<?xml version="1.0" encoding="UTF-8"?><!DOCTYPE article  PUBLIC "-//NLM//DTD Journal Publishing DTD v3.0 20080202//EN" "http://dtd.nlm.nih.gov/publishing/3.0/journalpublishing3.dtd"><article xmlns:mml="http://www.w3.org/1998/Math/MathML" xmlns:xlink="http://www.w3.org/1999/xlink" dtd-version="3.0" xml:lang="en" article-type="research article"><front><journal-meta><journal-id journal-id-type="publisher-id">MSCE</journal-id><journal-title-group><journal-title>Journal of Materials Science and Chemical Engineering</journal-title></journal-title-group><issn pub-type="epub">2327-6045</issn><publisher><publisher-name>Scientific Research Publishing</publisher-name></publisher></journal-meta><article-meta><article-id pub-id-type="doi">10.4236/msce.2018.65001</article-id><article-id pub-id-type="publisher-id">MSCE-84813</article-id><article-categories><subj-group subj-group-type="heading"><subject>Articles</subject></subj-group><subj-group subj-group-type="Discipline-v2"><subject>Chemistry&amp;Materials Science</subject></subj-group></article-categories><title-group><article-title>
 
 
  Effect of Annealing Temperature and Atmosphere to Surface Solid Phase Reaction of Sapphire Substrates and Spin-Coated Copper Nitrate Gel Films
 
</article-title></title-group><contrib-group><contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Takashi</surname><given-names>Ehara</given-names></name><xref ref-type="aff" rid="aff1"><sub>1</sub></xref><xref ref-type="corresp" rid="cor1"><sup>*</sup></xref></contrib></contrib-group><aff id="aff1"><label>1</label><addr-line>Faculty of Human Studies, Ishinomaki Senshu University, Ishinomaki, Japan</addr-line></aff><author-notes><corresp id="cor1">* E-mail:<email>ehara@isenshu-u.ac.jp</email></corresp></author-notes><pub-date pub-type="epub"><day>24</day><month>05</month><year>2018</year></pub-date><volume>06</volume><issue>05</issue><fpage>1</fpage><lpage>10</lpage><history><date date-type="received"><day>11,</day>	<month>April</month>	<year>2018</year></date><date date-type="rev-recd"><day>22,</day>	<month>May</month>	<year>2018</year>	</date><date date-type="accepted"><day>25,</day>	<month>May</month>	<year>2018</year></date></history><permissions><copyright-statement>&#169; Copyright  2014 by authors and Scientific Research Publishing Inc. </copyright-statement><copyright-year>2014</copyright-year><license><license-p>This work is licensed under the Creative Commons Attribution International License (CC BY). http://creativecommons.org/licenses/by/4.0/</license-p></license></permissions><abstract><p>
 
 
  The solid-phase reaction of sapphire (Al
  <sub>2</sub>O
  <sub>3</sub>) substrates and spin-coated copper nitrate films was studied. X-ray diffraction analysis revealed that a CuO fraction was observed by annealing at temperatures higher than 800℃. In addition, crystalline CuAlO
  <sub>2</sub> was formed at annealing temperatures in the range of 900
  ℃ – 1000℃ by solid-phase reaction of the spin-coated films and sapphire substrate. Crystalline CuAlO
  <sub>2</sub> was formed by annealing at 1000℃ for 5 - 10 h, and CuAl
  <sub>2</sub>O
  <sub>4</sub> was formed by annealing at 1000℃ for 15 h. When annealing under N
  <sub>2</sub> flow, Cu
  <sub>2</sub>O was observed rather than CuAlO
  <sub>2</sub>. For a sample annealed in air at 1000℃ for 5 h, X-ray photoelectron spectroscopy measurements at various depths from surface revealed that Cu
  <sup>2+</sup> ions are located around the surface, which suggests that the CuO fraction is present near the surface while the CuAlO
  <sub>2</sub> fraction is located at greater depths from the surface of the samples. The depth profile of the sample suggests that there is no pure CuAlO
  <sub>2</sub> layer in the sample, but that crystalline CuAlO
  <sub>2</sub> is present in the sample as a mixture with CuO and Al
  <sub>2</sub>O
  <sub>3</sub>.
