Juzheng
Zhang
a,
Lauren R.
Grabstanowicz
b,
Shanmin
Gao
*ab,
Narayan S.
Hosmane
b,
Baibiao
Huang
c,
Ying
Dai
c,
Di-jia
Liu
d and
Tao
Xu
*b
aSchool of Chemistry and Materials Science, Ludong University, Yantai, 264025, Shandong, P. R. China
bDepartment of Chemistry and Biochemistry, Northern Illinois University, DeKalb, IL 60115, USA. E-mail: txu@niu.edu; gaosm@ustc.edu
cState Key Lab of Crystal Materials, Shandong University, Jinan, 250100, Shandong, P. R. China
dChemical Sciences and Engineering Division, Argonne National Laboratory, Argonne, IL 60439, USA
First published on 18th November 2011
We report an architecturally controlled synthesis of SiO2/TiO2−xCx/C nanoporous composites that exhibit high absorption capability and efficient visible-light photocatalytic activity. The nanoporous composites are composed of silica particles as the cores and TiCl4 as the precursor for the TiO2 shell. Tannin is used as the binding agent between the core and the precursor shell, the carbon source, and the porosity promoter. The structure, crystallinity, morphology, and other physical–chemical properties of the samples are characterized by X-ray diffraction (XRD), transmission electron microscopy (TEM), high-resolution transmission electron microcopy (HRTEM), X-ray photoelectron spectroscopy (XPS), N2 adsorption–desorption isotherm measurements, UV–vis diffuse reflectance spectroscopy (DRS), and photoluminescence (PL). The chemical contents of the SiO2/TiO2−xCx/C nanoporous composites were also analyzed by energy dispersive X-ray spectra (EDX). The formation mechanism of the nanoporous composites was extensively discussed. Methylene blue (MB) solutions were used as model wastewater to evaluate the adsorption and photocatalytic activity of the samples under natural sunlight and visible light. Fourier transform-infrared spectroscopy (FT-IR) and mass spectrometry (MS) were used to investigate the photodegradated species on the photocatalysts and in solution, respectively. The SiO2/TiO2−xCx/C nanoporous composite samples exhibit remarkably enhanced visible-light photoactivity than Degussa P25 and pure TiO2, and can be readily collected for reuse by gravitational sedimentation.
In general, two methods are utilized to enhance the light harvesting of TiO2 in the visible region. One method is to sensitize TiO2 with color centers that have proper energy levels for photoelectron transfer between the color centers and TiO2.6,7 A cost-effective sensitization of TiO2 is typically achieved by addition of non-metals such as I8,9 and S.10,11
The other way is to form a doping level through intercalation of proper atoms into the anatase form. For example, by doping carbon12,13 and nitrogen14–16 atoms into the TiO2 lattice, a new, weak absorption is generated at lower energies, which is a promising approach for inducing effective vis-absorption. This is because the C2p or N2p orbital has a higher energy than that of O2p. The C or N doping involves substitution of O atoms by C or N producing new energy states deep in the TiO2 band gap, which are responsible for the visible light absorption. Direct doping of impurity into the lattice of anatase TiO2 by using a chemical method is not feasible because it requires very high temperature, causing transition of photoactive anatase to non-active rutile, and thermal rupture of the desired TiO2 structure. Thus, the dopants must be premixed with the precursor TiO2 at a molecular level, followed by the conversion of the precursor TiO2 to anatase. Thus, organotitanium compounds are often used as the precursor source for TiO2 and carbon dopants. However, organotitanium is too expensive for mass production. Although doping by a gas-phase method can avoid this defect, the requirement of equipment is relatively high.16
In addition to the narrow band gap, the enhancement of surface area of the TiO2 is another important aspect for the efficiency of the materials, because the desired photocatalytic reactions occur at the interfaces of the catalyst-pollute solution.17 Intuitively, a plausible approach is to maximize the photoactivity of TiO2 through synthesis of small titania nanoparticles (NP) so as to possess a large surface area and a large number of reactive sites. However, the small particle size makes it a practical challenge for the reuse of the TiO2-nanoparticle-based photocatalysts because the separation of the nanoparticles from the pollute solutions requires a costly centrifugation process. Moreover, reduction in particle size also introduces more internal crystal defects that act as charge trap states to diminish the effective transport of photoinduced charges to the external surface sites,18,19 where the desired photocatalytic reaction occurs.
