<?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">JCPT</journal-id><journal-title-group><journal-title>Journal of Crystallization Process and Technology</journal-title></journal-title-group><issn pub-type="epub">2161-7678</issn><publisher><publisher-name>Scientific Research Publishing</publisher-name></publisher></journal-meta><article-meta><article-id pub-id-type="doi">10.4236/jcpt.2014.44023</article-id><article-id pub-id-type="publisher-id">JCPT-50286</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>
 
 
  Low Pressure Chemical Vapor Deposition of TiO&lt;sub&gt;2&lt;/sub&gt; Layer in Hydrogen-Ambient
 
</article-title></title-group><contrib-group><contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>atoshi</surname><given-names>Yamauchi</given-names></name><xref ref-type="aff" rid="aff1"><sup>1</sup></xref><xref ref-type="corresp" rid="cor1"><sup>*</sup></xref></contrib><contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Kazuhiro</surname><given-names>Ishibashi</given-names></name><xref ref-type="aff" rid="aff1"><sup>1</sup></xref></contrib><contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Sakura</surname><given-names>Hatakeyama</given-names></name><xref ref-type="aff" rid="aff1"><sup>1</sup></xref></contrib></contrib-group><aff id="aff1"><addr-line>Department of Biomolecular Functional Engineering, Ibaraki University, Hitachi, Japan</addr-line></aff><author-notes><corresp id="cor1">* E-mail:<email>ysatoshi@mx.ibaraki.ac.jp(AY)</email>;</corresp></author-notes><pub-date pub-type="epub"><day>06</day><month>10</month><year>2014</year></pub-date><volume>04</volume><issue>04</issue><fpage>185</fpage><lpage>192</lpage><history><date date-type="received"><day>25</day>	<month>July</month>	<year>2014</year></date><date date-type="rev-recd"><day>22</day>	<month>August</month>	<year>2014</year>	</date><date date-type="accepted"><day>16</day>	<month>September</month>	<year>2014</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>
 
 
  Low pressure chemical vapor deposition (LPCVD) of anatase TiO
  <sub>2</sub> as a reduction gas was demonstrated at pres- sure of 3 mtorr in comparison to that using TTIP and O
  <sub>2</sub> with study for the property of the layers. Dissociation energy of TTIP in H
  <sub>2</sub> was higher than that in O
  <sub>2</sub> but resistivity of the layer deposited in H
  <sub>2</sub> was significantly decreased to 0.2 Ω cm in contrast to the high resistivity beyond 100 Ω cm of the layer deposited in O
  <sub>2</sub>. UV-Vis optical transmission spectra showed absorption around 2.2 eV was increased in the layer deposited by TTIP + H
  <sub>2</sub> in addition to decrease of forbidden energy gap due to increase of Urbach tail. Resistivity at low temperature below 100 K indicating the layer deposited in H
  <sub>2</sub>-ambient was degenerated by the high electron density but the resistivity was decreased with temperature above 100 K with the activation energy about 100 meV. A possible electronic conduction model based on kernel, grain boundary and surface trap to clarify the temperature dependent resistivity suggesting resistivity of the layer was limited by depletion region in the grain-boundary extended from the surface and the kernel with significantly low resistivity in 10
  <sup>-3</sup> Ω cm order was formed in the layer.
