3.1. As-Fabricated NiO Films
Figure 3 shows the SEM images of the NiO films with different oxygen flow rates. All the films were dense and homogeneous and had smooth surfaces. The SEM results shown in
Figure 3 reveal no clear differences. Before the RTA treatment, the NiO thin films deposited via sputtering did not achieve sufficient crystal growth owing to the fact that the sputtered atoms did not have enough energy to carry out crystal growth. Thus, XRD measurements were used to investigate the details of the crystallographic properties.
Figure 4 shows a homogeneous surface morphology independent of the oxygen flow rate obtained via AFM with a scan area of 1 × 1 μm
2. The root-mean-square (RMS), which was used to evaluate the roughness of the surface, increased from 1.694 to 15.506 nm. When the oxygen flow rate increased, the surface roughness presented an uptrend because the oxygen content in the chamber influenced the deposited thin film during sputtering. The interstitial oxygen in the NiO film was applied as a point defect. The more defects in a film, the lower its crystallinity. This means that the interfacial contact between NiO and another material will deteriorate. However,
Figure 4d depicts a lower RMS, 2.616 nm, than the other samples without 0 sccm. This result either shows that the NiO film fabricated with 4 sccm had excellent roughness or reflects an error in measurement.
The theoretical stoichiometry of the NiO films presented XRD peaks (JCPDS card no. 01-1239) of (111), (200), (220), (311), and (222) [
29]. The NiO film deposited using a flow rate of 0 sccm was strongly associated with the (111), (200), and (220) peaks and weakly associated with the (311) and (222) peaks. As the oxygen flow ratio was increased to 2 sccm, all the peak intensities decreased. Upon a further increase to 10 sccm, the XRD pattern of the NiO film showed very weak peaks. This decrease in the peak intensity indicates the low crystallinity of the film. Thus, we can conclude that the interstitial oxygen causes a decrease in the crystallinity of the NiO film because interstitial oxygen is a point defect [
30] on NiO films. Point defects, such as interstitial anions and cation vacancies, result in lattice mismatches and reduce crystallinity or crystallographic properties. NiO film which has stoichiometry composition is NaCl crystal structure. The interstitial oxygen introduced via an excessive oxygen flow rate influences the change from a NaCl crystal structure to an amorphous structure. This means that to attain a crystalline NiO film, the oxygen flow rate must be controlled. Additionally, the lattice constant and 2θ are related through Bragg’s law [
31]
where d is the distance between successive layers of atoms, and n is the diffraction order.
Here, a is the lattice constant, and h and k are the Miller indices.
Table 3 lists the calculated crystallographic parameters of the NiO films. XRD peaks were not observed in the NiO film deposited via RF sputtering with a 10 sccm oxygen flow.
Table 3 shows the increase in the lattice constant. The theoretical lattice constant of NiO is 4.1678 Å [
32], which is in agreement with the result regarding the NiO film deposited at an oxygen flow rate of 0 sccm. When the oxygen flow rate was gradually increased, the lattice constant also increased because of the expansion of the lattice due to the presence of interstitial oxygen. According to Bragg’s law, the 2θ and lattice constant exhibit a trade-off relationship. The values in
Table 3, calculated using various equations, may differ from the actual values. In general, a low FWHM and a large D indicate the coincidence of peaks, sharp peak intensity, and high crystallinity. However, the values in
Table 3 do not correspond to the crystallinity shown in the XRD pattern in
Figure 5 because the calculated FWHM and D are influenced by the lattice structure, peak intensity, and shape. Therefore, a decrease in the peak intensity or a change in the peak shape can reduce the calculated FWHM. Moreover, the increase in the lattice constant indicates lattice expansion, which leads to a large D.
Figure 6 shows the change in transmittance with oxygen content during the sputtering process. The transmittance of the NiO film is clearly influenced by the oxygen flow rate. When the oxygen flow rate increases from 0 to 10 sccm, the transmittance of the NiO film changes from 65% to 40% because the Ni
3+ ions strongly absorb in the visible region [
33]. In addition, the optical bandgap energy E
g and strain ε can be calculated using the following equations [
34]:
Here, α is the absorption coefficient, hv is the photon energy, and A is a constant.
Above, a is the measured lattice parameter, and a0 (0.41678 nm) is the theoretical lattice parameter of the NiO film.