It has been confirmed that TiO2/carbon composites or carbon-modified TiO2 could increase adsorption capacity and improve photodegradation performance in the visible region.20–25 Composites of TiO2/C have also been shown to improve the energy and power density of electrochemical cells and enhance the energy-storage capacity.26 Therefore, TiO2 composited with different forms of carbon, such as activated carbon,27,28graphite,29 and carbon nanotubes,30,31 have been fabricated to obtain novel structures and properties. Various organic compounds are suitable as carbon sources.32,33 The prepared carbon-coated anatase nanocrystals exhibit fast adsorption of MB with high capacity.29
Furthermore, as most photocatalytic reactions occur at the surface region of the TiO2 particles, it is not an economical configuration to have a large amount of photocatalytic materials residing in the internal bulk of the particles which are not in direct contact with the pollute solutions.
In all these regards, it is exceptionally warranted to develop a TiO2 matrix with a large surface area for adsorbing more pollute molecules and proper doping for visible light harvesting. However, simultaneously the TiO2 matrix must maintain a large particle size so that the photocatalysts can be conveniently collected through gravitational precipitation. Logically, a larger particle size usually leads to less surface area, and these two factors are diametrically opposing. However, an effective way to decouple this inverse interlink is to construct highly porous large particles.
Hence, in this work, we aim to integrate (1) the synthesis of large TiO2 particles with high porosity for enhanced adsorption of pollute molecules, (2) carbon doping in TiO2 for photoactivity in the visible region, and (3) minimizing the usage of TiO2 by replacing some internal TiO2 with materials that are more cost-effective, e.g.silica. We chose silica sol as the internal stuffing material because of its rich surface hydroxyl groups that enable us to covalently bind precursor carbon dopants, and thus to spatially control the pathways of the doping process. Moreover, we also aim to coat a non-continuous ultrathin layer of amorphous carbon on the surface of TiO2, which can further boost the adsorption of pollute molecules.34,35 (4) The starting materials for TiO2 should be largely available based on the current industrial infrastructure. In industry, TiCl4 is an intermediate product during the mass production of TiO2, known as a chloride process (Dupont method). This process is widely used in North America due to its relatively low energy consumption and better product consistency.36,37 Therefore, for the commercialization of our photocatalysts, the use of TiCl4 as the precursor for TiO2 is more practical and attractive from an industrial point of view since it does not require additional production infrastructure. In contrast, the use of organotitanium as the precursor for TiO2 will inevitably involve additional costs and complications for the mass synthesis of organotitanium.
In this work, we utilize tannin as the binding agent, carbon source, and porosity promoter to achieve SiO2 (core)–C-doped-TiO2 (shell) nanoporous composites. In addition, an ultrathin amorphous carbon layer forms on the surface of TiO2 to further enhance the surface area. This structure is termed as SiO2/TiO2−xCx/C. Tannin is an organic molecule with multiple hydroxyl groups that can be utilized as a binding agent to glue the precursor SiO2 core with the precursor TiO2 shell, since both SiO2 and TiO2 are abundant with surface hydroxyl groups. The gaseous species, resulting from the decomposition of tannin under heat treatment, can pulverize the TiO2 shell to promote the formation of a nanoporous shell. Moreover, excessive tannin molecules can further anchor on the TiO2 shell to form a precursor carbon layer that can be converted to an ultrathin layer of amorphous carbon upon carbonization. The extra SiO2 particles in the composition serve as agglomeration centers in order to facilitate the interconnection between the particles. Thus, large TiO2 particles with high porosity and SiO2 cores are expected to form. As a proof-of-concept, we demonstrate that SiO2/TiO2−xCx/C nanoporous composites can be synthesized, exhibit an excellent adsorption and photodegradation of model pollute molecules in aqueous solution under visible light radiation, and be readily collected via gravitational sedimentation.
