Enhancement of the photocatalytic activity of a TiO2/carbon aerogel based on a hydrophilic secondary pore structure

Hua'nan Cuia, Zhenxing Liangb, JinZhong Zhangc, Hong Liua and Jianying Shi*a
aKey Laboratory of Environment and Energy Chemistry of Guangdong Higher Education Institutes, School of Chemistry and Chemical Engineering, Sun Yat-sen University, Guangzhou 510275, China. E-mail: shijying@mail.sysu.edu.cn
bGuangdong Provincial Key Laboratory of Fuel Cell Technology, School of Chemistry and Chemical Engineering, South China University of Technology, Guangzhou 510641, China
cDepartment of Chemistry and Biochemistry, University of California, Santa Cruz, CA 95064, USA

Received 29th March 2016 , Accepted 14th July 2016

First published on 14th July 2016


Abstract

Improving the separation and utilization of electrons and holes in a photocatalytic process is a guarantee for high photocatalytic efficiency. We report a strategy to enhance the photocatalytic performance based on fabrication of a hydrophilic secondary pore structure by incorporating TiO2 into a porous carbon aerogel (CA) with a 9.3 nm pore diameter, where TiO2 resides on both the inner and outer surfaces of CA as evidenced by N2 sorption isotherms and transmission electron microscopy. In such a structure, the spatial separation efficiency of photoelectrons and photoholes is supposed to get enhanced with interface electrons transferring into the inner surface of the pores via conductive CA. As a result, HO˙ formation can be promoted in the confined inter surface of the hydrophilic secondary channel through O2 reduction with the participation of photoelectrons and H2O. And the remaining photoholes on the outer surface can oxidize water to generate HO˙ as well. In contrast, TiO2 is mainly dispersed on the outer surface of CA as small pore diameters of 3.4 and 4.3 nm; as a result, only uncombined photoholes on the outer surface contribute to HO˙ generation via the water oxidation route. In line with this understanding, TiO2/CA (9.3 nm) shows the largest amount of HO˙ and thereby the highest efficiency of dimethyl phthalate degradation, as respectively evidenced by the electron paramagnetic resonance spectroscopy and the photocatalytic degradation test. These findings unveil the contribution of the surface/interface synergy effect on the separation and utilization of electrons and holes in photocatalytic process, and provide a potential strategy to enhance the photocatalytic performance.


Introduction

As an advanced oxidation process, photocatalytic degradation mediated via TiO2 is an efficient method to eliminate organic pollutants from water. It has drawn much attention in the field of removing phthalate esters (PAEs) from an aqueous environment, because the end products after photocatalysis on PAEs are carbon dioxide, water, and inorganic mineral ions.1–7 For TiO2 photocatalysts, improving the separation and utilization of electrons and holes in photocatalytic processes is highly desired for high photocatalytic efficiency.8 Surface modification,9 sensitization10 and transition-metal doping11 are widely used strategies to optimize TiO2 photocatalytic performance. In addition, assembling TiO2 with carbon materials is another effective way,12 as porous carbon support has been found to selectively accumulate reactants into its abundant pores13–15 and its excellent conductivity serves to accelerate the separation of photogenerated carriers.16–18 Some studies have suggested that such porous carbon powder is also capable of absorbing light, and the generated photoelectrons can be transferred to the conduction band of TiO2 for further use.19 Despite a large number of assemblies of TiO2 with carbon were reported to data,17,20–23 few systematic studies are undertaken to reveal the function of pore structure on photocatalytic performance, especially secondary pores with unique spatial features that are formed by encapsulating TiO2 into carbon pore cavities. It has been reported that the unique pore-confined space can potentially play a vital role in enhancing catalytic activity and selectivity in heterogeneous catalysis.24–26 Particularly, the CNT-confined TiO2 exhibited improved visible-light activity as the modification of the electronic structure of TiO2 induced by the unique confinement inside CNTs.27

Carbon aerogel (CA), possessing unique three-dimensional ultra-porous network with high porosity (80–98%), low electrical resistivity (≤40 mΩ cm), and large surface area (400–1100 cm2 g−1),28,29 is a promising material in the application of processing contaminants.28,30 In this work, three kinds of mesoporous CA with several nanometer pore diameters31 were employed as support to assemble TiO2/CA-X composite catalysts, where X denotes as the pore diameter of CA. Dimethyl phthalate (DMP), a member of phthalate acid esters (PAEs) detrimental to human being as endocrine disruptors, mutagens, reproductive and developmental toxicants,7,32,33 was chosen as the target pollutant for evaluating the photocatalytic properties of the TiO2/CA catalysts. Only TiO2/CA-9.3 shows the enhanced photocatalytic activity, and TiO2/CA-3.4 and TiO2/CA-4.3 even gives the lower activity than bare TiO2. It was found that the HO˙ formation is correlated with the secondary pore structure of TiO2/CA-X, and the contribution of surface/interface synergy effect on the separation and utilization of electrons and holes in the photocatalytic performance is discussed.