 
</p></abstract><kwd-group><kwd>Solid-Phase Reaction</kwd><kwd> Sapphire Substrate</kwd><kwd> CuAlO&lt;sub&gt;2&lt;/sub&gt;</kwd><kwd> CuO</kwd><kwd> X-Ray Dif-fraction</kwd><kwd> X-Ray Photoelectron Spectroscopy</kwd></kwd-group></article-meta></front><body><sec id="s1"><title>1. Introduction</title><p>Cu-delafossite, which comprises ternary metal oxide materials with a structure of CuMO<sub>2</sub> (M = Al, Ga, In, Sc, Y, La, Cr, Fe, etc.) has gathered much interest due to their potential in various applications, such as wide gap semiconductors [<xref ref-type="bibr" rid="scirp.84813-ref1">1</xref>] [<xref ref-type="bibr" rid="scirp.84813-ref2">2</xref>] [<xref ref-type="bibr" rid="scirp.84813-ref3">3</xref>] , catalysts [<xref ref-type="bibr" rid="scirp.84813-ref4">4</xref>] [<xref ref-type="bibr" rid="scirp.84813-ref5">5</xref>] or sensors [<xref ref-type="bibr" rid="scirp.84813-ref6">6</xref>] . Among the Cu-delafossite materials, CuAlO<sub>2</sub> is considered a promising candidate as a p-type transparent conductive oxide (TCO) [<xref ref-type="bibr" rid="scirp.84813-ref1">1</xref>] . Some TCO materials, such as indium tin oxide [<xref ref-type="bibr" rid="scirp.84813-ref7">7</xref>] or aluminum-doped zinc oxide [<xref ref-type="bibr" rid="scirp.84813-ref8">8</xref>] , have already been studied and applied in optoelectronic devices. However, most TCOs have n-type conductivity, so that TCO materials with p-type conductivity have been in demand to prepare transparent pn junctions. The properties of CuAlO<sub>2</sub> as a p-type TCO have been reported, such as an optical bandgap of 3.5 eV and conductivity of 1 Ω cm [<xref ref-type="bibr" rid="scirp.84813-ref1">1</xref>] . CuAlO<sub>2</sub> thin films have been prepared by various methods, including pulsed laser deposition [<xref ref-type="bibr" rid="scirp.84813-ref1">1</xref>] [<xref ref-type="bibr" rid="scirp.84813-ref9">9</xref>] [<xref ref-type="bibr" rid="scirp.84813-ref10">10</xref>] , sputtering [<xref ref-type="bibr" rid="scirp.84813-ref11">11</xref>] [<xref ref-type="bibr" rid="scirp.84813-ref12">12</xref>] [<xref ref-type="bibr" rid="scirp.84813-ref13">13</xref>] [<xref ref-type="bibr" rid="scirp.84813-ref14">14</xref>] , chemical vapor deposition [<xref ref-type="bibr" rid="scirp.84813-ref15">15</xref>] [<xref ref-type="bibr" rid="scirp.84813-ref16">16</xref>] , solid-phase reaction of Al<sub>2</sub>O<sub>3</sub>, sapphire substrate, and Cu<sub>2</sub>O thin layers [<xref ref-type="bibr" rid="scirp.84813-ref17">17</xref>] [<xref ref-type="bibr" rid="scirp.84813-ref18">18</xref>] , chemical spray pyrolysis [<xref ref-type="bibr" rid="scirp.84813-ref19">19</xref>] , and the sol-gel method [<xref ref-type="bibr" rid="scirp.84813-ref20">20</xref>] [<xref ref-type="bibr" rid="scirp.84813-ref21">21</xref>] [<xref ref-type="bibr" rid="scirp.84813-ref22">22</xref>] [<xref ref-type="bibr" rid="scirp.84813-ref24">24</xref>] . Among these preparation methods, the solid-phase reaction of sapphire substrate and Cu<sub>2</sub>O is interesting because the CuAlO<sub>2</sub> layer formed on the surface of the sapphire substrate can act as a transparent electrode with strong adhesion to the sapphire substrate. On the other hand, the sol-gel method has been studied extensively as a method for the preparation of CuAlO<sub>2</sub> thin films. In the studies of sol-gel preparation, various aluminum source materials have been used, such as aluminum acetate [<xref ref-type="bibr" rid="scirp.84813-ref20">20</xref>] , aluminum