A typical procedure for preparing the SiO2/TiO2−xCx/C nanoporous composites is described as follows. First, 20 g TiCl4 was added drop-wise slowly into 80 mL of distilled water in an ice bath. The obtained product was labeled as the TiCl4 stock solution. Then, 1.0 g tannin powder was dissolved in 30 mL of distilled water and the resulting solution was added drop-wise into 10 g 30 wt% silica sol. Under stirring, this mixture solution was warmed in a water-bath at 80 °C for 3 h. The above procedures lead to the formation of the SiO2–tannin composites.
Then, the freshly prepared TiCl4 stock solution was added slowly to the SiO2–tannin composite solution and the resulting mixture was kept at 60 °C for 4 hours. After that, the mixture became a suspension, which was continuously stirred for an additional 12 h at room temperature. Finally, the mixed slurry was desiccated at 80 °C for 6 h and at 120 °C for 6 h to yield a solid composition. In order to obtain carbon-doped and carbon coated TiO2, these solid composites were further heated at various temperatures under a nitrogen atmosphere. The heating rate was 5 °C min−1 and the flow rate of nitrogen was 50 mL min−1. In the final stage of the heat treatment, 5 v% of air was introduced and maintained for 20 min. After heat treatment, the resulting powders were cooled down to room temperature in a nitrogen atmosphere. The samples are now denoted as STC-T, where the second T refers to the applied temperature during the heat treatment. For comparison, pristine TiO2 powder calcined at 500 °C (denoted as TiO2-500) was also prepared without the addition of Si sol and tannin.
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Fig. 1 XRD patterns of STC-T porous composites heat treatment at different temperatures. (A = anatase; R = rutile). |
a Crystal size was determined based on the XRD peak (101) and the Debye–Scherrer equation. BET surface areas were calculated from the linear part of the BET plots. Total pore volumes were obtained from the volume of N2 adsorbed at P/P0 = 0.995. Average pore diameters were estimated using the desorption branch of the isotherm and the Barrett–Joyner–Halenda (BJH) formula. | ||||
---|---|---|---|---|
Heat treatment temperature/°C | 400 | 500 | 600 | 700 |
Crystalline size/nm | 9.3 | 11.4 | 14.3 | 21.6 |
BET specific surface area/m2 g−1 | 392.4 | 366.8 | 305.7 | 263.5 |
BJH pore volume/cm−3 g−1 | 0.547 | 0.492 | 0.387 | 0.316 |
Average pore diameter/nm | 8.423 | 9.745 | 11.612 | 13.327 |
In general, the crystallinity of anatase TiO2 can be improved by high temperature treatment, but at the risk of phase transition of the photoactive anatase to a poor photoactive rutile. Carbon doping, coating, and SiO2–TiO2 composite can mitigate this dilemma by effectively stabilizing the anatase structure of TiO2 under high temperature.38,39 This is evidenced by the fact that our SiO2/TiO2−xCx/C nanoporous composites calcined at 700 °C still retain the anatase phase.
The specific surface area and pore size of the samples were characterized by nitrogen adsorption–desorption isotherm measurements. Table 1 summarizes the BET specific surface area and the apparent average pore size of our samples. The pore volume and specific surface area decrease with increasing calcination temperature. However, the samples still maintain relatively high specific surface area and pore size even for sample STC-700. This high thermal stability of our sample is an important feature for maintaining high surface area since heat treatment is a necessary step for the formation of a porous structure.