 
</p></abstract><kwd-group><kwd>LPCVD</kwd><kwd> TTIP+H&lt;sub&gt;2&lt;/sub&gt;</kwd><kwd> Anatase-TiO&lt;sub&gt;2&lt;/sub&gt;</kwd><kwd> Low Resistive TiO&lt;sub&gt;2&lt;/sub&gt;</kwd></kwd-group></article-meta></front><body><sec id="s1"><title>1. Introduction</title><p>TiO<sub>2</sub> has been extensively investigated in view of photo-induced applications using the photo-catalytic reactions and the hydrophilicity [<xref ref-type="bibr" rid="scirp.50286-ref1">1</xref>] [<xref ref-type="bibr" rid="scirp.50286-ref2">2</xref>] in addition to dielectric applications using the high dielectric constant and optoelectronic applications by the high refractive index [<xref ref-type="bibr" rid="scirp.50286-ref3">3</xref>] [<xref ref-type="bibr" rid="scirp.50286-ref4">4</xref>] . On the other hand, the material has been also expected</p><p>for transparent conduction oxide (TCO) because of the wide band gap of 3.2 eV. In addition, the conductive TiO<sub>2</sub> with significantly high resistance in acid and alkaline solutions has interesting potentials to fabricate solar-cells, chemical sensors etc. However, it is easily recognized that the conductivity control is more difficult than the other TCO such as ITO, Sn<sub>2</sub>O and ZnO since d-orbital contributes to forming TiO<sub>2</sub>. Recently, laser-ab- lation and reactive sputtering with the post-annealing in reduction ambient have been applied to form highly conductive TiO<sub>2</sub> layer by using Nb as a donor-dopant [<xref ref-type="bibr" rid="scirp.50286-ref5">5</xref>] [<xref ref-type="bibr" rid="scirp.50286-ref6">6</xref>] . In such process, oxygen-deficiency is seemed to be required to enhance the electronic activation of the donor [<xref ref-type="bibr" rid="scirp.50286-ref7">7</xref>] , in which Ti<sup>3+</sup> reduced from Ti<sup>4+</sup> probably plays an important role of the conduction in TiO<sub>2</sub>. On the other hand, chemical vapor deposition (CVD) which is able to form thin film with step coverage better than that by physical vapor deposition has been studied on TiO<sub>2</sub> fabrication. In the CVD process, suitable primary-source is fundamentally required in addition to control of the deposition condition. It has been well recognized that titanium-tetra-iso-propoxide (TTIP: Ti(O-i-C<sub>3</sub>H<sub>7</sub>)<sub>4</sub>) is a suitable metalorganic precursor for the TiO<sub>2</sub> deposition and the thermally dissociated species is crystallized in the anatase-phase around 400˚C [<xref ref-type="bibr" rid="scirp.50286-ref8">8</xref>] . However, few studies have been reported for the conductivity control of TiO<sub>2</sub> layer by CVD. Also in the CVD process, it can be believed that Ti<sup>3+</sup> in TiO<sub>2</sub> layer plays an important role for the conductivity. Previously, we demonstrated low pressure chemical vapor deposition (LPCVD) of TiO<sub>2</sub> layer using TTIP + O<sub>2</sub> and Nb-F co-doping by using the dopant of NbF<sub>5</sub>, in which the resistivity was decreased to 0.2 Ω cm by the doping in contrast to high resistivity of the undoped layer beyond 100 Ω cm [<xref ref-type="bibr" rid="scirp.50286-ref9">9</xref>] . Further, XPS study showed that F substituted to the O-site contributes to the reduction of resistivity, which can be recognized; the F reduced Ti<sup>4+</sup> to Ti<sup>3+</sup> and Ti<sup>3+</sup> supports the activation of Nb-donor, but oxygen-vacancy increases the resistivity. These results are qualitatively in agreement with the results of molecular orbital calculations [<xref ref-type="bibr" rid="scirp.50286-ref9">9</xref>] , in which the donor level due to 6-fold-coordinated Ti<sup>3+</sup> is shallower than that of Ti<sup>3+</sup> associated with oxygen-va- cancy. These results indicate that Ti<sup>3+</sup> ions or the complex defects are essentially required to control in the density and the nature for increase of the conductivity.</p><p>In this paper, LPCVD of TiO<sub>2</sub> layer using TTIP and reduction gas of H<sub>2</sub> is demonstrated to increase Ti<sup>3+</sup> density and control the conductivity. The deposited layer is characterized by X-ray diffraction, UV-Vis transparent spectroscopy and the temperature dependent resistivity.