The E
g values of the NiO films fabricated under various conditions are listed in
Table 4. The E
g was calculated as 3.69 eV at 0 sccm and 3.57 eV at 10 sccm. The theoretical band gap energy of nickel oxide is 3.6–4.0 eV [
7], which is in agreement with
Figure 7. When the oxygen flow rate was increased, the E
g decreased. Therefore, the oxygen content of the NiO film affects the E
g. The reduction in the E
g can be attributed to various interactions between ions and carriers [
35]. In addition, films fabricated via various processes have residual stress due to lattice mismatch, impurities, and dislocation in the films. In this case, interstitial oxygen caused tensile stress through lattice expansion and reduced the E
g. The optical bandgap was narrowed for these reasons. The calculated strain exhibits a tendency that corresponds to the E
g, as shown in
Table 4. The calculation of film stress in addition to the measurement of film stress via glancing incident XRD (GIXRD) are shown in
Figure 8 and
Table 5.
Figure 8 shows a linear graph of epsilon vs. sin
2psi. The residual stress was calculated by considering elastic theory and diffraction theory in a sin
2psi system. The relationship between epsilon and sin
2psi is represented in the equation [
36] below
where ψ (shi) and φ (phi) are the polar and azimuthal angles. E = 181 Gpa (Young’s modulus) and v = 0.27 (Poisson’s ratio) are the constants for the NiO film during the residual stress measurements. σ
φ is the measured stress component in the φ direction.
Stress in a thin film is caused by applied stress (an externally applied load) and residual stress (stress existing in a thin film in the absence of an applied force). Applied stress, which is structural stress, arises through lattice mismatch and growth defects, and residual stress is typically caused during formation or heating. The tensile and compressive stresses are the residual stresses existing in a material without the application of an external load. The presence of tensile and compressive stress can be confirmed by referring to the slope of the graph. The six fitted lines have a negative slope, which indicates compressive stress. Thin films deposited via expansion and plasma during the sputtering process are subjected to compressive stress due to their tendency to return to their origin state. Thus, the NiO films deposited with interstitial oxygen exhibited signs of compressive stress. The compressive stress values range from −857.2 to −1604.0 MPa in
Table 5, in which the highest stress was indicated by the 2 sccm sample and the lowest stress was observed for the 6 sccm sample. This means that high crystallinity does not result in low stress owing to the lattice mismatch between the NiO film and the glass substrate. Compressive stress can change the physical properties of a thin film, leading to peeling via hillock formation and wrinkling. To manufacture stable devices, residual stress must be reduced.
As shown in
Figure 9, as the oxygen flow rate increased, the carrier concentration and resistivity of the NiO films improved, while their mobility decreased. The relationship between the oxygen content and Ni
3+ ions can be represented in the equation [
37] below
where Ni
vancancy is the ionized nickel vacancy.
Figure 9a–c show the carrier concentration, the resistivity, and the mobility of the NiO film, respectively. In the above equation, Ni
2+ is replaced by two Ni
3+ ions with Ni
vacancy to achieve electrical neutrality of the NiO film. Therefore, the oxygen-rich conditions during the sputtering process resulted in more Ni
3+ ions. Ni
vacancy generates a hole carrier, which is the reason behind the p-type characteristics observed, and causes an increase in carrier concentration. In
Figure 9b, the NiO film deposited with 0 sccm exhibited a higher resistivity than the other samples because the stoichiometric NiO film is a Mott–Hubbard insulator [
38]. As the oxygen flow rate increased, resistivity rapidly decreased because of an increase in the carrier concentration.
Figure 9c shows that the carrier mobility of the NiO films is influenced by the oxygen flow rate. The NiO films deposited under oxygen-rich conditions exhibited low carrier mobility. Interstitial oxygen can interrupt carrier movement because of impurity scattering. The higher the carrier concentration, the more impurity scattering that occurs among the hole carriers. Moreover, lattice expansion causes lattice imperfections, which can interrupt the carrier movement. Thus, carrier concentration and carrier mobility exhibit a trade-off relationship.
The NiO films affect the oxygen flow rate during the deposition process. To apply the various fields, the NiO films require the control of properties. As the oxygen flow rate increased, crystallinity, optical properties, and mobility decreased, and the carrier concentration increased. The stoichiometric composition of the NiO film reveals its excellent optical and crystallographic properties. However, its excessive resistivity close to an insulator makes it difficult to apply in devices. Thus, the NiO films must have interstitial oxygen, which induces a high carrier concentration. To obtain a NiO film with a high carrier concentration and excellent crystallinity, RTA gas conditions were considered. The RTA under O2 condition was predicted to prevent the evaporation of oxygen via heat.