Results and discussion

Pore structure of TiO2/CA-X

The pore structure of CA-X before and after assembling TiO2 are investigated by N2 adsorption–desorption isotherms, and the results are shown in Fig. 1a and b, respectively. The isotherms of CA-X and TiO2/CA-X featured IV-type character with specific hysteresis loop at relatively high pressure, implying that both CA-X and TiO2/CA-X are typical mesoporous materials. Fig. 2 shows the pore distribution of CA-X and TiO2/CA-X samples calculated by a DFT model on ASiQwin software.34,35 It can be seen that mesopores dominate the pore structure in both CA-X and TiO2/CA-X samples with a small proportion of micropores and macropores. The detailed information of the pore structure is summarized in Table 1, e.g. pore volume, pore diameter and BET surface area.
image file: c6ra08074j-f1.tif
Fig. 1 N2 adsorption–desorption isotherms of (a) CA-X and (b) TiO2/CA-X and pure TiO2.

image file: c6ra08074j-f2.tif
Fig. 2 Pore distribution of (a) CA-X and (b) TiO2/CA-X and pure TiO2.
Table 1 Pore parameters of carbon, TiO2, and TiO2/CA
Sample Da (nm) SBETb (m2 g−1) Vmicroc + Vmesod (cm3 g−1) DMP adsorption amount (mg g−1)
a Average mesopore size calculated form DFT method.b Brunauer–Emmett–Teller (BET) surface area calculated from adsorption branch of the N2-sorption isotherm.c Micropore (<2 nm) volume calculated from cumulative pore volume of DFT method.d Mesopore (2–50 nm) volume calculated from cumulative pore volume of DFT method.
CA-3.1 3.1 1173 0.88 8.6 ± 0.4
CA-4.3 4.3 954 0.96 7.7 ± 0.5
CA-9.3 9.3 709 1.2 10.6 ± 0.6
TiO2 4.4 84 0.07 0 ± 0.2
TiO2/CA-3.1 3.8 237 0.17 6.4 ± 0.5
TiO2/CA-4.3 4.1 215 0.18 6.2 ± 0.5
TiO2/CA-9.3 6.1 124 0.17 4.4 ± 0.5


The average pore diameters of three pristine CA samples are 3.1, 4.3 and 9.3 nm, as shown in Table 1. After assembling TiO2, the pore diameters of CA-3.1 and CA-4.3 remain almost unchanged, but it decreases from 9.3 to 6.1 nm for CA-9.3. As seen in Table 1, both the volume of micropore (<2 nm) and mesopore (2–50 nm) and the BET surface of three TiO2/CA-X samples decrease sharply when compared with those of the pristine CA-X samples. The decrease can be attributed to either the blockage of pore channels by TiO2 dispersed on the carbon surface or the shrinkage of pore channels as TiO2 was encapsulated into pore channels. The unchanged pore diameter of CA-3.1 and CA-4.3 indicates that TiO2 was prominently dispersed on the outer surface of CA-3.1 and CA-4.3. While for CA-9.3, the dwindled 6.1 nm pore size suggests that, in addition to being dispersed on the outer surface, a considerable amount of TiO2 was dispersed into the pore channels of CA-9.3. It is acknowledged that the capillary force is the driving force to infiltrate the precursor solution into the support channels during the preparation of supported catalysts,36 which could account for the formation of secondary pore in TiO2/CA-9.3. The 3.1 and 4.3 nm pore diameters of CA may be too small to allow the infiltrate of Ti precursor into the pore channel.

Composition and structure of TiO2/CA-X

The carbon content of TiO2/CA-X samples was analyzed by thermogravimetry (TG) and differential thermal gravity (DTG) (Fig. S1). The same loss steps at around 500 °C related to the carbon combustion indicate three samples possess the comparable carbon contents of about 15 wt% (Table 2), that is, the same amount of TiO2 is dispersed on them. X-ray diffraction was used to determine the crystal structure of pristine TiO2, TiO2/CA-X and CA-X, and diffraction patterns are shown in Fig. S2. A set of diffraction peaks related to anatase (PDF#21-1272) are observed in pristine TiO2 and TiO2/CA-X, in comparison, CA-X presents amorphous structure with broad diffraction patterns shown in insert of Fig. S2. The results indicate that three TiO2/CA-X samples possess the same TiO2 crystal structure, irrespective of the pore diameter of CA.
Table 2 Carbon content of TiO2/CA-X samples
Sample C content (%) TiO2 content (%) C/TiO2 ratio
TiO2/CA-3.1 15.0 85.0 0.18[thin space (1/6-em)]:[thin space (1/6-em)]1
TiO2/CA-4.3 14.9 85.1 0.18[thin space (1/6-em)]:[thin space (1/6-em)]1
TiO2/CA-9.3 15.1 84.9 0.18[thin space (1/6-em)]:[thin space (1/6-em)]1


