Active Site Considerations on the Photocatalytic H2 Evolution

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Active Site Considerations on the Photocatalytic H2 Evolution Performance of Cu-Doped TiO2 Obtained by Different Doping Methods Juan M. Valero, Sergio Obregón, and Gerardo Colon ACS Catal., Just Accepted Manuscript • DOI: 10.1021/cs500865y • Publication Date (Web): 15 Aug 2014 Downloaded from http://pubs.acs.org on August 17, 2014

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Active Site Considerations on the Photocatalytic H2 Evolution Performance of Cu-Doped TiO2 Obtained by Different Doping Methods Juan M. Valero, Sergio Obregón and Gerardo Colón* Instituto de Ciencia de Materiales de Sevilla. Centro Mixto Universidad de SevillaCSIC. Américo Vespucio s/n. 41092 Sevilla. Spain KEYWORDS: Cu-TiO2, photocatalysis, active site, sulfation, H2 evolution. ABSTRACT.

Photocatalytic H2 evolution reaction was performed over copper doped TiO2. The influence of sulfate pretreatment over fresh TiO2 support and the Cu doping method has been evaluated. Wide structural and surface characterisation of catalysts was carried out in order to establish a correlation between the effect of sulfuric acid treatment and the further Cu-TiO2 photocatalytic properties. Notably different copper dispersion and oxidation state is obtained by different metal decoration method. From the structural and surface analysis of the catalysts we have been stated that the occurrence of highly disperse and reducible Cu2+ species is directly related to the photocatalytic activity for

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H2 production reaction. Highly active materials have been obtained from chemical reduction method leading to 18 mmol·h-1·g-1 for 3 mol% copper loading.

INTRODUCTION. It has been widely stated that the improvement and optimisation of TiO2 as photocatalyst is an important task in order to achieve a real application of heterogeneous photocatalysis in the near-future.1 Within this context, the interest on energy related applications of photocatalysis are currently growing.2 Thus, H2 production by photoreforming or the synthesis of valuable fuels from CO2 photoreduction reactions appears as the new challenged topics in this field.3,4,5 Taking into consideration the current socioeconomical and environmental situation, it is widely believed that hydrogen will play an important role since it is considered the ultimate clean energy carrier. However, when TiO2 is exploited in hydrogen production using photoreforming reaction, some important factors make in principle its application far from a practical situation.1 In this sense, rapid recombination process of the photogenerated charge pairs and the occurrence of the eventually backward reactions are considered critical points that might be overcame. Thus, the incorporation of metal ions has been traditionally used as charge trapping sites and avoid the electron–hole recombination processes.6,7 Among the potential options, noble metals (Pt, Au, Pd) has been widely considered.8,9,10 Alternatively, transition metal doping with Cu, Fe, Co or Ni have recently turned as promising cheaper option.11,12,13,14,15 Although the rates obtained are still far from those obtained for noble metals, copper based catalysts appears as a promising candidate. In spite of this, the nature of the active copper species (Cu2O or CuO) and other external factors governing its photoactivity is less understood.15 Thus, some authors claimed that Cu2O species are the responsible of the photoactivity for H2 generation from water reduction.16,17 Thus, Xi et al correlated the presence of easily reducible Cu2O species 2 ACS Paragon Plus Environment

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toward metallic Cu during H2 production reaction with the improved photocatalytic activity.17 On the other hand, other authors argued that the presence of CuO would be the responsible of the enhanced the separation of photo-induced electrons and holes.18 Moreover, Ampelli et al reported the improving effect of Cu2+ incorporation into the TiO2 structure which leads to the creation of oxygen vacancies.13 Indeed, these authors concluded that embedded CuOx@TiO2 systems showed higher photocatalytic performances with respect to impregnated samples.19 Within this context, Korzhak et al investigated the relationships between the quantum efficiencies of the photocatalytic hydrogen production and the textural characteristics of a Cu-doped TiO2 system.20 These authors correlated the photoactivity with the Cu nanostructure obtained specially with deterioration of the electronic interactions between the components of metal– semiconductor composites with growth of the metal nanoparticles size. On this basis, the interaction with TiO2 is expected to stabilize the copper oxides against photocorrosion and could enhance the activity by a most efficient process. Thus, well dispersed CuOx nanoparticles would be easily reduced during the reaction forming well dispersed copper metal particles which would favour electron trapping.19 From these considerations, it is assumed that the complex structural, morphological and chemical features of copper species would strongly affect the final photocatalytic performance for H2 production reaction. In the present paper we try to present an exhaustive structural and surface characterization of different Cu-doped TiO2 obtained from different doping method. From the comparison of the chemical features of Cu species we propose a tentative correlation with the final photocatalytic performance for H2 production reaction.