</p></sec><sec id="s2"><title>2. Experimental</title><sec id="s2_1"><title>2.1. LPCVD of TiO<sub>2</sub> Layer</title><p>A bell-jar type reactor with the base pressure under 1 &#215; 10<sup>−</sup><sup>5</sup> torr by a combination of diffusion pump and a rotary pump was used for LPCVD of titanium-oxide. Titanium tetra-iso-propoxide (TTIP, Ti(O-i-C<sub>3</sub>H<sub>7</sub>)<sub>4</sub>: 99.7% purity) was used as source gas after purification in vacuum. Details of the apparatus configuration and the purification sequence of TTIP were already shown elsewhere [<xref ref-type="bibr" rid="scirp.50286-ref9">9</xref>] . High purity hydrogen gas (99.99999%) was simultaneously introduced into the reactor through an individual gas inlet during the deposition. In the case of the deposition in O<sub>2</sub>, high purity oxygen gas (99.9999%) instead of H<sub>2</sub> was introduced into the reactor. The gas sup- ply ratio of TTIP/H<sub>2</sub> or TTIP/O<sub>2</sub> were controlled by monitoring the reactor pressure using Shultz gage when TTIP and H<sub>2</sub> or O<sub>2</sub> were introduced into the reactor, in which sensitivity of the ion gage for H<sub>2</sub> and O<sub>2</sub> was taken into account to determine the gas supply ratio to TTIP. Substrate of 1 mm-thick quartz plate with optically flat surface was mounted on a substrate holder after chemical cleaning. Temperature of the substrate holder on resistive heater was monitored by K-type thermo-couple and controlled by PID-system.</p></sec><sec id="s2_2"><title>2.2. Evaluation of LCVD-TiO<sub>2</sub> Layer</title><p>Thickness of the layer was checked by a surface profiler (Veeco, DEKTAK150). Resistivity was evaluated by Van Der Pauw (VDP) method using symmetric four ohmic contacts of Indium-dots, in which the temperature was varied from 10 to 300 K in vacuum and dark by a cryogenic system (Janis Research, CCS-150). Crystallographic behavior was examined by θ - 2θ X-ray diffraction (RIGAKU: RAD-C) using CuK<sub>α</sub>. UV-Vis optical transmission spectra were obtained by UV-Vis spectrometer (OCEAN OPTICS: USB-2000) using a light source of Halogen lamp.</p></sec></sec><sec id="s3"><title>3. Results and Discussions</title><sec id="s3_1"><title>3.1. Deposition Rate and Resistivity of TiO<sub>2</sub> Layer</title><p><xref ref-type="fig" rid="fig1">Figure 1</xref>(a) shows Arrhenius plot of TiO<sub>2</sub> deposition rate in O<sub>2</sub> (open-circle) and H<sub>2</sub> (solid-circle) ambient for the deposition temperature, in which supply rate of the gas to TTIP was kept at 1. The deposition rate of the layer deposited in O<sub>2</sub> (TiO<sub>2</sub>/O<sub>2</sub>) and in H<sub>2</sub> (TiO<sub>2</sub>/H<sub>2</sub>) was increased with the temperature and then saturated above 360˚C. At such low temperatures, the layers were poly-crystallized into anatase-phase as shown by XRD spectra in <xref ref-type="fig" rid="fig1">Figure 1</xref>(b), in which the spectra of TiO<sub>2</sub>/O<sub>2</sub> and TiO<sub>2</sub>/H<sub>2</sub> deposited at 360˚C is shown by black-line and red-line respectively. In the both spectra, diffraction peaks originated from (101) and (200) anatase-TiO<sub>2</sub> were observed but not any peaks due to another phase such as rutile and brookite. The diffraction peak intensities of the TiO<sub>2</sub>/H<sub>2</sub> layer were weaker than that of the TiO<sub>2</sub>/O<sub>2</sub> layer but the peak angle shift was not observed in the spectrum. Activation energy of 138 kJ/mol for the deposition of TiO<sub>2</sub>/O<sub>2</sub> obtained the result in <xref ref-type="fig" rid="fig1">Figure 1</xref>(a) showed that TTIP-dissociation feature was scarcely influenced by O<sub>2</sub> because the energy was similar to CVD by TTIP single precursor [<xref ref-type="bibr" rid="scirp.50286-ref10">10</xref>] . In this case, it can be recognized TTIP is thermally dissociated then anatase-TiO<sub>2</sub> is formed with propene and isopropanol at such low temperatures as follow reaction [<xref ref-type="bibr" rid="scirp.50286-ref11">11</xref>] .