The structure of CA-X before and after assembling TiO2 was further studied by TEM and HRTEM, and the representative images of these samples are shown in Fig. 3. It can be seen that both CA-4.3 (Fig. 3a) and CA-9.3 (Fig. 3c) exhibit disordered wormhole-like mesopore structures, which are consistent with the previous report.31 After assembling TiO2 on CA-4.3 (Fig. 3b), abundant and spherical domains (marked in the dash line frame) on several nanometer scale with clear lattice fringes of TiO2 are disorderly dispersed on the surface of CA-4.3. When comparing CA-9.3 (Fig. 3c) vs. TiO2/CA-9.3 (Fig. 3d), the pore channels of CA-9.3 are partially filled by the assembled TiO2, deduced from the variation on contrast of the two images. In addition, TiO2 particles (marked in the dash line frame) with identifiable lattice fringes are observed on the edge of CA-9.3 without serious aggregation. The TEM results further confirm that TiO2 is dispersed on outer surface of CA-4.3, while on both inner and outer surfaces of CA-9.3, which are consistent with the pore structure analysis (vide supra).


image file: c6ra08074j-f3.tif
Fig. 3 HRTEM images of (a) CA-4.3, (b) TiO2/CA-4.3, (c) CA-9.3, and (d) TiO2/CA-9.3.

Effect of porous structure and wettability on DMP adsorption

The DMP adsorption on TiO2/CA-X is evaluated by kinetic adsorption curves in Fig. 4, and the one-hour absorption amount is listed in Table 1. CA-3.1 and CA-4.3 present the similar adsorption behaviors (dashed line) with ca. 8 mg g−1 DMP amount upon one-hour absorption, which is less than the amount of 10 mg g−1 on CA-9.3. After assembling TiO2, DMP adsorption on three TiO2/CA-X samples (solid lines) decreases in different levels compared with each pristine CA-X. It decreases from 10 to 4 mg g−1 when comparing CA-9.3 with TiO2/CA-9.3, and from ca. 8 to 6 mg g−1 upon assembling TiO2 on CA-3.1 or CA-4.3. It was reported the volume of mesopores and micropores determined the adsorption of organic micro pollutants, such as microcystins by activated carbons.37,38 The total volume of micropores and mesopores for CA-3.1, CA-4.3 and CA-9.3 (listed in Table 1) is about 0.88, 0.96 and 1.2 cm3 g−1, respectively. The volume data well accounts for the similar DMP adsorption capacities of CA-3.1 and CA-4.3 and the highest adsorption amount of CA-9.3. After assembling TiO2 on CA-X, the total volume of all three samples decreases significantly to the same level of ∼0.17 cm3 g−1, as presented in Table 1. The volume decrease of all three samples are consistent with their adsorption amount decrease, but the comparable 0.17 cm3 g−1 total volume cannot explain their different adsorption capacity, e.g. 4 mg g−1 in TiO2/CA-9.3 and the 6 mg g−1 in TiO2/CA-3.1 and TiO2/CA-4.3.
image file: c6ra08074j-f4.tif
Fig. 4 The adsorption curves for DMP onto CA-X, TiO2/CA-X, and pristine TiO2.

In addition to pore volume, the wettability of adsorbent also plays a vital role on its absorption performance, for example, the hydrophilic TiO2 possesses the negligible DMP adsorption in Fig. 4. Fig. 5 presents the contact angle results and the droplet images of all samples as well. It can be seen that all CA-X samples are hydrophobic with apparent contact angles over 120°. After loading hydrophilic TiO2 with a contact angle of less than 10°, all samples change to be hydrophilic accompanying with the decrease of contact angles. Notably, TiO2/CA-9.3 shows the smallest contact angle ca. 70° in three TiO2/CA-X samples, which is consistent with its unique pore structure that hydrophilic TiO2 was dispersed on both inner and outer surface of CA-9.3. The hydrophilic nature of TiO2/CA-9.3 enables it to be more inclined to adsorb H2O but not DMP. Thus, TiO2/CA-9.3 gives the lowest DMP adsorption amount, as shown in Table 1.


image file: c6ra08074j-f5.tif
Fig. 5 Contact angle and droplet images of CA-X and TiO2/CA-X.

Photocatalytic degradation of DMP

DMP was chosen as the target pollutant to study the influence of pore structure on the photocatalytic activities of TiO2/CA-X samples. It should be noted that no DMP degradation occurred when irradiating TiO2/CA-X photocatalysts with visible light (λ > 420 nm). As previous reports,39,40 the photodegradation process in our case occurs with UV-light irradiation of photocatalysts and carbon does not sensitize TiO2, though the visible absorption related to carbon is observed in UV-vis absorption spectra (Fig. S3).

