R. Jusoha,
A. A. Jalil*ab,
S. Triwahyonoc and
N. H. N. Kamarudina
aDepartment of Chemical Engineering, Faculty of Chemical Engineering, Universiti Teknologi Malaysia, 81310 UTM Johor Bahru, Johor, Malaysia. E-mail: aishah@cheme.utm.my
bInstitute of Hydrogen Economy, Universiti Teknologi Malaysia, 81310 UTM Johor Bahru, Johor, Malaysia
cDepartment of Chemistry, Faculty of Science, Universiti Teknologi Malaysia, 81310 UTM Johor Bahru, Johor, Malaysia
First published on 5th January 2015
Dual type Fe species (isomorphously substituted Fe species and a colloidal α-FeOOH (IS-FeOOH)) supported on mesostructured silica nanoparticles (IS-FeOOH/MSN) were prepared by a simple electrochemical method followed by impregnation. Characterization was conducted using X-ray diffraction, transmission electron microscopy, surface area analysis, Fourier-transform infrared spectroscopy, nuclear magnetic resonance, electron spin resonance, and X-ray photoelectron spectroscopy. The results suggested that silica removal occurred in the MSN framework to isomorphously substitute Fe cations while retaining the colloidal structure of IS-FeOOH. The catalytic activity of IS-FeOOH/MSN was tested on photo-Fenton-like degradation of 2-chlorophenol under fluorescent light irradiation. The performance of the catalyst was in the following order: 10 wt% IS-FeOOH/MSN > 15 wt% IS-FeOOH/MSN > 5 wt% IS-FeOOH/MSN > MSN, with removal percentages of 92.2, 79.3, 73.1, and 14.2%, respectively. The results suggest that a synergistic effect between the dual type of Fe species (Si–O–Fe and IS-FeOOH colloid) and MSN played important roles in enhancing the degradation. The results provide strong evidence to support the potential use of IS-FeOOH/MSN as a photo-Fenton-like nanocatalyst for organic pollutants treatment.
α-FeOOH has been widely used as a semiconductor catalyst for degradation of many chlorinated compounds owing to its unique electrical, optical, and photoluminescence properties with a low band-gap energy (2.2 eV).6,7 However, α-FeOOH nanoparticles have small surface areas that cause poor photocatalytic performances due to insufficient contact with the reactants.8 Thus, a suitable method to improve the contact between pollutant molecules and a catalyst with low usage of metal oxide in the treatment system should be investigated. One method is an incorporation of the metal oxide onto mesoporous materials support, which has been discussed by several research groups in recent years.9–11 For instance, mesostructured silica nanoparticles (MSN) is the most popular and has been considered as a potential solid support for heterogeneous catalysts.12
Recently, we have reported the effective use of modified MSN in drug delivery system, adsorption, isomerization, and photocatalysis,13–18 which related to its distinctive properties such as ordered porous structure, high surface area (>1000 m2 g−1), large pore volume, and tunable pore size (1.5–10 nm). On the other hand, we also reported a simple electrosynthesis of colloidal α-FeOOH nanoparticles in ionic surfactant (IS), which inhibited the electron–hole recombination to enhance the photodegradation of 2-CP.19 However, the result is still low and beyond the industrial requirement. Therefore, incorporation of the colloidal metal onto a support material is very decisive. Although several studies have been conducted to deposit the colloidal metal onto several supports including clay, metal oxide, and activated carbon,20–22 the study on the interaction of electrosynthesized colloidal metal oxide on a mesostructured silica nanoparticles support is still rare. Moreover, the properties of the catalyst are known to be strongly affected by the support, which makes it very complicated to understand its reaction mechanism. Thus, detail investigation on supported colloidal metal catalyst is very crucial.
Therefore, herein we report a synthesis of IS-FeOOH supported on MSN in order to enhance the surface contact for an efficient photodegradation. The physicochemical properties of the IS-FeOOH/MSN were studied in detail to clarify its structure. Remarkably, it was found that besides the retainment of IS-FeOOH colloidal structure, the isomorphously substituted Fe species was also formed. This dual types Fe species are synergically performed with MSN support to significantly give almost complete photo-degradation of 2-CP.
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0.1. After 30 min vigorous stirring with heating, 1.2 mmol TEOS were added to give a white suspension solution. This solution was stirred for another 2 h, followed by centrifugation, drying at 333 K and calcined at 823 K for 3 h.