</p><p><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/2-1010123x6.png" xlink:type="simple"/></inline-formula>,</p><p>where it is expected Ti=O bonds are formed on the deposition surface [<xref ref-type="bibr" rid="scirp.50286-ref12">12</xref>] . Further, it is considered the surface Ti=O bonds act as adsorption-site of the precursor and enhance the dissociation of TTIP as depicted in <xref ref-type="fig" rid="fig2">Figure 2</xref>(a). In contrast, the activation energy for TiO<sub>2</sub>/H<sub>2</sub> was obtained as 230 kJ/mol. Previously, Shmakov et al. demonstrated quantum chemical calculations using B3LYP for monomolecular dissociation of TTIP and suggested</p><fig-group id="fig1"><label><xref ref-type="fig" rid="fig1">Figure 1</xref></label><caption><title> (a) Deposition rate in O<sub>2</sub> (open-circle) and H<sub>2</sub> (solid-circle) for the temperature and (b) typical θ - 2θ XRD spectra of 200 nm-thick TiO<sub>2</sub> layer deposited at 360˚C in O<sub>2</sub> (black-line) and H<sub>2</sub> (red-line), where the miller indicate shows anatase-TiO<sub>2</sub> surface.</title></caption><fig id ="fig1_1"><label> (b)</label><graphic mimetype="image"   position="float"  xlink:type="simple"  xlink:href="http://html.scirp.org/file/2-1010123x7.png"/></fig><fig id ="fig1_2"><label></label><graphic mimetype="image"   position="float"  xlink:type="simple"  xlink:href="http://html.scirp.org/file/2-1010123x8.png"/></fig></fig-group><fig-group id="fig2"><label><xref ref-type="fig" rid="fig2">Figure 2</xref></label><caption><title> Expected scheme of TTIP-dissociation on deposition surface (a) without (b) with hydrogen contribution. Blue-bowline in (b) shows thermal dissociation of monomolecular TTIP.</title></caption><fig id ="fig2_1"><label>(b)</label><graphic mimetype="image"   position="float"  xlink:type="simple"  xlink:href="http://html.scirp.org/file/2-1010123x9.png"/></fig><fig id ="fig2_2"><label></label><graphic mimetype="image"   position="float"  xlink:type="simple"  xlink:href="http://html.scirp.org/file/2-1010123x10.png"/></fig></fig-group><p>the activation barrier to form Ti(OC<sub>3</sub>H<sub>7</sub>)<sub>3</sub>(OH) and propene via O-H-CH<sub>2</sub> interaction in isopropyl group of TTIP is 56.9 kcal/mol (238 kJ/mol) [<xref ref-type="bibr" rid="scirp.50286-ref13">13</xref>] . The calculated value is in good agreement with the activation energy for the deposition TiO<sub>2</sub>/H<sub>2</sub>, however, very high as compared to that for TiO<sub>2</sub>/O<sub>2</sub> and the previous report using TTIP single precursor. It can be recognized the large different of the activation energy is owing to hydrogen at the deposition surface as shown in <xref ref-type="fig" rid="fig2">Figure 2</xref>(b). When H<sub>2</sub> gas is simultaneously supplied with TTIP, methyl-group of TTIP cannot be allowed in the reaction to Ti-O or Ti on the deposition surface, because the surface consists of Ti=O is terminated by hydrogen. Therefore, the adsorption of the precursor is achieved after monomolecular dissociation to form Ti(OC<sub>3</sub>H<sub>7</sub>)<sub>3</sub>(OH), then the adsorbed species is dissociated to TiO<sub>x</sub>. It is noted Ti-H is probably remained in the deposited layer and the hydrogen is partially desorbed by thermal dissociation. In the scheme of the hydrogen-desorption, it is expected Ti<sup>4+</sup> is reduced to Ti<sup>3+</sup> and resulted in generation of donor- defect. <xref ref-type="fig" rid="fig3">Figure 3</xref> shows dependence of resistivity of TiO<sub>2</sub>/H<sub>2</sub> on the deposition temperature, in which the layers were deposited with the thickness about 200 nm and the resistivity was evaluated by VDP method at room- temperature. Although all of TiO<sub>2</sub>/O<sub>2</sub> layer was with high resistivity above 100 Ω cm beyond the evaluation limit of our system, resistivity of the TiO<sub>2</sub>/H<sub>2</sub> layer deposited in H<sub>2</sub> was decreased with the deposition temperature and then gradually increased above 360˚C. The activation energy of 244 kJ/mol obtained below 350˚C suggested that donor concentration was increased with the temperature. Recently, it was reported that hydrogen