ethoxide [<xref ref-type="bibr" rid="scirp.84813-ref21">21</xref>] , aluminum nitrate [<xref ref-type="bibr" rid="scirp.84813-ref22">22</xref>] [<xref ref-type="bibr" rid="scirp.84813-ref23">23</xref>] , or alumatrane [<xref ref-type="bibr" rid="scirp.84813-ref24">24</xref>] . In addition, some of those aluminum sources do not have an exact molecular weight due to hydration water. On the other hand, the preparation of copper oxide by sol-gel method has been well established. CuO or Cu<sub>2</sub>O thin films have been successfully prepared using the sol-gel method [<xref ref-type="bibr" rid="scirp.84813-ref25">25</xref>] [<xref ref-type="bibr" rid="scirp.84813-ref26">26</xref>] . The sol-gel films become CuO or Cu<sub>2</sub>O thin films depending on the annealing temperature or annealing atmosphere. Films annealed under nitrogen flow at temperatures higher than 900˚C generally become Cu<sub>2</sub>O thin films, whereas CuO films are formed by annealing in air at lower temperatures [<xref ref-type="bibr" rid="scirp.84813-ref25">25</xref>] .</p><p>In the present work, CuAlO<sub>2</sub> layers were prepared on the surface of sapphire substrates by solid-phase reaction of the sapphire substrate with spin-coated copper nitrate thin films. This method makes it possible to form a CuAlO<sub>2</sub> layer on the surface of sapphire substrate without the need for complicated vacuum equipment.</p></sec><sec id="s2"><title>2. Experimental</title><p>A copper source solution was prepared by dissolving 2.42 g of copper(II) nitrate trihydrate in 25 mL of 2-methoxyethanol. The solution was stirred for 24 h to produce a light blue and homogenous solution. The solution was spin-coated onto a c-oriented single-side-polished sapphire substrate with a thickness of 0.5 mm. Before spin-coating of the copper source solution, the sapphire substrates were degreased by ultrasonication in EtOH. Spin-coating was performed at 3000 rpm for 10 s. The coated films were first heated at 200˚C for 10 min in air, and then again at a higher temperature of 500˚C for 20 min using a hot-plate as the heating device. Spin-coating and subsequent heat treatment procedures were repeated 6 times to obtain a gel film with a thickness of 0.2 μm. The prepared samples were annealed at temperatures in the range of 800˚C - 1100˚C for 10 h in air or under nitrogen flow. In another experiment, the samples were annealed at 1000˚C for 2, 5, 10 and 15 h in air. The temperature was increased from room temperature to the specific temperature over a period of 3 h, held at the specific temperature for 10 h, and then cooled to room temperature over a period of more than 3 h.</p><p>The structural properties of the films were analyzed using X-ray diffraction (XRD; D8 Discover, Bruker) in θ - 2θ mode with Cu Kα radiation. A Ni filter with a thickness of 0.12 mm was used to avoid observation of the signal due to CuKβ radiation. The atomic compositions of the samples, including depth profiles, were measured using X-ray photoelectron spectroscopy (XPS; JPS-9010MC, JEOL) with Mg Kα radiation. Depth profiles of the samples were measured by etching with Ar sputtering. The etch rate of the sapphire substrate with Ar sputtering was determined to be 10 nm/min. The atomic compositions were determined using a sapphire substrate as a standard sample for the Al/O ratio. The Cu/Al ratios were determined using CuAlO<sub>2</sub> films prepared by the sol-gel method as a standard sample using Cu and Al nitrates as metal sources.