Fig. 6 shows the dynamic curves of DMP photocatalytic degradation during 3 hours. It can be seen that TiO2/CA-9.3 gives the highest degradation efficiency of 83%, and TiO2 shows the secondary degradation efficiency ca. 70%. TiO2/CA-3.1 and TiO2/CA-4.3 respectively exhibit the third and fourth degradation efficiency of 55% and 44%, which are followed by the mechanical mixture of TiO2 and CA-9.3 with 25% efficiency.


image file: c6ra08074j-f6.tif
Fig. 6 Dynamic curves of photocatalytic degradation DMP with TiO2/CA-X, TiO2 and TiO2 + CA-9.3.

The intermediates in DMP degradation process are identified from positive modes of MS (Fig. S4). The signal at m/z = 195 (+H) which belongs to DMP has been strongly weakened and two major intermediates were formed according to the signals in the mass spectra. The signals at m/z = 149 (+H) and 171 (+Na) might belong to o-phthalic anhydride. The signal at m/z = 167 (+H) might be phthalic acid. The similar intermediates were observed by Wang et al.3

Photocatalytic activity is acknowledged to rely on the adsorption capacity of organic molecules upon photocatalyst, and high adsorption capacity is favorable for the photocatalytic degradation due to the accumulation of organic molecules and the intermediates, if any.41 However, in our case, the high adsorption amount of DMP in TiO2/CA-3.1 and TiO2/CA-4.3 did not result in high degradation efficiency. TiO2/CA-9.3, which has lowest adsorption amount of DMP, presents the highest degradation efficiency. That is, the DMP accumulation in TiO2/CA-X relying on the adsorption capacity is unessential for its photodegradation in this case.

In consideration of the similar absorption features of TiO2/CA-X in UV-vis absorption spectra (Fig. S3), the amounts of photogenerated carriers in these samples are comparable, which cannot account for such a big difference in photodegradation efficiency (see Fig. 6) as well. The HO˙ was further studied to address the difference in DMP degradation efficiency. Fig. 7 gives the EPR spectra of DMPO-OH adduct produced by in situ illuminating aqueous solutions respectively containing TiO2, TiO2/CA-9.3 and TiO2/CA-3.1. The control experiment result of DMPO aqueous solution is also shown in Fig. 7. It can be seen that TiO2/CA-9.3 exhibits the largest amount of HO˙, TiO2 gives the secondary HO˙ amount, and TiO2/CA-3.1 shows the lowest HO˙ amount. This order of HO˙ amount is consistent with the DMP degradation sequence in Fig. 6. It was reported that water treatment processes was highly dependent on hydroxyl radical and it is critical to maximize hydroxyl radical generation during TiO2 photocatalysis.4 In light of above MS results, the major intermediates should be formed by the attack of hydroxyl radicals on the alkyl chains of DMP. Therefore, we focus on the formation of HO˙ to correlate the structures of TiO2/CA-X with their photocatalytic properties hereinafter.


image file: c6ra08074j-f7.tif
Fig. 7 EPR spectra of DMPO-OH adduct in aqueous solution respectively containing TiO2, TiO2/CA-9.3 and TiO2/CA-3.1 illuminating with Xe lamp.

The mechanism of photocatalytic degradation

A typical photocatalytic process begins with the light absorption to produce electrons and holes (eqn (1)). The photogenerated holes are consumed by the oxidization of H2O to produce active HO˙ (eqn (5));42 meanwhile, the photoelectrons are consumed by O2 reduction to ˙O2− (eqn (2)), followed by the generation (eqn (3)) and decomposition (eqn (4)) of H2O2, in which process active HO˙ is also generated. It is noted that active HO˙ with strong oxidation ability leads to the fast degradation of organic molecules (eqn (6)).43
 
TiO2(surface) + → eCB + hVB+ (1)
 
eCB + O2 → ˙O2 (2)
 
˙O2 + H2O → H2O2 (3)
 
H2O2 → HO˙ + OH (4)
 
H2O + hVB+ → HO˙ + H+ (5)
 
HO˙ + C10H10O4 → H2O + CO2 (6)

In above processes, there are two ways for HO˙ formation: H2O oxidation in eqn (5) and O2 reduction with the participation of H2O in eqn (2)–(4). Most important of all, in both ways, H2O molecule is indispensable for HO˙ formation. Thus, the more hydrophilic surface in TiO2/CA-9.3 can account for its higher HO˙ generation ability than that of TiO2/CA-3.1 with hydrophobic surface. However, it is still puzzling that the HO˙ amount produced in TiO2/CA-9.3 is even larger than that in pristine TiO2, concerning the super-hydrophilic TiO2 vs. hydrophilic TiO2/CA-9.3. We propose that a structure-related effect exists in TiO2/CA-9.3 toward HO˙ generation and the mechanism of HO˙ formation on the outer and inner surfaces of TiO2/CA-9.3 is illustrated in Fig. 8 (vide infra).


