can be drawn. As for the resulting residual stress, the data obtained after annealing will be discussed later. For Si content x≥0.09, the 002 peak FWHM values increase substantially from ~0.7° to ~1.8° indicating extensive grain refinement. For x≥0.14, the 002 peak position gradually shifts slightly towards lower 2θ angles, corresponding to an out-of plane lattice parameter of 4.27 Å for x=0.19. The shift coincides with the increase of compressive stress, compare Error! Reference source not found.. This could find its explanation in the formation of a Si3N4 tissue phase with or without Ti, since Si3N4 has a substantially larger molar volume compared to the NaCl-structure solid solution. Fractured cross-sections of the as-deposited films were investigated by scanning electron microscopy. From these, the film thickness was measured to ~1.5-2.5 µm. On this relatively coarse scale the film microstructures were dense and columnar with 10 incorporated macro particles from the arc evaporation process. Films with x≥0.14 appear as fine-grained. Cross-sectional transmission electron micrographs (XTEM) and selected area electron diffraction (SAED) patterns of as-deposited TiN and (Ti0.91Si0.09)N1.04 films on WC-Co substrates are presented in Error! Reference source not found. and Error! Reference source not found.. The images of both films display a dense columnar structure, while the SAED patterns suggest a more coarse grained substructure for TiN in comparison to (Ti0.91Si0.09)N1.04. The difference in structure is expected, as Si acts as a grain refiner and induces point defects. The SAED patterns also verify the random crystallographic orientation for TiN as well as the <002> preferred out-of-plane orientation for x=0.09 observed in XRD. The high-resolution (HR) image in Error! Reference source not found.(b) shows parts of two overlapping grains with corresponding moiré fringes. The low-angle grain boundary is defined by dislocations and (semi) coherency strain. It is difficult, however, to rule out the presence of any monolayer-thick amorphous SiNz phase. Error! Reference source not found. shows TEM images as well as SAED and fast Fourier transform (FFT) patterns from the as-deposited (Ti0.81Si0.19)N1.13 film on WC-Co substrate. The film exhibits a dense, extremely defect-rich, fine grained, feather-like structure as can be seen in the cross-sectional image in Error! Reference source not found.(a). The combination of the cross-sectional SAED and plan-view FFT in Error! Reference source not found.(a,d) state an <002> fiber texture. The 002 dark-field image in Error! Reference source not found.(b) reveals that individual feathers consist 11 of bundles of elongated nm-size crystallites or nanocolumns. A HRTEM cross-sectional image of a typical bundle is shown in Error! Reference source not found.(c). It illustrates that the crystallites have low-angle grain boundaries in-between themselves. Error! Reference source not found.(d) depicts a plan-view image with an apparent phase separation into a crystalline cubic and an amorphous phase according to the lack of diffraction contrast in the latter, also after tilting of the sample. The cubic phase builds up the bundles of nanocolumns seen in Error! Reference source not found.(b,c). An EDX map across 20x20 nm2 with a pixel resolution of 0.33 x 0.33 nm2, not shown here, indicates that the crystallites consist of Ti-rich cubic (Ti,Si)N crystallites and the amorphous areas of Si-rich SiNz:Ti. The higher magnification image in Error! Reference source not found.(e) reveals that, the (Ti,Si)N crystallites in bundles are composed of ~2x2 nm subgrains (or basic structural units), which are delineated by dislocations in the form of semi-coherent grain boundaries. Consequently, individual subgrains are slightly tilted with respect to each other, causing an in-plane trans-rotation with a radius of ~100 nm (as derived from the crystal plane trace indicated by the white line in Error! Reference source not found.