acts as donor in TiO<sub>2</sub> by experimental results for anatase-TiO<sub>2</sub> powder (Degussa P25) treated by atomic-hydrogen [<xref ref-type="bibr" rid="scirp.50286-ref14">14</xref>] and molecular orbital theoretical results [<xref ref-type="bibr" rid="scirp.50286-ref15">15</xref>] , in which hydrogen was found to be bound to lattice oxygen in TiO<sub>2</sub>. In this work, it is however considered that the door species in the layer was not the hydrogen bound to O, because the absorption due to Ti-OH (Chemisorbed OH) which was identified in IR-spectrum of amorphous Ti- O<sub>x</sub> layer deposited by plasma-assisted deposition at room-temperature [<xref ref-type="bibr" rid="scirp.50286-ref16">16</xref>] could not be observed in the TiO<sub>2</sub>/H<sub>2</sub> layers. On the other, Nakamura et al. studied reduction treatment of anatase-TiO<sub>2</sub> powder by radio-frequency hydrogen-gas plasma at 400˚C to enhance the visible light activity for NO removal [<xref ref-type="bibr" rid="scirp.50286-ref17">17</xref>] . In the report, ECR spectra indicated the anatase-TiO<sub>2</sub> is reduced by hydrogen excited in the plasma and oxygen-vacancies are for- med with the double defect levels of 0.75 and 1.18 eV below the conduction band minimum. Although non-ex- cited hydrogen gas was supplied below 380˚C during the deposition in this work, it can be considered hydrogen was adsorbed to Ti as shown in <xref ref-type="fig" rid="fig3">Figure 3</xref> and maybe form oxygen-vacancies in the layer. However, the defect level is too deep to decrease the resistivity at room-temperature. Therefore, the defect to reduce the resistivity is not oxygen-vacancy but Ti<sup>3+</sup> with the defect level shallower than the complex centers predicted by theoretical calculations [<xref ref-type="bibr" rid="scirp.50286-ref15">15</xref>] . Indeed, the activation energy of 244 kJ/mol obtained by the result in <xref ref-type="fig" rid="fig3">Figure 3</xref> was similar to the dissociation energy of 208 kJ/mol for Ti-H bond [<xref ref-type="bibr" rid="scirp.50286-ref18">18</xref>] .</p></sec><sec id="s3_2"><title>3.2. Optical Absorption</title><p>Figures 4 shows optical absorption spectra in UV-Vis region. Dot-lines in <xref ref-type="fig" rid="fig4">Figure 4</xref>(a) show transmission spectra of TiO<sub>2</sub>/H<sub>2</sub> (red-line) and TiO<sub>2</sub>/O<sub>2</sub> (black-line) layers grown at 360˚C with the thickness about 200 nm. Gra- dual increase and relatively low value of optical transmittance in Vis-region suggested deep-level defects were included in the forbidden energy gap. The spectra were successfully deconvoluted into two-spectra with the peak at 2.2 eV and 3.0 eV, which were described by Gaussian-function, and near band edge absorption obtained after removal the two-spectra from the raw transmission spectrum. In <xref ref-type="fig" rid="fig4">Figure 4</xref>(a), the deconvoluted spectra and</p><fig id="fig3"  position="float"><label><xref ref-type="fig" rid="fig3">Figure 3</xref></label><caption><title> Resistivity of TiO<sub>2</sub>/H<sub>2</sub> for the deposition temperature, in which the layers were deposited with thickness about 200 nm</title></caption><graphic mimetype="image"   position="float"  xlink:type="simple"  xlink:href="http://html.scirp.org/file/2-1010123x11.png"/></fig><fig-group id="fig4"><label><xref ref-type="fig" rid="fig4">Figure 4</xref></label><caption><title> (a) Transmission spectra (dot-lines) and the deconvoluted spectra (solid-lines) with the fitting lines (blue-lines) of TiO<sub>2</sub>/O<sub>2</sub> (black-lines) and TiO<sub>2</sub>/H<sub>2</sub> (red-lines); (b) (αhν)<sup>1/2</sup> plots for photon energy with the linear relation line (dash-lines) to determine the optical band gap; and (c) absorption coefficient in near band edge region after removal the absorptions due to deep-levels centered at 2.2 eV and 3.0 eV.