image file: c6ra08074j-f8.tif
Fig. 8 Schematic illustration of DMP degradation in TiO2/CA-9.3 under light irradiation. The red ring describes the reactions occurring in the secondary pores. The processes include: (I) on the external surface, HO˙ formation with H2O reduction and oxidation, (II) the photoelectrons generated on external surface migrates to the internal surface through the carbon layer, (III) on the internal surface, the photoelectrons are trapped by O2 to produce ˙O2−, (IV) HO˙ are generated with the participation of H2O and ˙O2−, (V) DMP is oxidized by active HO˙ on both external and internal surface.

It is understandable that the primary factor inhibiting HO˙ formation via either the oxidation way (eqn (5)) or reduction way (eqn (2)–(4)) is the recombination of photoholes and photoelectrons in the photodegradation process. With respect to the special structure of TiO2/CA-9.3 with TiO2 dispersed on both inner and outer surfaces, it is possible that the photoelectrons generated on the outer surface transfer to its inner surface through the conductive CA (process II in Fig. 8). This process potentially increases the separation efficiency of photoelectrons and photoholes. As a result, HO˙ formation via H2O oxidation with photoholes (eqn (5)) is enhanced on the outer surface TiO2 (process I in Fig. 8). Meanwhile, the formation of HO˙ via O2 reduction with participation of H2O and photoelectrons (eqn (2)–(4)) is improved in the hydrophilic secondary channels of TiO2/CA-9.3 (process IV in Fig. 8 amplifying red-circle region), because in this secondary channels the three integral components of photoelectrons, O2 and H2O needed for HO˙ formation are simultaneously satisfied with the photoelectrons transfer aforementioned, air bubbling in aqueous solution, and surface hydrophilic property, respectively. In addition, the spatial confinement effect44,45 arising from narrower secondary channel further facilitates the HO˙ formation by stabilizing the intermediates of ˙O2− and H2O2. In summary, the interface electron transfer between TiO2 and CA-9.3 promotes the spacial separation of photoelectrons and photoholes, and hydrophilic secondary-pore surface with confined space results in the increase of HO˙ formation possibility in reduction way (eqn (2)–(4)), and thereby leads to the highest DMP degradation activity of TiO2/CA-9.3 (process V in Fig. 8).

Comparing with TiO2/CA-9.3 with uniform distribution of TiO2 on both outer and inner surface of CA-9.3 support, prepared by introducing CA-9.3 into titanium precursor solution prior to sol–gel formation, TiO2 + CA-9.3 is a simply mixture of TiO2 and CA-9.3 and no hydrophilic porous structure exists, in addition, part of CA-9.3 covering on TiO2 could block the incident light by its self-absorption. Therefore, the degradation activity of TiO2 + CA-9.3 is far lower than TiO2/CA-9.3, even lower than TiO2/CA-3.1 and TiO2/CA-4.3, where TiO2 mainly dispersed on the outer surface of CA supports as their small pore diameter.

Conclusions

TiO2/CA-X photocatalysts with variable pore structures were fabricated and the correlation between the pore structure and the photocatalytic property was systematically studied. Our date indicates that dispersion of TiO2 on CA-X relies on the pore diameter of CA support. The large diameter enables TiO2 to be dispersed on both inner and outer surface of CA support, accompanying with the formation of the secondary pore with narrower channel. This special porous structure of TiO2/CA-9.3 leads to the separation of electrons and holes in space in the photocatalytic process. Correspondingly, the two routes of HO˙ formation in H2O oxidation and O2 reduction with participation of H2O are promoted. The largest amount HO˙ finally causes the highest DMP degradation efficiency in TiO2/CA-9.3. It was concluded that the surface/interface synergy effect plays a positive role on the spatial separation and utilization of electrons and holes in photocatalytic process, which suggests a potential strategy for designing high efficiency photocatalysts.

Experimental

Materials

Titanium(IV) isopropoxide (95%) and tetraethyl orthosilicate (TEOS, 98%) were purchased from Aladdin (Shanghai, China). Other reagents used were all analytical reagents and purchased from Guangzhou Chemical Reagent Plant (Guangzhou, China). All reagents were used as received without further purification, and the double distilled water was used in all experiments.