XPS measurements were carried out to investigate the presence, contents, and chemical states of Ti, Si, C, and O in the samples. The XPS of the STC-500 composite with a Ti/Si ratio of 2.1:
1 are presented in Fig. 2. In the survey spectra (Fig. 2(a)), the elements Ti, Si, O and C are clearly identified. Fig. 2(b) shows the high-resolution XPS (HR-XPS) of O1s, showing a broad peak that can be split into four peaks at 529.6, 531.2, 532.0, and 533.1 eV. These four peaks are attributed to Ti–O–Ti, Ti–O–Si, –OH, and Si–O–Si bonds, respectively.40 The binding energy of the O1s electron of Ti–O and Si–O in the composite is 1.37 eV higher than that in pure TiO2,41 but is 0.26 eV lower than that of Si–O in pure SiO2. The shift of the binding energy of the O1s electron in our samples can be ascribed to the bond of Ti–O–Si.22 The HR-XPS of Si2p (Fig. 2(c)) show two peaks at 103.7 eV and 101.6 eV, which correspond to Si–O–Si and Si–O–Ti bonds, respectively.42
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Fig. 2
XPS spectra of STC-500 with a Ti/Si molar ratio of 2.1![]() ![]() |
Fig. 2(d) and (e) show the HR-XPS of Ti2p and C1s core levels. The Ti2p spectrum can be deconvoluted into three peaks at 458.3, 459.0, and 459.5 eV, which can be attributed to Ti–C–Ti, Ti–O–Ti, and Ti–O–Si bonds, respectively.43,44 The four peaks at 282.3, 284.9, 286.2, and 288.7 eV were observed for C1s. The C–Ti bond is located at ca. 282.5–281.5 eV and the C–Si bond is located at about 282.2–282.8 eV.45 Accordingly, the C1s peak at 282.4 eV can be ascribed to the substitution of an oxygen atom by a carbon atom in the lattice of TiO2, leading to an O–Ti–C bond.46 The peak at 284.9 eV is due to the elemental carbon at the surface of TiO2.47 This is further evidenced by a TEM study, which will be described below. The peaks at 286.2 and 288.7 eV are likely due to the C–H and C–O bonds in residual tannin.
XPS analysis of the STC-500 sample demonstrated that the atomic concentrations of O, Ti, C, and Si are 67.38%, 15.12%, 12.04%, and 5.01%, respectively. The atomic ratio of titanium to silicon was about 3:
1. In the sample preparation process, the ratio of titanium to silicon is ca. 2.1
:
1, the XPS results show that the ratio of titanium to silicon is significantly higher than the synthetic stoichiometry. Since XPS is a surface sensitive analysis technique, the higher content of Ti found in the XPS study suggests that Ti is preferred on the surface region while Si is more preferential in the bulk. As indirect and supportive evidence, EDX analysis in Fig. 2(f) shows that the atomic ratio of Ti to Si is 2.4
:
1, close to the synthetic stoichiometry. This is because EDX is not a surface-sensitive technique and it detects the elements in deeper layers. Thus, it is not surprising that the EDX result is closer to the stoichiometry based on the sample preparation. The XPS and EDX studies on other samples are summarized in Table 2. With an increase in the heat treatment temperature, the carbon content decreases gradually, indicating the loss of tannin at higher temperatures. Meanwhile, with the increase in the heat treatment temperature, the ratio of Ti to Si becomes closer to the synthetic stoichiometry. This can be understood as the result of sintering of the TiO2 with SiO2 at elevated temperature.
The typical microstructures of transparent silica sols and STC-T samples were characterized by TEM and HRTEM analysis, and the results are shown in Fig. 3. Also, Fig. 3a shows that the silica sol consists of silica nanospheres of ∼10 nm in diameter with a narrow size distribution. Fig. 3b shows the TEM image of sample STC-400, however, STC-400 does not exhibit an obvious porous structure, but the SiO2 nanoparticles embedded in the TiO2 can be observed. As the calcination temperature increases to 500 °C, the sample becomes more porous as shown in the TEM image (Fig. 3c). Moreover, there is a very thin layer of amorphous carbon covering the surface as shown in the HRTEM image (Fig. 3d). A further elevation of heat treatment to 600 °C yields a sample with a bimodal meso/nanoporous structure (Fig. 3e). More interestingly, we also observed the cavity core/shell structure (Fig. 3f) in sample STC-600. We assume that the complete decomposition of the tannin layer that is sandwiched between the SiO2 nanoparticles and the outer TiO2 layer led to the pulverization of the TiO2 layer. When the heat treatment temperature reaches 700 °C, the nanoporous structure diminished due to sintering, while the mesopores remain as shown in Fig. 3g. In the HRTEM image of STC-700 (Fig. 3h), the lattice structure of TiO2 can be clearly indexed. Carbon is clearly visible at the surface region of the composite. Overall, TEM images clearly demonstrate the temperature effect on the morphology of SiO2/TiO2−xCx/C nanoporous composites.