</p></sec><sec id="s3"><title>3. Results and Discussion</title><p><xref ref-type="fig" rid="fig1">Figure 1</xref> shows XRD patterns of the sapphire substrate with spin-coated copper nitrate films annealed at various temperatures (a) in air and (b) under nitrogen flow. For annealing in air at 800˚C or 900˚C, only peaks of CuO are observed. The CuO (110), (002)(-111) and (111) peaks are observed at 32.5˚, 35.5˚, and 38.7˚, respectively (PDF 00-045-0937). However, the samples annealed at 1000˚C showed the (006) peak of CuAlO<sub>2</sub> at 31.6˚ (PDF 00-035-1401) in addition to the peaks of CuO. At an annealing temperature of 1100˚C, all the CuAlO<sub>2</sub> and CuO peaks disappeared, which is considered to be due to evaporation of the spin-coated copper nitrate film at high temperature before oxidation or reaction with the sapphire substrate could occur. The samples annealed under nitrogen flow showed different results. As shown in <xref ref-type="fig" rid="fig1">Figure 1</xref>(b), a peak of Cu<sub>2</sub>O was observed at 36.3˚ (PDF 00-005-0667) in addition to the peaks of CuO at annealing temperatures higher than 900˚C. The intensity of the Cu<sub>2</sub>O peak increased with the annealing temperature up to 1000˚C, which is consistent with a previous study on films of CuO and Cu<sub>2</sub>O prepared by the sol-gel route on SiO<sub>2</sub> substrates [<xref ref-type="bibr" rid="scirp.84813-ref25">25</xref>] . At an annealing temperature of 1000˚C, a CuAlO<sub>2</sub> peak was observed at 31.7˚, as was the case for the samples annealed in air; however, the intensity was very weak and the peak width was broadened.</p><p>The results indicate that the crystalline CuAlO<sub>2</sub> in the sample has a small volume ratio and small crystallite size. At an annealing temperature of 1100˚C, no peaks were observed, similar to the samples annealed in air. <xref ref-type="fig" rid="fig2">Figure 2</xref> shows wide angle range XRD patterns of the samples annealed in air or under nitrogen flow</p><p>at 1000˚C to compare the effect of the annealing atmosphere. For the sample annealed in air, peaks of CuAlO<sub>2</sub> were observed at 15.6˚ (003), 31.6˚ (006), and 48.3˚ (009). However, no peaks beside the c-axis oriented CuAlO<sub>2</sub> peaks were observed, which indicates that the CuAlO<sub>2</sub> in the samples is highly c-axis oriented. In contrast, the sample annealed under nitrogen flow shows only one (006) peak for CuAlO<sub>2</sub> at 31.6˚. These results indicate that annealing in air is more preferable than annealing under N<sub>2</sub> flow to form CuAlO<sub>2</sub> by solid-phase reaction between a spin-coated copper nitrate film and sapphire substrate. In the case of solid phase reaction of powders, the CuAlO<sub>2</sub> formation reaction under nitrogen flow is preferable than in the air.</p><p>At the temperature of 1000˚C, copper oxide takes form of Cu<sub>2</sub>O, even if the atmosphere includes oxygen gas. Thus, CuAlO<sub>2</sub> is formed by the solid-phase reaction shown in (1) as well as in the case of solid phase reaction of powders [<xref ref-type="bibr" rid="scirp.84813-ref14">14</xref>] .</p><p>Cu 2 O + Al 2 O 3 → 2CuAlO 2 (1)</p><p>However, the solid phase reaction in the present work is accompanied by diffusion of oxygen and copper into sapphire substrate. In the annealing under nitrogen flow, it is considered that the supply of oxygen to the reaction interface is not sufficient and the formation of CuAlO<sub>2</sub> stops at a specific depth. As a result, the formation reaction of CuAlO<sub>2</sub> by the annealing in air becomes rather preferable than that under nitrogen flow.