(e)). We propose that the {002} lattice planes are rotating in a self-organized manner due to the segregation of Si to the grain boundaries. The corresponding FFT in Error! Reference source not found.(e) from an area as small as 12x12 nm2 verifies the tilting between the subgrains. The lattice defect density assessed from counting dislocations in the sub-grains is ~1x1014 cm-2, which corresponds to values found for heavily cold work hardened material. The observed phase separation with a concomitant grain refinement agrees with the XRD analysis in which a substantial peak broadening 12 was observed for x≥0.14, c.f., Error! Reference source not found.. On a larger scale, the dark-field micrograph in Error! Reference source not found.(b) illustrates that the (Ti,Si)N-crystallites and the amorphous phase grows in a vertical lamellar mode where the grain width is determined by the rates of deposition and element partitioning on the surface for the two phases. While a self-organized nano-columnar structure has also been observed for B-superstoichiometric Ti-B thin films [23] and for Zr-Si-N films in [24], the present observation includes the in-plane trans-rotation within the columns, which is original. Chemical bonding in the as-deposited films X-ray photoelectron spectroscopy on the as-deposited TiN, (Ti0.91Si0.09)N1.04, (Ti0.86Si0.14)N1.09, and (Ti0.81Si0.19)N1.13 films on WC-Co substrates was carried out in order to investigate the chemical bonds of the solid solution and two-phase structures, respectively. The XPS scans of Ti2p, N1s and Si2p core levels are presented in Error! Reference source not found.. The seemingly high oxygen-related XPS signals can be ascribed to surface contaminations as they disappear after clean sputtering, and hence, do not contradict the overall low oxygen content determined by ERDA (compare Table I). The Ti2p signal displays three distinct peaks, associated with chemically shifted Ti2p3/2 core levels. The high binding energy feature at 458.25 eV is attributed to TiO2 [25], the other peaks at 456.7 eV and 455.2 eV correspond to Ti-O-N [26] and TiN [25], respectively. The film with highest Si content exhibits shifts for the TiO2 and TiN contributions with respect to the other films. These shifts can be tentatively assigned to the change of chemical environment in the vicinity of TiO2 due to presence of Si in the film. A change in the shape of the N1s line is observed depending on the Si content in the 13 sample. The Si contribution in the N1s signal can be observed at 398.0 eV and is assigned SiNz [27]. The contribution from Ti-N is found at 397.3 eV [25,27]. The peaks at 396.0 eV and ~396.4 eV are attributed to surface contamination such as Ti-O-N [27], since they disappear after Ar-sputtering. As observed from the normalized Si2p spectra, the recorded signal exhibits a more or less retained shape at 101.8 eV independently of the Si content in the sample. There is, however, a small peak broadening of ~0.2 eV for x=0.19 compared to x=0.09, which may be assigned to the formation of amorphous Si3N4:Ti phase. Furthermore, no SiOx peaks were detected in this analysis, which indicates that Si in the films is not subject to oxidation. Since there is no XPS data available in literature from cubic Si-N phases, we measured on a dc magnetron sputtered c-SiNx/TiN multilayer thin film from Ref. [8] where cSiNx(001) is epitaxially stabilized between TiN(001) layers. The layer thicknesses are 20 Å and 5 Å for TiN and SiNx, respectively, and are thus thin enough to provide XPS signal from several layers. Whether the c-SiNx has octahedral or tetrahedral Si-N bonds is still under discussion [8] The N1s and Si2p spectra from the c-SiNx/TiN multilayer film are included in Error! Reference source not found.. The N1s line has very similar appearance in comparison to the x=0.09 film, with corresponding peaks assigned to TiN, SiNx as well as Ti-O-N surface contaminations. The Si2p peak is observed at 102.0 eV, which corresponds to a shift of only ~0.2 eV compared to the binding energy of 101.8 eV for the as-deposited x=0.09 film. The reason for the shift may be the absence of Ti as second nearest neighbor. 