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Fig. 3 (a) and (b) TEM images of transparent colloidal silica sol and STC-400. (c) and (d) TEM and HRTEM images of STC-500. (e) and (f) TEM images of STC-600. (g) and (h) TEM and HRTEM images of STC-700. |
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Scheme 1 Schematic presentation of the fabrication of SiO2/TiO2−xCx/C nanoporous composites. |
First, there are many surface hydroxyl groups on the SiO2 colloid particles, which provide sufficient sites to bind tannin molecules containing multi-hydroxyl groupsviahydrogen bonds (Schemes 1(a) and (b)). Upon heating, the surface active sites on silica particles can react with the attached tannin through dehydration. Note that there are still excessive tannin molecules in the solution phase as indicated in Scheme 1c.
As TiCl4 solution was added into the above mixture, part of the TiCl4 hydrolyzes at the surface of the SiO2 nanoparticles due to the enriched surface hydroxyl groups provided by the surface tannin molecules. This leads to the formation of a shell of precursor TiO2 that attaches to the SiO2 nanoparticleviatannin molecules. Because of the abundant surface hydroxyl groups on the shell of the TiO2 layer, the excessive tanning molecules in the solution phase can further attach to the surface of the TiO2 shell viahydrogen bonds (Scheme 1d).48,49 This structure is termed as SiO2/tannin/TiO2. However, we do not exclude the possibility that a certain amount of TiCl4 hydrolyzed directly in the solution to form independent amorphous TiO2 particles, and some SiO2 particles are not wrapped by TiO2.
Upon gradual evaporation of the solvent, the SiO2/tannin/TiO2 particles, the TiO2 particles, and the SiO2 particles aggregate to form the precursor composites (Scheme 1e).
The initial calcinations were carried out in a nitrogen atmosphere, which leads to the crystallization of TiO2, carbonization of tannin (i.e. the formation of the amorphous carbon layer at the surface of the TiO2 shell), carbon intercalation (i.e.carbon doping into the TiO2 lattice), and the pulverization of the TiO2 layer due to the release of gaseous species from the decomposition of the tannin layer in between the SiO2 cores and the TiO2 shell. In order to minimize the oxygen vacancies in the TiO2 lattice upon heating, air was introduced during the final calcination stage. However, this can also lead to the loss of carbon, which is evident in the TEM and XPS studies.
Photoluminescence (PL) emission spectra have been widely used to explore the efficiency of charge carrier trapping, migration, and recombination in order to understand the fate of electron–hole pairs in semiconductor particles.50Fig. 5(a) shows the room-temperature PL spectra for pure TiO2-500 and STC-T samples excited by UV light at 320 nm. It is clear that the PL intensity of the pure TiO2-500 is higher than that in the spectra of STC-T composite samples. This indicates that carbon doping, SiO2 composites, the surface amorphous carbon, and surface hydroxyl groups serve as charge trap states to suppress the radioactive electron and hole recombination.51,52
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Fig. 5 PL spectra of TiO2-500 and STC-T samples under UV-320 nm (a) and visible light 520 nm (b). |
However, for excitation with visible light at 520 nm, the STC-T samples exhibit a much better PL effect than pure TiO2-500 (Fig. 5b). The disappearance of PL in TiO2-500 is due to the insufficient energy of the visible photons that is lower than the band gap of pure TiO2. In contrast, for the carbon doped STC-T samples, the reduced band gap allows absorption in the visible region to produce photoelectrons and holes.53
Methylene blue (MB) is a brightly colored blue cationic thiazine dye and is often used as a test model pollutant in semiconductor photocatalysis. Fig. 6(a) shows the adsorption and photodegradation ability of methylene blue (MB) solutions by using our STC-T samples in comparison to P25 and pure TiO2-500. A blank experiment was also carried out. The pure MB solution cannot decompose without a catalyst. Prior to the turn-on of the solar light, the concentrations of MB in the presence of the STC-T samples deplete much faster than those in the P25 and TiO2-500 samples. This is especially seen for the STC-400 sample, nearly 60% of the dye molecules were adsorbed within 30 min. We ascribe this effect to the much larger surface area of the STC-T samples than that of the P25 or TiO2-500 samples as characterized and discussed above. For STC-T samples, their adsorption capacity increases with the decrease in the heat treatment temperatures. This can be credited to the reduced surface area and the loss of the surface amorphous carbon upon sintering and oxidation of carbon at higher temperatures.