Before studying the effect of RTA gas conditions, it is important to account for the RTA temperature, which is an important parameter that affects the properties of NiO films. To evaluate the effect of RTA temperature, the samples deposited at 0, 2, 4, 6, 8, and 10 sccm oxygen flow rates were annealed via RTA at 100, 200, 300, 400, and 500 °C, respectively. The atoms in the film thermally vibrated at low temperatures in circles during the thermal treatment. The samples processed at 100 and 200 °C showed no significant changes. However, when the temperature was increased, the atoms provided sufficient energy and moved from the film lattice to the air because sufficient energy around the atoms can overcome the binding system of the film. In the NiO film, the Ni-O binding energy was higher than the interstitial oxygen binding energy. Therefore, the samples processed at 400 and 500 °C showed similar properties to those of the sample fabricated at a 0 sccm oxygen flow rate in
Table 6 and
Table 7. This indicates that oxygen on the NiO film evaporated at high temperatures. Thus, the optimal temperature for investigating the effect of the atmosphere was 300 °C.
3.2. NiO Film Annealed at 300 °C RTA under Ar, O2, and N2 Atmospheres
The samples were then annealed at 300 °C via RTA under Ar, O2, and N2 atmospheres, respectively. To prevent the reduction in the oxygen content in the NiO films through the RTA process, the effect of the RTA atmosphere was intensively investigated in terms of its electrical, optical, and crystallographic properties.
Figure 10a–c show the carrier concentration, the resistivity, and the mobility of the NiO film by RTA on the NiO films under different atmospheres. After annealing the NiO films, the carrier concentration decreased, and the resistivity increased. This is because oxygen atoms were transferred from the NiO film to air via the RTA process. Interstitial oxygen in the lattice of NiO caused the formation of Ni
3+ ions, which are hole carriers. In contrast, carrier mobility was improved. This was due to the reduction in point defects and carrier concentration. The impurity scattering on the films was influenced by the carrier concentration. In particular, the carrier mobility was maximally improved under an O
2 atmosphere. However, the carrier concentration was not a higher value than that under other conditions. This means that mobility was affected by not only the carrier concentration but other parameters such as crystallinity. The low carrier mobility, which is a disadvantage of p-type oxide semiconductors, can be improved via the RTA process under an O
2 atmosphere compared to other atmospheres.
Figure 11a–c show an improvement in transmittance of the NiO film after carrying out the 300 °C RTA process under different atmosphere. This indicates a reduction in the number of Ni
3+ ions in the NiO film. The samples processed via RTA under Ar and N
2 atmospheres slightly increased the transmittance. On the other hand, the samples processed via RTA under an O
2 atmosphere significantly improved transmittance compared with those processed under other conditions. The transmittance of the NiO films was influenced by various conditions as well as the presence of Ni
3+ ions. This suggests that there are various ways to improve optical properties.
Table 8 and
Figure 12a–f show that the optical band gaps of the samples increased after annealing, except for 0 sccm. This is because of the reduction in electrostatic attraction between electrons in the valence band and holes in the conduction band due to the carrier concentration. Moreover, the RTA process can be associated with improved crystallographic properties and a reduction in point defects, with the latter being interstitial oxygen and lattice imperfections. In addition, tensile stress decreased after the RTA process, while the optical band gap increased. The optical band gap energy of the NiO film processed under an O
2 atmosphere showed a tendency of having a higher energy value than it did under other atmospheres.
The NiO films annealed at 300 °C were investigated for their effect on the oxygen flow rate and gas conditions. The samples deposited with 0, 2, 4, 6, 8, and 10 sccm oxygen flows showed electrical and optical properties. All the samples exhibited improved transmittance, optical bandgaps, and mobility. To evaluate the NiO films under RTA conditions in greater detail, three oxygen flow rates were selected. Among these samples numbered the 0 sccm sample, which had the stoichiometric composition of an NiO film; the 4 sccm sample, with higher carrier mobility than the other samples; and the 8 sccm sample, which had a higher carrier concentration than the other samples, while the 10 sccm was excluded; the samples XRD peaks are shown in
Figure 4.