14 Our interpretation of the XPS result is that the Si-N bonds have tetrahedral coordination, but the presence of octahedral coordination can, however, not be ruled out, since there are no reference values in literature. In the context whether Si is located in the amorphous or crystalline phase in the samples, XPS does not provide unambiguous evidence since the observed shifts are in the order of the energy resolution of the instrument. Hence, other techniques with higher energy resolution are suggested to reveal the bond nature of SiNz. As a final remark, we note that Ar-sputtering of the films induces peak shift for the Si2p peak, this was not taken into account in our previous paper where the shift of the Si2p peak position to 100.9 eV was most likely sputter-induced [9]. To conclude the analysis of the as-deposited (Ti1-xSix)Ny films grown by arc-evaporation onto WC-Co substrates we note that when x increases from 0 to 0.20, also y increases from 0.98 to 1.13. Films with 0.01≤x≤0.09 exhibit a metastable cubic solid solution phase with a lattice parameter of 4.24 Å, where Si acts as a grain refiner. Higher Si contents initiates a phase separation into metastable c-(Ti1-xSix)Ny nanocrystallites and an amorphous SiNz:Ti. All films are under compressive residual stress, which increases from σ=-2.7 GPa to σ=-5.5 GPa with increasing Si. XPS suggests the presence of tetrahedral binding configuration between Si-N for at least Si rich films. The location of this Si to the amorphous or cubic crystalline Ti-Si-N phases (or both), however, has not been elucidated this far. In the next section we will consider the thermal stability of the (Ti1-xSix)Ny films on WCCo after isothermal annealing at 1000 °C for 2 h. This is followed by a study on 15 thermally more stable sintered c-BN and Ta substrates annealed at 1000, 1100, and 1200 °C. Composition and microstructure of annealed (Ti1-xSix)Ny films on WC-Co In the discussion below, the films are labeled according to the as-deposited composition. To study the influence of annealing on the film composition, the nine films deposited on WC-Co were analyzed by ERDA. The corresponding compositions after isothermal annealing for 2 h at 1000 °C are presented in Table II. The solid-solution films with x≤0.09 exhibit no Si loss, while the N content decreases slightly. On the contrary, the two-phase films with x≥0.14 exhibit an increasing loss of both Si and N. It is noteworthy that regardless of the initial Si content within these films, the retained Si content after annealing is ~5 at.% (x≈0.10). This value, in fact corresponds to the effective solid solution limit found for the as-deposited films. Furthermore, besides the Si and N outward diffusion, we also observe a Co and W release from the substrate and diffusion into the films. Each of these effects which also increases with increasing Si content of the as-deposited films. In contrast, the O impurities are more or less retained for all films, whereas the C impurities increase minutely. Error! Reference source not found. shows the x-ray diffractograms from the corresponding post-annealed samples. The 1000 °C heat treatment did not induce any phase transformation as the diffractograms appear similar to those from the as-deposited films, (c.f., Error! Reference source not found.). All films have thus also preserved their texture, i.e., films with x≤0.04 exhibit a preserved random crystallographic 16 orientation, while films with x≥0.09 maintain their strong <002> out-of-plane preferred orientation. Moreover, the FWHM decreases slightly for x≤0.09 films and more prominent for x≥0.14. Results for the film residual stress states after annealing are presented in Error! Reference source not found.