Preparation

The carbon aerogels were synthesized following a previously published procedure.31 Briefly, the raw materials of glucose (2 g), tetraethyl orthosilicate (TEOS, 3 mL) and sulfuric acid (H2SO4) solution (4 mL, pH = 2) were mixed and stirred until a homogenate was formed. The mixture was then treated by hydrofluoric acid (HF, 4 wt%) under stirring, gelated, and aged in a plastic bottle as follows: 40 °C for 2 days, followed by 100 °C for 6 h, and finally 160 °C for 6 h. The xerogel was subsequently carbonized in nitrogen atmosphere at 900 °C for 3 h, and washed by 40 wt% HF to remove silica. The HF/TEOS molar ratio used was 0, 1/30 and 1/7, and as a result, the pore diameters were controlled by changing the amount of HF during the sol–gel process of TEOS. The notation of “CA-X” is used to denote the samples, with X being the pore diameter of CA calculated by the density function theory (DFT) model. The TiO2/CA-X sample was synthesized with CA-X as the support material.

TiO2/CA-X samples were prepared by a sol–gel method with titanium isopropoxide as Ti source. A typical procedure is as follows. Titanium(IV) isopropoxide (3 mL) was introduced into ethanol (20 mL) with vigorous stirring for 30 min, and then concentrated nitric acid (0.16 mL) was added into this solution. After stirring for 5 minutes, CA (0.16 g) was distributed into this solution. The mixture solution was constantly stirred until a homogenous CA-contained gel was formed. The gel was aged in air to form a ergoes, which was then ground into fine powder. The powder was calcined at 400 °C for 5 h in the nitrogen atmosphere, and TiO2/CA-X samples were thus obtained. For comparison, pure TiO2 was also prepared following the same procedure in the absence of CA. Mechanically mixed TiO2 and CA-X sample with the same mass ratio as TiO2/CA-X samples, marked as TiO2 + CA-9.3 was also prepared.

Characterization

The crystalline structures of TiO2/CA-X samples were analyzed by D8 Advance X-ray Diffractometer (XRD, Bruker, D8 advance, Germany) with Cu-Kα radiation source at scanning rate of 10 min−1. The morphologies of TiO2/CA-X samples were observed by transmission electron microscope (TEM, JEOL, JEM-2100, Japan) on a JEM 2100F 200 kV field emission transmission electron microscope. The carbon content in TiO2/CA-X samples was determined by thermogravimetry analysis (TG, Netzsch, TG209, Germany) in air atmosphere. The pore structures of samples were probed by N2 adsorption–desorption isotherm at 77 K (Quantachrome, AutosorbiQ, American). Before measurement, the samples were out-gassed at 200 °C for 12 h. The specific surface area was determined by Brunauer–Emmett–Teller (BET) model, while the pore size and volume were calculated by density functional theory (DFT) method on Quantachrome ASiQwin software. Diffuse reflection spectra (DSR) were recorded on UV-vis spectrophotometer (Shimadzu, UV-3150, Japan, equipped with an integrating sphere) to study the optical properties of the samples.

Electron Paramagnetic Resonancse spectrometer (EPR, Bruker, A 300, Germany) were used to detect the hydroxyl radical with 5,5-dimethy-1-pyrroline-N-oxide (DMPO, Sigma-Aldrich) as the radical trap. The samples were irradiated with xenon arc source system (LOT Oriel 75-150, UK). Data acquisition parameters were as follows: magnetic field, 3514 G; microwave power, 5.95 mW; modulation frequency, 100 kHz; modulation amplitude, 1.00 G; microwave frequency, 9.86 GHz; sweep time, 20.48 s. The hydrophilic properties of CA-X and TiO2/CA-X were measured by OCA contact angle system (Dataphysics, OCA20, Germany). The intermediates in the degradation process were identified from positive modes of MS (AB Sciex, triple QuadTM 4500).

Adsorption and photocatalytic degradation of DMP

Dimethyl phthalate (DMP, 2 mg L−1) was chosen as the model target to investigate the photocatalytic properties of porous TiO2/CA-X samples. Prior to the photocatalytic reaction, the adsorption experiment of DMP on TiO2/CA-X was carried out in dark at room temperature by adding 0.01 g of TiO2/CA-X sample into 100 mL 2 mg L−1 DMP aqueous solution. The photodegradation experiments were carried out in a cylindrical glass reactor (Φ 9.0 cm × 10.6 cm) covered by a cylindrical quartz vessel (Φ 9.0 cm × 9.0 cm), which was full-filled with double distilled water to remove the infrared light radiated from 300 W Xe lamp (Changtuo, PLS-SXE 300/300 UV, Beijing). The light intensity was 85 mW cm−2 determined by a radiometer (FZ-A, Photoelectric Instrument factory of Beijing Normal University). The emission spectrum of the Xe lamp has been reported in ref. 8. For a typical photocatalytic experiment, 0.1 g L−1 of TiO2/CA-X catalysts were firstly pre-adsorbed with 100 mL 2 mg L−1 DMP in dark before irradiation to establish adsorption–desorption equilibrium. Then photocatalytic experiments were initiated by air bubbling and irradiation. During the experiments, 0.5 mL of solution was sampled at preset time interval for the analysis of the concentration of DMP by high performance liquid chromatography (HPLC, Techcomp, LC2130, Shanghai, China) equipped with a reverse phase column (Waters, XT erra MS C-18, 5 μm) and a UV detector. The mobile phase was composed of 50% acetonitrile and 50% water, and the detection wavelength was 276 nm. For comparison, pristine TiO2 and mechanical mixtures of TiO2 and CA-9.3 (TiO2 + CA) were also tested under the same condition. The amount of TiO2 was to the same as that in TiO2/CA-X.