</title></caption><fig id ="fig4_1"><label> (b)</label><graphic mimetype="image"   position="float"  xlink:type="simple"  xlink:href="http://html.scirp.org/file/2-1010123x14.png"/></fig><fig id ="fig4_2"><label> (c)</label><graphic mimetype="image"   position="float"  xlink:type="simple"  xlink:href="http://html.scirp.org/file/2-1010123x13.png"/></fig><fig id ="fig4_3"><label></label><graphic mimetype="image"   position="float"  xlink:type="simple"  xlink:href="http://html.scirp.org/file/2-1010123x12.png"/></fig></fig-group><p>the fitting curves are shown by solid-line (red-line: TiO<sub>2</sub>/H<sub>2</sub>, black-line: TiO<sub>2</sub>/O<sub>2</sub>) and blue-lines, respectively. Previously, Sekiya et al. suggested the origin of absorption at 3.0 eV and in between 2.2 and 2.3 eV, which were coincident to peak energies of the deconvoluted spectra in <xref ref-type="fig" rid="fig4">Figure 4</xref>(a), is attributed to oxygen-vacancies with two-trapped electrons and electron transition of Ti<sup>3+</sup> from <sup>2</sup>T<sub>2</sub> to <sup>2</sup>E state contributed by crystal field interaction with surrounding oxygen, respectively [<xref ref-type="bibr" rid="scirp.50286-ref19">19</xref>] . They also showed intensity of the absorption in between 2.2 and 2.3 eV is decreased by post-annealing above 300˚C with decreasing electrical conductivity. In this work, the absorption peak at 2.2 eV was significantly increased in the intensity for TiO<sub>2</sub>/H<sub>2</sub> whereas the absorption peak at 3.0 eV was scarcely different as compared with TiO<sub>2</sub>/O<sub>2</sub>. From these results, it is considered that increase of Ti<sup>3+</sup> density in TiO<sub>2</sub>/H<sub>2</sub> was independent from the increase of oxygen-vacancy and resulted in the reduction of resistivity. It is noted significant broadening of the absorption around 2.2 eV was also observed for the TiO<sub>2</sub>/H<sub>2</sub> in comparison with TiO<sub>2</sub>/O<sub>2</sub> as shown in <xref ref-type="fig" rid="fig4">Figure 4</xref>(a), in which the full-with at half-maximum (FWHM) was 1.4 eV and 0.86 eV for the TiO<sub>2</sub>/H<sub>2</sub> and TiO<sub>2</sub>/O<sub>2</sub> respectively. The absorption broadening could be recognized crystal field around Ti<sup>3+</sup> was more fluctuated in the layer as compared with the TiO<sub>2</sub>/O<sub>2</sub>, that is, structural disordering of TiO<sub>2</sub>/H<sub>2</sub> was higher than that of TiO<sub>2</sub>/O<sub>2</sub>. Indeed, XRD spectra showed crystallinity of TiO<sub>2</sub>/H<sub>2</sub> was inferior to that of TiO<sub>2</sub>/O<sub>2</sub> as shown in <xref ref-type="fig" rid="fig1">Figure 1</xref>(b). Further, it has been reported structural disordering causes band gap narrowing in crystal. <xref ref-type="fig" rid="fig4">Figure 4</xref>(b) shows Tauc plot in (αhν)<sup>1/2</sup> vs. photon energy (hν) to determine the optical band gap of TiO<sub>2</sub>/H<sub>2</sub> (red-line) and TiO<sub>2</sub>/O<sub>2</sub> (black-line), where α is absorption coefficient. The band gap of 3.16 eV given by the extrapolated linear line (black dot-line) for the TiO<sub>2</sub>/O<sub>2</sub> was scarcely smaller than that of 3.2 eV for anatase-TiO<sub>2</sub>. In contrast, the band gap was significantly reduced to 3.0 eV for the TiO<sub>2</sub>/H<sub>2</sub>. The estimated band gap of 3.0 eV was similar to that for rutil-TiO<sub>2</sub> but the lowering of band gap could be considered to be originated from defect states in the band gap, because any XRD diffraction peak corresponding to rutile phase could not be observed in the layer. On the other, it has been recognized localized defect states originated from structural disordering are extended form an optical absorption tail to lower energy side below the band gap and resulted in origin of the optical band gap narrowing, in which the tail is referred as Urbach tail represented by α = α<sub>o</sub>exp(hν/E<sub>u</sub>) using Urbach energy (E<sub>u</sub>) [<xref ref-type="bibr" rid="scirp.50286-ref20">20</xref>] . <xref ref-type="fig" rid="fig4">Figure 4</xref>(c) shows absorption coefficient of the TiO<sub>2</sub>/H<sub>2</sub> (red- line) and TiO<sub>2</sub>/O<sub>2</sub> (black-line) in log-scale against photon energy, where two-absorption spectra centered at 2.2 eV and 3.0 eV were numerically removed. Urbach energy obtained by the linear relationship in log(α) vs. photon energy