(b). The stress in the TiN film has decreased to around zero due to defect annihilation and grain coarsening, which are known to operate at an annealing temperature of 1000 °C [28]. Films with Si content of 0.01≤x≤0.09, exhibit a reduced, but still relatively high compressive stress of between σ=-0.9 GPa for x=0.01 and σ=-2.5 GPa for x=0.09. Structurally, this may be correlated to migration of ionbombardment induced Si defects in the NaCl lattice and the formation of an x-ray amorphous SiNz grain boundary phase. All films with higher Si contents are virtually fully relaxed, but the relaxation mechanisms is complicated by the superimposed Si and N out-diffusion and Co and W interdiffusion presented above. For a more detailed analysis on the relaxation processes we consider the XRD data presented in Error! Reference source not found.(a,b), and the FWHMs and positions of the 002 peak depending on the as-deposited Si content x. We start with the single-phase (x≤0.09) films in Error! Reference source not found.(a). TiN exhibits a small peak shift of to higher angle of ~0.1° after the annealing. This can be attributed to both the decrease of the N-content from TiN0.99 to TiN0.86 and the stress reduction. An N-substoichiometry for TiN effectively reduces the lattice parameter [29] and also a decreased in compressive stress will reduce the out-of-plane lattice parameter, and hence yield a higher 2θ-angle. Furthermore, the FWHM has decreased from ~0.55° to ~0.40°, which corroborates the 17 occurrence of point defect annihilation and grain coarsening as introduced above. The same applies to films with 0.01≤x≤0.09, but to a lower extent, correspondingly the asdeposited peak positions are retained after annealing, and the FWHM is decreased only slightly, less than 0.05°. On the other hand, all films with x≥0.14 exhibit a substantial peak shift after annealing to higher angles, close to the position of annealed TiN at 42.6° as a consequence of the virtually complete stress relaxation. Also, the FWHM decreases considerably from ~1.2-1.8° to ~0.7-0.8°, which again is due to grain coarsening, intensified by the W and Co interdiffusion. To further characterize the W and Co interdiffusion, we studied the elemental distribution in the annealed films by analytical STEM as displayed in Error! Reference source not found.. The STEM image of the 1000 °C annealed (Ti0.81Si0.19)N1.13 film in Error! Reference source not found.(a) reveals a film recrystallization into a cellular structure, with – according to the Z contrast – heavier elements gathered at the grain boundaries. Also the EDX maps in Error! Reference source not found.(b-f) state that Ti and N are accumulated within the grains, while W and Co are mainly situated at the grain boundaries. Contrary, the low Si content in combination with the overlap of Si Kα and W Mα lines does not provide evidence whether Si is located within the grains and/or at the grain boundary, see Error! Reference source not found.