The synthesis procedure of α-FeOOH nanoparticles were similar to those reported in literature.15,16,19 15 mL IS/water solution, with IS to water of 1
:
1 volume ratio was added to one-compartment cell equipped with magnetic stirring bar and a two-electrode configuration of an iron plate (2 cm × 2 cm) anode and a platinum plate (2 cm × 2 cm) cathode. Electrolysis was conducted at a constant current of 60 mA cm−2 and 273 K under air atmosphere. The weight percentage of IS-FeOOH supported on MSN was calculated by the time of electrolysis, which is based on the Faraday's law (eqn (1)),
![]() | (1) |
486 C mol−1, which is the Faraday constant; I is the electric current applied (mA); z is the valency number of ions of substance (electrons transferred per ion); and n is the number of moles of substance (number of moles, liberated n = m M−1). After electrolysis of prescribe weight percentage of IS-FeOOH, the corresponding mixture was impregnated to MSN at 353 K to give a series of IS-FeOOH/MSN.
Surface area of IS-FeOOH/MSN was calculated with Brunnauer–Emmett–Teller (BET) method using a Micromeritics ASAP 2010 instrument. The functional groups of IS-FeOOH/MSN were identified using an Agilent Cary 640 Fourier-transform infrared (FT-IR) Spectrometer using the KBr method with a scan range of 400–4000 cm−1.
29Si MAS NMR spectra were recorded on a Bruker Advance 400 MHz 9.4 T spectrometer at frequency of 104.2 MHz and 79.4 MHz, respectively. A JEOL JES-FA100 ESR spectrometer was used to observe the formation of electron–holes or unpaired electrons at room temperature. Chemical oxidation state of the IS-FeOOH/MSN catalyst was determined using XPS conducted on a Kratos Ultra spectrometer equipped with a Mg Kα radiation source (10 mA, 15 kV) in the range of 0–800 eV. Photo-luminescence (PL) (JASCO Spectrofluorometer) (FP-8500) with 150 W Xe lamp as excitation source were employed to study the electronic structure, optical and photochemical properties of semiconductor.
The analysis regarding the optical absorption properties of the catalysts were obtained using a PerkinElmer UV-vis/DRS Spectrophotometer in the range of 200–800 nm at room temperature. The band gap of catalysts was determined from plots of the Kubelka–Munk (K–M) function [fK–M = (hν/λ)1/2] as a function of the energy of the excitation light [hν].
The entire set-up was placed inside a chamber covered with aluminium foil to prevent the passage of other lights. Initial pH of the solution was 5 and the reaction was carried out at 303 K. Then 0.156 mM hydrogen peroxide (H2O2) was added and ambient air was bubbled into the system continuously using an air pump (AC 100–240 V, 12 W motor) before the reaction was performed for another 8 h under UV-Vis light irradiation. During the reaction, aliquots of 2 mL were taken out at 15 min intervals and centrifuged in a Hettich Zentrifugen Micro 120 at 75
000 rpm for 10 min before analysis by a double-beam UV-Vis spectrophotometer (Cary 60 UV-Vis Agilent) at 274 nm. All experiments were performed in triplicate; error bars represent standard error of the mean.
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| Fig. 1 XRD patterns of catalysts. (A) Region 15–65° of IS-FeOOH; (B) region 2–10° of MSN and IS-FeOOH/MSN. | ||
Insight at higher magnification (Fig. 2C) showed that the deposited IS-FeOOH did not fuse into larger particles and retained its original particle size (5–10 nm) (ESI Fig. S1†), signifying a high stability even after introduction onto the MSN support. The average particle-to-particle distance (dpp) measured was 2 ± 0.5 nm, shorter than twice the length of the IS molecule, which is 3.6 nm. This may suggest a retained colloidal structure around the α-FeOOH on the MSN support.27 The value of the interplanar distance (d-spacing) of the lattice fringes estimated from the magnification of a selected area was 0.403 nm and it was consistent with the value of lattice spacing of IS-FeOOH obtained from the XRD analysis at (110) facet (Fig. 2D).