Acknowledgements

The research was financially supported by the 973 Program (2014CB845600), NSFC (No. 21103235), NSF of Guangdong Province (No. S2012010010775), the Key Laboratory of Fuel Cell Technology of Guangdong Province, and the Key Laboratory of Environmental Pollution Control and Remediation Technology of Guangdong Province (No. 2011K0011). JZZ is grateful to the BES Division of the US DOE for financial support.

References

  1. Y. C. Chung and C. Y. Chen, Water, Air, Soil Pollut., 2009, 200, 191–198 CrossRef CAS.
  2. Y. H. Chen, L. L. Chen and N. C. Shang, J. Hazard. Mater., 2009, 172, 20–29 CrossRef CAS PubMed.
  3. W. C. Liao and P. Wang, J. Braz. Chem. Soc., 2009, 20, 866–872 CrossRef CAS.
  4. W. J. Jiang, J. A. Joensa, D. D. Dionysiou and K. E. O' Shea, J. Photochem. Photobiol., A, 2013, 262, 7–13 CrossRef CAS.
  5. Z. J. Huang, P. X. Wu, Y. H. Lu, X. R. Wang, N. W. Zhu and Z. Dang, J. Hazard. Mater., 2013, 246–247, 70–78 CrossRef CAS PubMed.
  6. Y. Jing, L. S. Li, Q. Y. Zhang, P. Lu, P. H. Liu and X. H. Lu, J. Hazard. Mater., 2011, 189, 40–47 CrossRef CAS PubMed.
  7. L. Xu, X. Yang, Y. H. Guo, F. Y. Ma, Y. N. Guo, X. Yuan and M. X. Huo, J. Hazard. Mater., 2010, 178, 1070–1077 CrossRef CAS PubMed.
  8. J. Y. Shi, H. N. Cui, Z. X. Liang, X. H. Lu, Y. X. Tong, C. Y. Su and H. Liu, Energy Environ. Sci., 2011, 4, 466–470 CAS.
  9. D. Zhao, C. C. Chen, Y. F. Wang, H. W. Ji, W. H. Ma, L. Zang and J. C. Zhao, J. Phys. Chem. C, 2008, 112, 5993–6001 CAS.
  10. S. G. Bairu, E. Mghanga, J. Hasan, S. Kola, V. J. Rao, K. Bhanuprakash, L. Giribabu, G. P. Wiederrecht, da. R. Silva, L. G. C. Rego and G. Ramakrishna, J. Phys. Chem. C, 2013, 117, 4824–4835 CAS.
  11. M. Garcia-Mota, A. Vojvodic, F. Abild-Pedersen and J. K. Norskov, J. Phys. Chem. C, 2013, 117, 460–465 CAS.
  12. R. Leary and A. Westwood, Carbon, 2011, 49, 741–772 CrossRef CAS.
  13. C. Pelekani and V. L. Snoeyink, Water Res., 1999, 33, 1209–1219 CrossRef CAS.
  14. X. W. Zhang, M. H. Zhou and L. Lei, Carbon, 2005, 43, 1700–1708 CrossRef CAS.
  15. Y. H. Ao, J. J. Xu, D. G. Fu, X. W. Shen and C. W. Yuan, Colloids Surf., A, 2008, 312, 125–130 CrossRef CAS.
  16. H. Zhang, X. J. Lv, Y. M. Li, Y. Wang and J. H. Li, ACS Nano, 2010, 4, 380–386 CrossRef CAS PubMed.
  17. H. Y. Ng, S. Ikeda, M. Matsumura and R. Amal, Energy Environ. Sci., 2012, 5, 9307–9318 Search PubMed.
  18. W. D. Wang, C. G. Silva and J. L. Faria, Appl. Catal., B, 2007, 70, 470–478 CrossRef CAS.
  19. W. Wei, C. Yu, Q. F. Zhao, G. S. Li and Y. Wan, Chem.–Eur. J., 2013, 19, 566–577 CrossRef CAS PubMed.
  20. Y. Yao, G. Li, S. Ciston, R. M. Lueptow and K. A. Gray, Environ. Sci. Technol., 2008, 42, 4952–4957 CrossRef CAS PubMed.
  21. X. H. Xia, Z. H. Jia, Y. Yu, Y. Liang, Z. Wang and L. L. Ma, Carbon, 2007, 45, 717–721 CrossRef CAS.
  22. L. Gu, Z. X. Chen, C. Sun, B. Wei and X. Yu, Desalination, 2010, 263, 107–112 CrossRef CAS.