(c). Chemical bonding of annealed (Ti1-xSix)Ny films XPS on annealed (Ti0.81Si0.19N)1.13 at 1000 °C confirmed the presence of W and Co in the film. Scans over the Si2p peak, however, revealed a shift from 101.8 eV to ~102.3 eV. We attribute the peak shift to the formation of Si-O-N [30], due concurrent segregation of 18 Si and O to the boundary. Any Ti2Si formation due to the out-diffusion of N has binding energy at ~98 eV and can be excluded for our films. For Co-Si, which would be expected at the grain boundaries, a peak should be present at ~101 eV [31] both for Si2p and Co3s bindings. No Co-Si signal was, however, resolved. Mechanical properties (Ti1-xSix)Ny films on WC-Co The hardness of the as-deposited and 1000 °C annealed films on WC-Co substrates are presented in Error! Reference source not found.. The as-deposited TiN film exhibits a hardness of 29.8±1.5 GPa. The addition of Si to TiN induces a hardness increase to a maximum of 41.8±2.0 GPa for a Si content close to x=0.14. Further increase in the Si content results in a small hardness reduction. The hardness of the as-deposited TiN film is in the same order as for other arc-evaporated TiN [9,32], but significantly higher than monolithic TiN(001) of 20 GPa [33]. The difference to the single-crystal material is attributed to defect hardening from the high density of lattice point defects common to arc evaporation as discussed in [35]. This is also expressed here in the compressive stress state of the films. The hardness enhancement for the as-deposited films with 0.01≤x≤0.09 can be explained by a combination of several hardening mechanisms as solid solution, grain size, point defects (residual stresses). Solid solution hardening originating from atomic and elastic modulus mismatch is explained in the Fleischer model [34]. A smaller grain size induces hardening according to the Hall-Petch relation [35,36] and point defects impede dislocation movements by inducing local lattice distortions. Any thermally induce strain between WC-Co and the film (TiN) would yield tensile stress in the order or ~1 GPa for a deposition temperature of 500 °C [37]. The film with x=0.14 exhibits all above hardening mechanisms as well as coherency strain hardening from the 19 phase separation into a two-phase structure. The films with Si-content x>0.14 possess slightly lower hardness than 41.8 GPa because of weakening of the grain boundaries due to thickening of the SiNz:Ti phase as the Si content increase. Formation and thickening of the a-SiNz phase above a few monolayers is known to decrease the hardness due to amorphization and lost coherency as seen in for instance [4] for nanocomposites and [6,7] for nanolaminates. After annealing at 1000 °C for 2 h the hardness for TiN decreases to 23.5±1.5 GPa. This decrease is commonly reported in literature, e.g., [28], and consistent with the XRD diffractograms and stress results presented above, and again, is an effect of defect annihilation and stress relaxation. The films with Si content 0.04≤x≤0.09, however, retain the hardness at 30.2±1.6 GPa and 38.8±2.0 GPa, respectively. This implies that the SiNz phase segregated to the grain boundary constitutes a strong coherent interface with the grains. Furthermore, the hardness drops to <28 GPa for films with x≥0.14 (in the asdeposited state),. This is due to recrystallization within in the cubic state due to Si and N out-diffusion as well as Co and W interdiffusion from the substrate as observed by EDXSTEM and ERDA. It can be assumed that these elements possibly together with O form tissue phases, including CoSi2, TiO2 or SiO2, which together with the decrease in residual stress weaken the structure. Phase stability of the films on thermally more stable substrates In order to clarify whether the observed Si and N losses at temperatures above 900 °C for films with an as-deposited Si content of x≥0.14 are inherent, or induced by the WC-Co interdiffusion, more temperature stable substrates have to be employed. Furthermore, 20 thermally more stable substrates are required also for the high temperatures needed to study any additional phase transformations for the solid solution films with 0.01≤x≤0.09. We use both sintered polycrystalline c-BN, a commonly used substrate in metal cutting applications, and Ta plates. Table III presents the compositions measured by ERDA of the as-deposited films on cBN substrates and their composition after isothermal annealing at 1000 °C, 1100 °C, and 1200 °C. The as-deposited films on c-BN substrate have a (Ti0.83Si0.17)N0.9 composition. The films on c-BN substrate were stable up to 1000 °C. At 1100 °C, however, Si and N out-diffusion and desorption took place, which changed the composition to (Ti0.85Si0.15)N0.85. When annealed at 1200 °C, the film content changed drastically with an up-take of 11.4 at.