As shown in Table 1, surface area (SBET) of IS-FeOOH/MSN decreased from 1107 to 665 m2 g−1, following the order MSN > 5 wt% IS-FeOOH/MSN > 10 wt% IS-FeOOH/MSN > 15 wt% IS-FeOOH/MSN. This suggested that a portion of the IS-FeOOH was dispersed on the surface of MSN. Average pore size of MSN was found to be increased upon the introduction of IS-FeOOH, that might be due to the increase in interparticle pores, as shown in Fig. 3. Indeed, formation of a bimodal pore structure may be related to the removal of silica from MSN framework.28 Increasing the amount of IS-FeOOH loaded may induce the silica removal rate, which then led to the reduction in pore size and increase in pore volume of the MSN.29
| Sample | Surface area, SBET (m2 g−1) | Average pore size, Dpore (nm) | Average pore volume, Vpore (cm3 g−1) |
|---|---|---|---|
| MSN | 1107 | 3.00 ± 1.20 | 2.14 |
| 5 wt% IS-FeOOH/MSN | 850 | 3.10 ± 1.14 | 0.61 |
| 10 wt% IS-FeOOH/MSN | 734 | 3.09 ± 1.27 | 1.04 |
| 15 wt% IS-FeOOH/MSN | 665 | 3.01 ± 1.19 | 0.99 |
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| Fig. 4 FT-IR spectra of catalysts. (A) Region 3800–2700 cm−1; (B) region 1800–1360 cm−1; (C) region 1300–400 cm−1; (D) in evacuated system for region 3770–3700 cm−1. | ||
Fig. 4B shows a broad band at 1621 cm−1 in all samples, which attributed to the bending vibration of the OH group for both IS-FeOOH and MSN.30 Doublet peaks observed at band 1480 and 1465 cm−1 in the IS-FeOOH spectrum correspond to the CH2 scissoring mode of the IS methylene chain.31 These bands were significantly observed in IS-FeOOH/MSNs, suggesting the presence of colloidal IS-FeOOH. The peak at 1430 cm−1, which corresponds to head group vibrations of the IS, was observed for all samples.19 This implies that the interaction of N+ with IS-FeOOH is retained for all samples.
The bands at 1090, 790, and 455 cm−1 for MSN and IS-FeOOH/MSN catalysts shown in Fig. 4C are attributed to the characteristics of the silica structure of asymmetric stretching, symmetric stretching, and bending vibration of Si–O–Si bonds, respectively.32 The introduction of IS-FeOOH species onto MSN decreased the intensity of all bands, implying a perturbation of silica network due to removal of silica. Meanwhile, the slight shift of the 790 cm−1 band to 775 cm−1 may be attributed to the vibration of Fe3+–OH, which illustrates the formation of OH layer around the metal core.33 The vibrational mode at around 960 cm−1 is attributed to silanol groups present at “defective sites”.32 The decrease of this band with increasing IS-FeOOH loading also signifies its possible interaction with Fe species. Furthermore, the band at 550 cm−1, which corresponds to Si–O bond,34 was also decreased with increasing IS-FeOOH loading, indicating significant interaction of silica framework with Fe species from IS-FeOOH.
For further investigation of IS-FeOOH/MSN structural properties, the catalysts were evacuated for 1 h at 623 K prior to IR measurement to remove the physisorbed water. In Fig. 4D, a new band at 3750 cm−1 appeared in all IS-FeOOH/MSN samples which attributed to the germinal silanol groups.35 The band at 3740 cm−1, which is ascribed to the terminal silanol groups36 decreased with increasing IS-FeOOH loading, which confirmed the perturbation of silica framework. Meanwhile, the band at 3718 cm−1 which is assigned to hydroxyl nests,37 decreased with increasing IS-FeOOH loading. Thus, the results suggested that introduction of IS-FeOOH onto the MSN caused silica removal in the silica framework. It was also found that the colloidal IS-FeOOH still retain its structure after its loading onto MSN. These may due to the strong binding of IS molecules to the IS-FeOOH nanoparticles which hinder other binding displacement to its surface.38 In a mean time, the colloidal IS-FeOOH may adsorbed to the MSN surface which induced the attachment of colloidal IS-FeOOH onto the MSN support.39
Meanwhile, in order to investigate the bonding of MSN framework with the Fe species, the overlapped band at 960 cm−1 was also further confirmed by a Gaussian curve-fitting as shown in ESI (Fig. S2†). Significantly, a new band was observed at 955 cm−1 when 5 wt% IS-FeOOH was added onto the MSN, which correspond to Si–O–Fe stretching vibrations.32 The band increased by increasing IS-FeOOH loading up to 10 wt%, which confirmed the isomorphous substitution of Fe species after the removal of silica from MSN framework. This Fe species may be originated from the abundant Fe3+ ions in electrolysis cell which have not yet transformed to IS-FeOOH. However, the increase of IS-FeOOH loading up to 15 wt% showed no further increase in the band. This may be due to the saturation of Fe species–MSN interactions. The result also illustrated that the isomorphously substituted Fe species was not from the bulky colloidal structure of IS-FeOOH.