below band gap was 153 meV and 114 meV for the TiO<sub>2</sub>/H<sub>2</sub> and TiO<sub>2</sub>/O<sub>2</sub>, respectively. Previously, Choudhury et al. [<xref ref-type="bibr" rid="scirp.50286-ref21">21</xref>] reported the Urbach energy is dependent on anneal condition for sol-gel TiO<sub>2</sub>, and the energy of 140 meV for the anatase-TiO<sub>2</sub> annealed in vacuum and about 100 meV for anatase/rutile mixed TiO<sub>2</sub>. They concluded such increase of the Urbach energy is come from oxygen-vacancies or structural disordering at interface with different crystal phases. In this work, Urbach energy for the TiO<sub>2</sub>/H<sub>2</sub> was higher than that for the TiO<sub>2</sub>/O<sub>2</sub>, however, the density of oxygen-vacancy was similar for the both layers as shown by the absorption intensity around 3.0 eV in <xref ref-type="fig" rid="fig4">Figure 4</xref>(a). In contrast, from the result that the absorption around 2.2 eV was increased in the intensity for the TiO<sub>2</sub>/H<sub>2</sub>, it can be suggested not only the oxygen-vacancy but also the Ti<sup>3+</sup>-re- lated defects and/or the complexes contributed the band gap narrowing.</p></sec><sec id="s3_3"><title>3.3. Temperature Dependence of Resistivity</title><p><xref ref-type="fig" rid="fig5">Figure 5</xref>(a) shows dependence of resistivity evaluated by VDP method for TiO<sub>2</sub>/H<sub>2</sub> layer. The electrodes using Indium-dots were ohmic at overall temperatures as shown in <xref ref-type="fig" rid="fig5">Figure 5</xref>(b), in which the current-voltage characteristics at 10 K (open-circle) and 300 K (solid-circle) are plotted. The saturated feature at low temperature indicated the layer was degenerated by the high density of conduction electron originated from shallow donors. In contrast, the resistivity was exponentially decreased with increasing temperature above 100K in Arrhenius relationship with the activation energy of 96.1 meV. Since it is difficult to attribute the activation energy to donor-level energy below conduction-band minimum in the degenerated semiconductor, influence in the grain boundary region should be taken into account in the electric conduction of the layer. In the grain boundary region, it is easy to consider deep level defects are formed by significantly disordered structures. The defects in the boundary region trap the carriers or compensate the shallow donors. In the case that the carriers are traps in the deep defects, depletion region is introduced toward the kernel. Previously, Blom et al. presented a conduction model for poly-crystalline layer consists of kernels and grain-boundaries and applied the analysis for temperature dependent conduction of ZnO layer [<xref ref-type="bibr" rid="scirp.50286-ref22">22</xref>] . In the model, resistivity of the layer parallel to the substrate is limited by that of grain boundaries surrounding kernel, because Schottky barrier is formed by traps in the grain- boundary because the resistivity of kernel can be expected to be much lower than that of the boundary region. Since the density of thermally emitted carrier across the barrier is increased with temperature, resistivity of the layer is decreased with temperature and then saturated to the resistivity due to the kernels at high temperature. However, the model is insufficient to the result in this work because the resistivity was saturated at low temperature. On the other, in the case that the carrier density is significantly reduced by compensation of shallow donors in the boundary region, resistivity in the region is much higher than in the kernel and dependent on the temperature. The resistivity in grain-boundary region is expected to be decreased with temperature. In this case, although resistivity of the layer limited by the resistance in grain-boundary is saturated at low temperature and reduced with temperature, the activation energy experimentally obtained by the result of <xref ref-type="fig" rid="fig5">Figure 5</xref>(a) is too large to explain the result of temperature dependent resistivity. Here, it should be noted that defects at deep level are also formed at surface. When