% C. The source for this C is the binding phase of TiC in the substrate. Hence, the c-BN substrates offered effective stability of 1100 °C, which is up to 200 °C more than for the WC-Co substrate, but the interdiffusion of C hinders the assessment on the inherent stability of the film. The two films investigated on Ta substrate have the compositions of (Ti0.91Si0.09)N1.04 and (Ti0.81Si0.19)N1.13 as measured by ERDA (see Table III) to. The Si content in the (Ti0.91Si0.09)N1.04 film on Ta substrate is sustained up to 1000 °C. At 1100 °C, however, local Si and N out-diffusion via the grain boundaries and eventual desorption is initiated, which cause a composition changes to (Ti0.92Si0.08)N. This process of Si and N is enhanced at 1200 °C and the remaining film consists of (Ti0.98Si0.02)N. 21 The (Ti0.81Si0.19)N1.13 film on Ta substrate is compositionally stable up to 1000 °C, at 1100 °C Si and N out-diffusion occurs resulting in a, (Ti0.??Si0.??)Ny composition. At 1200 °C the Si depletion is more or less complete and only ?? at.% remain. Error! Reference source not found. displays a cross-sectional TEM from the asdeposited (Ti0.83Si0.17)N0.9 film on c-BN substrate, which exhibits a dense, very defectrich segregated two-phase structure. Error! Reference source not found.(b) shows the XTEM image from the area close to the free surface of the same film annealed at 1100 °C for 2 h for which no substrate interdiffusion was observed in ERDA. The film volume closest to the free surface (see Error! Reference source not found.(b)), however, has locally recrystallized into ~10-50 nm grains that are elongated along the substrate normal. XTEM analysis of the 1200 °C-film on c-BN substrate (not shown) reveals that the film has recrystallized throughout its thickness to grain sizes of >100 nm. Moreover, the grains are facetted, typical for a relaxed, annealed structure. Error! Reference source not found. (observera att figurordningen mellan 12 och 11(ce) ska ändras) shows a STEM image together with EDX elemental maps of the (Ti0.83Si0.17)N0.9 film on c-BN substrate annealed at 1100 °C. The Si depleted grains appear with a dark contrast in the STEM micrograph in Error! Reference source not found.(a). The maps display that the structure has recrystallized due to Si out-diffusion. At this annealing temperature also segregation of Si within the film is present into Si-rich precipitate as shown in Error! Reference source not found.(b-d). 22 Error! Reference source not found.(c) displays the as-deposited (Ti0.81Si0.19)N1.13 film on Ta substrate. It reveals a dense, very defect-rich segregated two-phase feather-like structure, similar to the (Ti0.81Si0.19)N1.13 film deposited on WC-Co, c.f., Error! Reference source not found.(a). Error! Reference source not found.(d and e) shows bright-field (d) and dark-field (e) XTEM images from the (Ti0.81Si0.19)N1.13 film on Ta substrate annealed at 1200 °C. The microstructure has recrystallized from the feather-like two-phase structure into a nanocrystalline structure with nm-sized polyhedral grains elongated in the film growth direction. The film consists essentially of TiN any O Manfred?? as revealed by ERDA. The bright contrast at the grain boundaries in (d) indicates the presence of a porous structure, which is a consequence from the outdiffusion of Si and N. As a result, Ti and Si have diffused into the Ta substrate and formed a 1-µm-thick Ta-Si layer as revealed by EDX-STEM. Within this layer, Ti has together with O from the substrate constitute TiO2 precipitates, which appear as bright regions in the Ta-Si layer in Error! Reference source not found.