</p><p>In the XRD patterns of the samples annealed in air, no peaks of Cu<sub>2</sub>O are observed, although Cu<sub>2</sub>O is required to the solid phase reaction to form CuAlO<sub>2</sub>. It is because the Cu<sub>2</sub>O which exist at the temperature of 1000˚C is oxidized to CuO by air at lower temperature during the temperature decreasing process in the annealing.</p><p>Cu 2 O + 1 / 2O 2 → CuO (2)</p><p>As a result, XRD patterns show peaks of only CuAlO<sub>2</sub> and CuO.</p><p><xref ref-type="fig" rid="fig3">Figure 3</xref> shows XRD patterns of samples annealed at 1000˚C in air for various times. The sample annealed for 2 h showed only peaks due to CuO. In contrast, after annealing the sample for 5 h, XRD peaks of CuAlO<sub>2</sub> were observed with peaks of CuO. After annealing of 10 h, both CuAlO<sub>2</sub> and CuO peaks were observed, as with the sample annealed for 5 h. The intensity of both the CuAlO<sub>2</sub> peaks increased with annealing time from 5 h to 10 h. In the sample annealed at 1000˚C for 15 h, a different XRD pattern from the sample annealed for 10 h was observed. The sample does not show either CuO or CuAlO<sub>2</sub> peaks, but instead peaks of CuAl<sub>2</sub>O<sub>4</sub> are observed at 31.3˚ (220) and 36.9˚ (311) (PDF 00-033-0448). These results suggest that CuAlO<sub>2</sub> reacts with the sapphire substrate:</p><p>2CuAlO 2 + Al 2 O 3 + O → 2CuAl 2 O 4 (3)</p><p>No specific annealing time was determined when the sample produced only the CuAlO<sub>2</sub> crystalline phase. The sample annealed for more than 20 h showed no copper related XRD peaks. This is considered to be due to the further diffusion of Cu atoms into the sapphire substrate. This suggests that the samples annealed for more than 20 h become copper-doped sapphire substrates, whereby only XRD peaks of crystalline Al<sub>2</sub>O<sub>3</sub> are observed.</p><p><xref ref-type="fig" rid="fig4">Figure 4</xref> shows an XPS spectrum for the surface of the sample annealed at 1000˚C for 5 h. Peaks of Cu 2p, O 1s, and Al 2p are observed at binding energies of and 930 - 955 eV, 531.2 eV, and 74.4 eV, respectively. Peaks at binding energies of 745, 766, and 780 eV are ascribed to Auger electrons (O KLL). Cu 2p has</p><p>two peaks at 933.4 eV and 953.2 eV, which are assigned to Cu 2p<sub>3/2</sub> and Cu 2p<sub>1/2</sub>, respectively. The peak positions observed in <xref ref-type="fig" rid="fig4">Figure 4</xref> are shifted from those for CuAlO<sub>2</sub> or CuO reported previously [<xref ref-type="bibr" rid="scirp.84813-ref27">27</xref>] [<xref ref-type="bibr" rid="scirp.84813-ref28">28</xref>] because the sample in the present work contains not only CuAlO<sub>2</sub> and CuO, but also Cu-doped Al<sub>2</sub>O<sub>3</sub>.</p><p><xref ref-type="fig" rid="fig5">Figure 5</xref> shows depth profile of the atomic concentrations for the sample annealed at 1000˚C for 5 h. The atomic concentration of copper is 25% at the surface, which then decreases monotonically with increasing depth from the surface and becomes 0% at a depth of 450 nm. XRD measurements showed the sample contains not only crystalline CuAlO<sub>2</sub> but also crystalline CuO; therefore, the sample is considered to consist of both of CuAlO<sub>2</sub> and CuO fractions or layers embedded in the Al<sub>2</sub>O<sub>3</sub> substrate. The XRD patterns of the sample measured after etching of the surface to 500 nm showed no copper related peaks.