electrons are captured by the traps at the surface, depletion region is extended in the boundary region with low carrier density from the TiO<sub>2</sub> surface. The depletion length can be estimated by density of the trapped electron in the surface state (N<sub>sse</sub>) and effective donor density in the boundary region (N<sub>bd</sub>) in the relationship of N<sub>bd</sub>/N<sub>sse</sub>. The depletion region acts to cut off carrier transport across the boundary region and the depleted length is decreased with temperature due to activation of electrons captured the traps, which is resulted in decrease of the resistivity with temperature. Details based on the model including surface treatment of the layer are in progress, but the simulated result can explain well the temperature dependent resistivity as shown by solid-line in <xref ref-type="fig" rid="fig5">Figure 5</xref>(a). The result indicated N<sub>bd</sub>/N<sub>sse</sub>, peak energy of the surface trap below conduction band minimum, FWHM of surface trap distribution for electron energy and resistivity without the cut-off of electron transport in grain boundary is 1.8 &#215; 10<sup>−</sup><sup>5</sup>, 195 meV, 136 meV and 4.2 &#215; 10<sup>−</sup><sup>3</sup> Ω cm, respectively. The obtained parameters suggested resistivity of the kernel is much lower than the effective resistivity limited by the grain boundary.</p><fig-group id="fig5"><label><xref ref-type="fig" rid="fig5">Figure 5</xref></label><caption><title> (a) Arrhenius plot of resistivity for TiO<sub>2</sub>/H<sub>2</sub>, in which the resistivity was evaluated by VDP method and (b) I-V property of the layer at 10 K (open-circle) and 300 K (solid-circle).</title></caption><fig id ="fig5_1"><label> (b)</label><graphic mimetype="image"   position="float"  xlink:type="simple"  xlink:href="http://html.scirp.org/file/2-1010123x16.png"/></fig><fig id ="fig5_2"><label></label><graphic mimetype="image"   position="float"  xlink:type="simple"  xlink:href="http://html.scirp.org/file/2-1010123x15.png"/></fig></fig-group></sec></sec><sec id="s4"><title>4. Conclusion</title><p>Low pressure chemical vapor deposition of TiO<sub>2</sub> layer was performed in H<sub>2</sub>-ambient. The deposition rate and activation energy for the deposition were decreased and decreased as compared with the deposition in O<sub>2</sub>-am- bient. Crystallographic property of the layer deposited in H<sub>2</sub> was inferior to that in O<sub>2</sub> but the resistivity was drastically reduced by using H<sub>2</sub> during the deposition. Optical absorption around 2.2 eV was notably increased by the deposition in H<sub>2</sub> with scarce increase around 3.0 eV. These results and a possible dissociation scheme of TTIP on the deposition surface suggested that donor in the layer was originated from Ti<sup>3+</sup> and/or Ti<sup>3+</sup>-related complex, which was increased by hydrogen. Temperature dependent resistivity was also evaluated for the layer deposited in H<sub>2</sub>, in which the resistivity was saturated at low temperature region but decreased with temperature above 100 K. A possible model consisted of kernel, grain-boundary and surface trapped electrons was applied to clarify the conduction mechanism of the layer. As a result, the temperature dependent result could be well fitted by the model and showed that electron transport in the layer was limited by depletion region in the grain- boundary, Further, the obtained parameters indicated that the grain with the resistivity of 4 &#215; 10<sup>−</sup><sup>3</sup> Ω cm was formed with the surface traps around 200 meV below the conduction band minimum by the demonstrated deposition process, and the boundary and the surface engineering were fundamentally necessary to perform transparent conductive TiO<sub>2</sub> layer.</p></sec><sec id="s5"><title>NOTES</title></sec></body><back><ref-list><title>References</title><ref id="scirp.50286-ref1"><label>1</label><mixed-citation publication-type="other" xlink:type="simple">Wang, R., Hashimoto, K. and Fujishima, A. (1997) Light-Induced Amphiphilic Surfaces. 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