(d). In-between the TaSi layer and the film, there is a ~100 nm broad recrystallized TiN band. The film thickness has decreased from 2.0 µm to 1.5 µm during annealing at 1200 °C because of the diffusion of Ti, Si, and N from the film into the substrate. The hardness of the films on c-BN substrates measured with nanoindentation is shown in Error! Reference source not found.. As-deposited films had hardness a of 39.5±2.1 GPa. In difference to the film annealed on WC-Co substrate, the hardness was retained at 1000 °C. At 1100 °C the hardness was slightly reduced to 38.6±2.3 GPa, as a consequence of the Si depletion confined mainly close to the film surface. At 1200 °C the 23 hardness has dropped to 15.8±1.5 GPa because of a fully recrystallized, porous structure strongly influenced by interdiffusion of mainly C from the TiC binder phase. Conclusions (Ti1-xSix)Ny films with 0≤x≤0.20 were deposited by arc-evaporation onto WC-Co substrates. As-deposited films with 0.01≤x≤0.09 exhibit a dense, defect-rich, polycrystalline, metastable (Ti1-xSix)Ny solid solution with a lattice parameter of ~4.24 Å. For x≥0.14, the films attain a <002> fiber-textured two-phase structure, which consists of defect-rich Ti-rich c-(Ti,Si)N crystallites and Si-rich a-SiNz:Ti. The N-content increased close to linear with increasing Si content from y=0.99 to y=1.13. The nanoindentation hardness increased from 30 GPa for TiN to 42 GPa for x=0.14. For higher Si contents, the hardness was reduced slightly to 38 GPa due to formation amorphous SiNz:Ti phase. We propose that Si exists in the films in four different forms: A) Si is substituted for Ti in the NaCl-type lattice in octahedral coordination. B) Si point defects of induced by the metal ion-bombardment generates tetrahedrally coordinated SiNz defect clusters. C) Crystalline SiNz grain boundary phase which forms a coherent interface with (Ti,Si)N grains. 24 D) Amorphous SiNz grain boundary phase, which is semi or incoherently bonded to the environment. XPS analysis could, however, not reveal any significant distinction between the different forms of Si coordinations. As a reference investigation, TiN/SiNx superlattice with cSiNx epitaxially stabilized between TiN(001) layers did not reveal any clear peak shifts of the Si2p peak compared to the as-deposited films. Isothermal annealing experiments of the solid solution films with x≤0.09 in the asdeposited state result in a defect annihilation process and an inherent thermodynamically driven segregation of type B Si to the grain boundaries to form a coherent x-ray amorphous SiNz grain boundary phase (type C) with thickness of a few monolayers. The SiNz phase effectively inhibits diffusion across grains, which limits further recrystallization as well as stress relaxation. As additional Si reach the grain boundary, the SiNz phase thickens and eventually amorphize (type D). At ~1100 °C, out-diffusion of amorphous Si and N is initiated. Similar annealing experiments were performed on the two-phase films with x≥0.14 and result in recrystallization into polyhedral grains and increased Si-N confinement to the grain boundaries. These films are compositionally stable up to 1000 °C, before local Si depletion occurs which consequently result in residual porous grain boundary structures. Finally, nanoindentation experiments reveal that the hardness of 38 GPa for the x=0.09 film on WC-Co substrates is retained at 1000 °C as a result of the recrystallization and 25 formation of the strong coherent interface phase of SiNz. For x≥0.14, W and Co interdiffusion decrease the hardness to <28 GPa, due to formations of weaker