  23. M. F. Wu, Y. N. Jin, G. H. Zhao, M. F. Li and D. M. Li, Environ. Sci. Technol., 2010, 44, 1780–1785 CrossRef CAS PubMed.
  24. D. Wang, G. H. Yang, Q. X. Ma, M. B. Wu, Y. S. Tan, Y. Yoneyama and N. Tsubaki, ACS Catal., 2012, 2, 1958–1966 CrossRef CAS.
  25. H. Q. Yang, L. Zhang, L. Zhong, Q. H. Yang and C. Li, Angew. Chem., Int. Ed., 2007, 46, 6861–6865 CrossRef CAS PubMed.
  26. Z. J. Chen, X. H. Li and C. Li, Chin. J. Catal., 2011, 32, 155–161 CAS.
  27. W. Chen, Z. L. Fan, B. Zhang, G. J. Ma, K. Takanabe, X. X. Zhang and Z. P. Lai, J. Am. Chem. Soc., 2011, 133, 14896–14899 CrossRef CAS PubMed.
  28. Y. N. Jin, M. F. Wu, G. H. Zhao and M. F. Li, Chem. Eng. J., 2011, 168, 1248–1255 CrossRef CAS.
  29. J. M. Miller and B. Dunn, Langmuir, 1999, 15, 799–806 CrossRef CAS.
  30. H. D. Du, L. Gan, B. H. Li, P. Wu, Y. L. Qiu, F. Y. Kang, R. W. Fu and Y. Q. Zeng, J. Phys. Chem. C, 2007, 111, 2040–2043 CAS.
  31. D. C. Wu, Z. H. Li, Y. R. Liang, X. Q. Yang, X. H. Zeng and R. W. Fu, Carbon, 2009, 47, 916–918 CrossRef CAS.
  32. U. Heudorf, V. Mersch-Sundermann and E. Angerer, Int. J. Hyg. Environ. Health, 2007, 210, 623–634 CrossRef CAS PubMed.
  33. S. Takeuchi, M. Iida, S. Kobayashi, K. Jin, T. Matsuda and H. Kojima, Toxicology, 2005, 210, 223–233 CrossRef CAS PubMed.
  34. Z. Y. Ryu, J. T. Zheng, M. Z. Wang and B. J. Zhang, Carbon, 1999, 37, 1257–1264 CrossRef CAS.
  35. M. L. Occelli, J. P. Olivier, J. A. Perdigon-Melon and A. Auroux, Langmuir, 2002, 18, 9816–9823 CrossRef CAS.
  36. J. H. Park, S. K. Kim, H. S. Kim, Y. J. Cho, J. Park, K. E. Lee, C. W. Yoon, S. W. Nam and S. O. Kang, Chem. Commun., 2013, 49, 10832–10834 RSC.
  37. C. Donati, M. Drikas, R. Hayes and G. Newcombe, Water Res., 1994, 28, 1735–1742 CrossRef CAS.
  38. P. Pendleton, R. Schumann and S. H. Wong, J. Colloid Interface Sci., 2001, 240, 1–8 CrossRef CAS PubMed.
  39. A. L. Linsebiger, G. Q. Lu and J. T. Yates Jr, Chem. Rev., 1995, 95, 735–758 CrossRef.
  40. S. Sakthivel, M. C. Hidalgo, D. W. Bahnermann, S. U. Geissen, V. Murugesan and A. Vogelpohl, Appl. Catal., B, 2006, 63, 31–40 CrossRef CAS.
  41. J. H. Im, S. J. Yang, C. H. Yun and C. R. Park, Nanotechnology, 2012, 23, 035604 CrossRef PubMed.
  42. M. R. Hoffmann, S. T. Martin, W. Choi and D. F. Bahnemann, Chem. Rev., 1995, 95, 69–96 CrossRef CAS.
  43. J. H. Sun, X. L. Wang, J. Y. Sun, R. X. Sun, S. P. Sun and L. P. Qiao, J. Mol. Catal. A: Chem., 2006, 260, 241–246 CrossRef CAS.
  44. J. Shi, Chem. Rev., 2013, 113, 2139–2181 CrossRef CAS PubMed.
  45. I. J. Morales, J. S. González, P. M. Torres and A. J. López, Appl. Catal., B, 2011, 105, 199–205 CrossRef.

Footnote

Electronic supplementary information (ESI) available: The thermogravimetry (TG), differential thermal gravity (DTG), X-ray diffraction and UV-vis absorption spectra for all samples. See DOI: 10.1039/c6ra08074j

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