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Fig. 6 (a) The blank MB solution, adsorption and photodegradation of MB solutions by using pure TiO2-500, P25 and STC-T samples as photocatalysts under visible light irradiation. (b)–(f) The photographs of 20 mg STC-T and P25 in 100 mL MB solution under sunlight in the static state. The photograph of a pure MB solution is also shown for comparison. |
Furthermore, Fig. 6(a) shows that under visible light illumination, the MB solutions containing the STC-T samples underwent significant degradation and became nearly transparent within 40 min. It should be noted that the STC-500 sample exhibits the best photocatalytic activity and within 23 minutes the absorption band due to MB nearly diminishes. In contrast, the MB solutions containing pure TiO2-500 and P25 show very limited degradation.
Fig. 6(b)–(f) shows the real-time photographs of the samples under radiation by natural sunlight. It is striking that after initial stirring, the MB solutions containing STC-400 and STC-500 samples become nearly transparent and the powders are all precipitated. In fact, over 90% of the methylene blue was degraded after 25 min of sunlight irradiation at 18 °C.
In contrast, the MB solution containing P25 is still opaque and bluish. This simple separation by gravitational sedimentation exhibited by the STC-400 and STC-500 samples increases the potential use of our samples as practical photocatalysts for degradation of organic pollutants. In comparison, the pure TiO2-500 sample and P25 showed very little MB adsorption and the suspensions have to be separated by centrifugation.
The cyclic stability test under the same conditions of the STC-500 sample was also examined and shows excellent photocatalytic activity in degrading MB solution, as shown in Fig. 7. No significant decrease in its photocatalytic oxidation activity is observed after being used 6 times, which makes it very promising for practical application.
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Fig. 7 Recycling test results by using the STC-500 sample. |
To eliminate the possibility that the enhanced photocatalytic activity of our STC-T samples mainly results from their enhanced physisorption alone, the FTIR and MS spectra of the STC-500 samples have been collected before and after the photodegradation of MB. As illustrated in Fig. 8, the FTIR spectra of sample STC-500 before (curve a in Fig. 8) and after degradation (curve b in Fig. 8) show no significant discrepancy. In contrast, the FTIR spectrum of MB (curve c in Fig. 8) shows more complicated vibrational modes due to the organic molecule. Therefore, it is unambiguous that the visible-light photodegradation on TiO2 is the cause of the depletion of MB molecules.
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Fig. 8 FT-IR spectra of STC-500 and pure methylene blue: (a) STC-500 before degradation, (b) STC-500 after degradation and (c) pure methylene blue. |
For further confirmation, a mass spectrometer is used to study the species in the solution after photocatalysis. Fig. 9 suggests that the organic species in water undergo a structural degradation during the course of photocatalysis. After 30 minutes, the remaining species in solution are mainly formic acid and acetic acid.
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Fig. 9 Mass spectra of (a) the methylene blue solution before photocatalysis, (b) after 10 minutes and (c) after 30 minutes photocatalysis with sample STC-500 under one Sun 1.5 AM G provided by a solar simulator (Photo Emission Inc. CA, model SS50B). The 47 and 61 peaks are attributed to the protonated formic acid and acetic acid respectively. |
The high adsorption capacity of our nanoporous composite (the STC-T) samples is a product of several facts. First, the nanoporous structure resulting from the decomposition of tannin and the meso/nanopores composed of the voids between particles, together, provide a vast amount of surface active sites to adsorb reactive species. Moreover, the ultrathin amorphous carbon layer covering the surface of TiO2 provides additional adsorption sites. The enhanced specific surface area consequently promotes the photocatalytic activity by increasing the concentration of contaminants and reaction intermediates near the surface of TiO2. Carbon doping in the lattice of TiO2 narrows the band gap, thus leading to visible light-induced charges that are essential for the desired enhanced photocatalytic oxidation. In addition, the near-surface doping of carbon in TiO2 shortens the transport distance of photocharges to the surface region, where the desired photocatalytic reaction occurs.
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