grain boundary phases. The nanoindentation hardness of (Ti0.83Si0.17)N0.9 on sintered c-BN substrates was despite the local Si and N out-diffusion at 1100 °C almost retained at ~3840 GPa. Acknowledgements The Swedish Research Council (VR) and the Swedish Foundation for Strategic Research (SSF) MS2E program are acknowledged for financial support. Jens Jensen (Tandem Laboratory), Urban Wiklund, and Mattias Lindquist at Uppsala University are acknowledged for assistance with ERDA measurements and nanoindentation, respectively. Mats P. Johansson at Seco Tools AB is acknowledged for the residual stress measurements and preparation of one the FIB TEM specimens. Björn Alling at Linköping University is acknowledged for fruitful theoretical discussion. Hans Söderberg at Swerea Kimab AB (earlier at Luleå University of Technology) is acknowledged for providing the c-TiN/SiNx multilayer sample. References 26 Table I. Elemental composition of the as-deposited films on WC-Co substrates as measured with ERDA. The values are obtained from averaging over the measured depth profiles (~100-300 nm), and have been normalized to 100 at.%. Before annealing Sample Ti Si N O C Others (at.%) (at.%) (at.%) (at.%) (at.%) (at.%) 1 49.34 0.12 49.20 0.45 0.77 0.12 2 49.33 0.64 48.86 0.56 0.51 0.1 3 47.07 1.86 49.96 0.60 0.38 0.13 4 44.12 4.20 50.69 0.43 0.42 0.14 5 40.84 6.52 51.42 0.59 0.51 0.12 6 39.36 7.33 52.08 0.65 0.44 0.14 7 38.46 8.25 52.08 0.70 0.41 0.1 8 37.33 9.14 52.26 0.76 0.41 0.1 9 37.29 9.02 52.26 0.81 0.52 0.1 Composition TiN0.99 (Ti0.99Si0.01)N0.98 (Ti0.96Si0.04)N1.02 (Ti0.91Si0.09)N1.04 (Ti0.86Si0.14)N1.09 (Ti0.84Si0.16)N1.12 (Ti0.92Si0.18)N1.11 (Ti0.80Si0.20)N1.12 (Ti0.81Si0.19)N1.13 Table II. Elemental composition of the post annealed films at 1000 °C on WC-Co substrates as measured with ERDA. The values are obtained from averaging over the measured depth profiles (~100-300 nm), and have been normalized to 100 at.%. After annealing Sample Ti Si N O C Co W Composition (at.%) (at.%) (at.%) (at.%) (at.%) (at.%) (at.%) 1 52.84 0.17 45.55 0.46 0.97 0.00 0.00 TiN0.86 2 51.68 0.58 46.60 0.45 0.68 0.00 0.00 (Ti0.99Si0.01)N0.89 3 48.11 1.80 47.80 0.77 1.23 0.00 0.00 (Ti0.96Si0.04)N0.96 4 45.27 4.10 48.26 0.95 1.20 0.00 0.00 (Ti0.92Si0.08)N0.98 5 43.22 4.65 48.23 0.66 0.83 2.06 0.34 (Ti0.90Si0.10)N:(Co,W) 6 42.56 5.07 45.34 0.87 0.42 5.18 0.55 (Ti0.89Si0.11)N:(Co,W) 7 40.04 4.62 44.61 0.87 1.33 7.75 0.77 (Ti0.90Si0.10)N:(Co,W) 8 38.95 5.39 44.08 0.98 0.95 8.86 0.67 (Ti0.88Si0.12)N:(Co,W) 9 42.77 3.46 43.32 0.68 1.08 6.81 1.78 (Ti0.93Si0.07)N:(Co,W) Table III. Elemental composition of the as-deposited and post annealed films at 1000 °C, 1100 °C, and 1200 °C on c-BN and Ta substrates, respectively, as measured with ERDA. 27 The values are obtained from averaging over the measured depth profiles (~100-300 nm), and have been normalized to 100 at.%. c-BN substr. as-dep. 1000°C 1100°C 1200°C Ta substr. as-dep. 1000°C 1100°C 1200°C Ta substr. as-dep. 1000°C 1100°C 1* 1100°C 2* 1200°C Ti (at.%) 43.5 43.2 45.4 51.1 Ti (at.%) 43.1 42.6 42.9 48.3 Ti (at.%) 36.9 37.2 42.8 39.8 45.9 Si (at.%) 8.6 9.0 7.9 3.2 Si (at.%) 5.0 4.9 3.2 1.8 Si (at.%) 9.3 9.2 1.4 7.8 1.2 N (at.%) 47.3 47.0 45.5 34.0 N (at.%) 50.5 49.9 46.2 44.1 N (at.%) 52.3 52.0 41.1 50.4 37.7 C (at.%) 0.6 0.7 1.4 11.4 C (at.%) 0.5 1.8 6.5 4.1 C (at.%) 0.4 0.7 11.6 1.8 12.8 O (at.%) O (at.%) 0.8 0.8 1.0 1.6 O (at.%) 1.0 0.9 3.0 0.2 2.4 others (at.%) others (at.%) 0.1 0.0 0.2 0.1 others (at.%) 0.1 0.0 0.1 0.0 0.0 Composition (Ti0.83Si0.17)N0.90 (Ti0.83Si0.17)N0.90 (Ti0.85Si0.15)N0.85 (Ti0.94Si0.06)N0.63 Composition (Ti0.90Si0.10)N1.05 (Ti0.90Si0.10)N1.05 (Ti0.93Si0.07)N1.00 (Ti0.96Si0.04)N0.88 Composition (Ti0.80Si0.20)N1.13 (Ti0.80Si0.20)N1.12 (Ti0.98Si0.02)N0.93 (Ti0.84Si0.16)N1.06 (Ti0.97Si0.03)N0.80 [1] P.H. 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