Figure 13 shows the clearly different surfaces of the NiO films compared with the samples before the RTA process. Before applying the RTA process, the samples had low crystallinity owing to the presence of interstitial oxygen. Thermal treatment led to the evaporation of interstitial oxygen in the NiO film, halting lattice expansion and improving the crystallinity of the NiO film. The SEM images show grain boundaries and large grains compared to those of the as-fabricated samples. XRD was used to evaluate the crystallinity of the NiO films.
In
Figure 14, the peak of the XRD pattern is slightly sharpened because the RTA process induced an improvement in the crystallinity of the NiO film. Moreover, the peaks shifted to the right compared to the samples before the RTA process as shown by
Table 9. This peak shift is related to the lattice constant according to Bragg’s law. This means that lattice expansion caused by interstitial oxygen was resolved, and the RTA process reduced the interstitial oxygen in the NiO film. The corresponding results are shown in
Table 10. The value of strain indicates whether the strain turned into either compressive stress (ε < 0) or tensile stress (ε > 0). The strain applied to the thin film by interstitial oxygen was reduced compared to that before RTA process. Thus, the strain applied to the thin film can be reduced via the RTA process. The NiO films annealed under Ar gas showed lower strain values. This might have been due to the oxygen content.
The properties of the NiO films were mostly affected by the oxygen content. The effect of the RTA atmosphere was slightly different under the Ar, O2, and N2 conditions. The atomic compositions of the NiO films were measured to evaluate the specific effects of the gas conditions during the RTA process. The atomic composition of the NiO film fabricated with an 8 sccm oxygen flow rate and processed via the RTA process was investigated via XPS measurement because the sample fabricated with an 8 sccm oxygen flow rate had a higher carrier concentration, indicating higher oxygen and Ni3+ ion content, and was expected to show a clear difference in atomic composition before and after RTA.
XPS measurements were performed using the following parameter: spot size: 400 μm, pass energy: 200 eV, and step size: 1.0 eV. The XPS binding energy of all the samples was aligned by reference [
39,
40]. The sample work function was calculated as the sum of the electron affinity (the value in the literature was 1.46 eV) and the optical bandgap energy (which, in this study, was 8 sccm and 3.61 eV) [
41]. The C 1s peak position was calculated as follows: BE = 289.58 − Φ
SA (5.07 eV) = 284.51 eV. Thus, all peaks were shifted by taking the difference of the measured BE (284.8 eV) and the calculated BE.
Figure 15 shows the XPS survey spectra (
Figure 15a) and the NiO peaks of the XPS system, such as the Ni 2p and O 1s spectra (
Figure 15b–i). As shown in the images, the Ni 2p
1/2 represented two peaks Ni
2+ at ~872 eV and a satellite at ~878 eV. The Ni 2p
3/2 showed Ni
2+ at ~853 eV, Ni
3+ at ~855 eV, and a satellite at ~861 eV. In the O 1s spectrum, only two peaks were exhibited: Ni
2+ at ~529 eV and Ni
3+ at ~531 eV. The binding energy of the NiO film was not influenced by the RTA process because the peak shift caused a change in the oxidation number and the bonding of other atoms. The Ni 2p
1/2 peak at ~872 eV and O 1s peak at ~529 eV related to the Ni–O octahedral bonding of cubic NiO correspond to the lattice oxygen and Ni
2+ because the lattice oxygen exists as O
2- in NiO films [
42]. The Ni 2p
3/2 peak at ~855 eV and O 1s peak at ~531 eV correspond to Ni
3+. The Ni
3+ was present because of the interstitial oxygen and nickel vacancy, as shown in Formula (5), or due to the excess oxygen from NiOOH owing to exposure and the pollution. The peak intensity of the XPS measurement system is proportional to the amount of material on the surface. The Ni 2p peak intensity indicates that there were more Ni
2+ ions than Ni
3+ ions in all the samples. This means that the presence of Ni
3+ ions, which was very high, affected the properties of NiO films. The atomic compositions of the NiO films are shown in
Table 11, and the as-fabricated sample exhibited the highest oxygen content. After the RTA process, the sample processed in an O
2 atmosphere showed a higher oxygen content in Ar and N
2 atmospheres. In terms of preventing oxygen content in the NiO film during the RTA process, O
2 atmosphere is an optimal condition compared to Ar and N
2 gas.