EXPERIMENTAL.

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Catalysts preparation and characterisation TiO2 system was prepared by a sol-gel method using titanium tetraisopropoxide (TTIP) as precursor (10 mL TTIP) in water/isopropanol solution (200 mL iPrOH and 2 mL H2O). Forced hydrolysis of the TTIP solution was achieved by adding certain volume of bidistilled water (8.4 mL). Finally the pH was adjusted to 9 by adding NH4OH. Copper doping has been performed by means of two different methods: Impregnation and chemical reduction. Impregnated copper doped systems were obtaining by incipient wetness impregnation using Cu(NO3)2 as copper precursor dispersed in H2SO4 1M

by means of 2 mL

dispersion per gram of fresh TiO2 (These samples were named as CuXSTi where X is the Cu mol%). Thus obtained precursors were then dried at 120ºC overnight. Doped TiO2 systems were calcined in air at 650ºC for 2 hours. In order to discuss the effect of H2SO4 impregnation we have also prepared a reference CuXTi catalyst by using water instead of H2SO4 in the impregnation step. This reference CuXTi series has been calcined at 400ºC for 2 hours. Without sulfate pretreatment, TiO2 precursor suffers rutilization process from the first stage of calcination. For this reason non sulfated reference material was submitted to calcination at 400ºC vs. 650ºC of sulfated one. These temperatures correspond to the optimum calcination temperature for non-sulfated and sulfated series (result not shown).21 On the other hand, the reduced series has been obtained by chemical reduction of copper precursor by means of NaBH4. Thus 1 g of STiO2 or TiO2 (calcined at 650ºC and 400ºC respectively) was dispersed in 100 mL of water solution containing the corresponding stoichiometric amount of copper precursor. Then an excess of NaBH4 was added and the dispersion was thoroughly stirred for 1 hour at room temperature.

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Finally this solution has been filtered and washed with distilled water and the obtained powder dried at 110ºC overnight. BET surface area measurements were carried out by N2 adsorption at 77 K using a Micromeritics 2000 instrument. X-ray diffraction (XRD) patterns were obtained using a Siemens D-501 diffractometer with Ni filter and graphite monochromator. The X-ray source was Cu Kα radiation. Anatase-rutile fractions were calculated by taking into account the relative diffraction peak intensities. From the line broadening of corresponding X-ray diffraction peaks, we have calculated the mean crystallite size according to Scherrer equation. Diffuse reflectance spectra were obtained on a UV–vis scanning spectrophotometer Shimadzu AV2101, equipped with an integrating sphere, using BaSO4 as reference. UV-vis spectra were performed in the diffuse reflectance mode (R) and transformed to a magnitude proportional to the extinction coefficient (K) through the Kubelka-Munk function, F(R∝). For the sake of comparison, all spectra were arbitrary normalized in intensity to 1. Band gap values were obtained from the plot of the modified KubelkaMunk function (F(R∝)E)1/2) versus the energy of the absorbed light E. XPS data were recorded on 4·4 mm2 pellets, 0.5 mm thick, prepared by slightly pressing the powdered materials which were outgassed in the prechamber of the instrument at 105ºC up to a pressure < 2·10-8 torr to remove chemisorbed water from their surfaces. Spectra were recorded using a Leybold-Heraeus LHS-10 spectrometer, working with constant pass energy of 50 eV. The spectrometer main chamber, working at a pressure