</p><p><xref ref-type="fig" rid="fig6">Figure 6</xref> shows XPS of Cu 2p, O 1s, and Al 2p spectra at various depths from</p><p>the surface. XPS peaks of Cu 2p, i.e., Cu 2p<sub>3/2</sub> at a binding energy of 933.5 eV and Cu 2p<sub>1/2</sub> peaks at 953.2 eV, are observed with a decrease in peak intensity with an increase in the depth from the surface. In addition, a weak and broad signal is also observed at a binding energy of 944 eV, which is assigned as a satellite peak that has been reported as a shake-up signal of Cu<sup>2+</sup> [<xref ref-type="bibr" rid="scirp.84813-ref27">27</xref>] . It has been reported that the shake-up signal has not been observed in the case of Cu<sup>+</sup>, because of multiplet splitting of the signal [<xref ref-type="bibr" rid="scirp.84813-ref29">29</xref>] . The relative intensity of the signal at the surface is significantly weaker than that for pure CuO reported previously [<xref ref-type="bibr" rid="scirp.84813-ref30">30</xref>] , which suggests that both Cu<sup>2+</sup> and Cu<sup>+</sup> are present at the surface, so that both CuO and CuAlO<sub>2</sub> are present at the surface. The relative intensity of the satellite peak to the peak at 933 eV is dependent on the depth from the surface. The shake-up signal is clearly observed in the spectra measured at the surface and at a depth of 50 nm. However, the satellite peak is not observed clearly at depths greater than 150 nm, which indicates that Cu<sup>2+</sup> is present mainly around the surface. Therefore, CuO is present at surface, while CuAlO<sub>2</sub> is present at greater depths from the surface. In the case of the XPS O 1s and Al 2p peaks shown in <xref ref-type="fig" rid="fig6">Figure 6</xref>, the dependence of the binding energy on the depth from surface was observed as a peak shift. At the surface, the O 1s peak is observed at a binding energy of 531.2 eV, which is then is shifted to 531.5 eV at a depth of 200 nm from the surface. The XPS Al 2p peak at surface is observed at 74.4 eV, which is then shifted to 74.7 eV at a depth of 200 nm from the surface. However, the peak shift is not significant, with the shift of binding energy at only 0.3 eV for both the O 1s and Al 2p peaks.</p></sec><sec id="s4"><title>4. Conclusion</title><p>The solid-phase reaction of sapphire substrate and spin-coated copper nitrate thin films by thermal annealing was studied. XRD analysis revealed that both CuO and CuAlO<sub>2</sub> fractions were formed at an annealing temperature of 1000˚C for annealing times of 5 h or 10 h. The formation of CuO is due to oxidation of the spin-coated copper nitrate gel film by the sol-gel route reaction. In contrast, the formation of CuAlO<sub>2</sub> is evidence for the occurrence of a solid-phase reaction. XPS measurements revealed that CuO is present around the surface, while the CuAlO<sub>2</sub> fraction is located at greater depths from the surface.</p></sec><sec id="s5"><title>Acknowledgements</title><p>This work was financially supported by Ishinomaki Senshu University Kyoso Kenkyu Josei.</p></sec><sec id="s6"><title>Cite this paper</title><p>Ehara, T. (2018) Effect of Annealing Temperature and Atmosphere to Surface Solid Phase Reaction of Sapphire Substrates and Spin-Coated Copper Nitrate Gel Films. 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