SiO)4Si. This peak reduced and shifted to −105.110 by the loading of IS-FeOOH, indicating the alteration at (
SiO)4Si sites.
New shoulders were developed in the range of −80 to −90 ppm and −90 to −100 ppm, which signified that the (
SiO)2Si and (
SiO)3Si sites were formed in consequence of silica removal in MSN framework.26 This result is consistent with XRD and FTIR, which support the decreased of Si–O–Si bonds. In fact, the silica removal that occurred may be due to the presence of ammonium salt in the synthesis process.40 The interaction between ammonium ions and silica followed by subsequent attack of the hydroxide ions on the external surface of MSN may dissociate some Si–O–Si bonds from the framework.
The 10 wt% IS-FeOOH/MSN catalyst was then subjected to XPS analysis in order to elucidate its exact structure. The Fe2p doublet with binding energies of 708 and 722 eV shown in Fig. 5C implied the presence of Fe–O bond of the IS-FeOOH species.44 Meanwhile, the three peaks at 527, 530, and 533 eV displayed by the O1s (Fig. 5D) correspond to the presence of Si–O–Si, Si–O–Fe and Si–O–H bonds, respectively, since the binding energy of electrons at the oxygen atom increases as the electron–electron repulsion decreases due to the electronegativity sequence of its adjacent atom: hydrogen > iron > silica.45 Therefore, it was confirmed that Si–O–Fe groups were present in the IS-FeOOH/MSN catalyst and this was in agreement with FTIR results.
The IS-FeOOH/MSN catalysts were also subjected to photoluminescence (PL) analysis at an excitation wavelength of 650 nm in visible region (Fig. 8). 5 wt% IS-FeOOH/MSN showed highest peak intensity, followed by the 15 wt% and 10 wt% IS-FeOOH/MSN. Addition of IS-FeOOH decreased the content of surface oxygen vacancies and/or defect sites, which affected the intensity and response range of PL signals.46 Indeed, the oxygen vacancies and defect sites are important to trap the electrons to keep the e−–h+ pairs separate in order to enhance photocatalytic activity. It has been reported that the lower the peak intensity, the lower the recombination rate of the photoinduced electron–hole pair, which results in higher photocatalytic activity.15 This fact may explain why the photocatalytic activity was in the following order: 10 wt% IS-FeOOH/MSN > 15 wt% IS-FeOOH/MSN > 5 wt% IS-FeOOH/MSN. The limitation of increasing IS-FeOOH loading to 15 wt% may be because of the accumulation of excess IS-FeOOH on the surface of the IS-FeOOH/MSN catalysts, which led to the lower rate constant and photoactivity.41
This result is in agreement with the band gap determination results shown in Table 2. The band gap energy of IS-FeOOH and IS-FeOOH/MSNs was determined using Kubelka–Munk (K–M) spectrum. The results show a reduction in band gap energy with increase in IS-FeOOH loading up to 15 wt%. It was known that low band gap energy results in efficient performance of photocatalyst. However, the aforementioned possibility of the IS-FeOOH accumulation on 15 wt% IS-FeOOH/MSN surface may hinder its effective performance towards the 2-CP degradation, regardless of the low band gap energy value.
Fig. 9A shows that PD reduced the degradation efficiency to 59%. The addition of IP and PI decreased the 2-CP degradation efficiency to 16% and 18%, respectively, while the addition of SO fully inhibited the degradation efficiency, confirming that photogenerated hole was the main oxidation species for degrading 2-CP and significantly assisted by hydroxyl radicals (˙OH) and hydroxyl radicals adsorbed on the catalyst surface (˙OHads).
As proposed in Fig. 9B, both type of the iron species played role in the photocatalytic process. The IS-FeOOH could trap the photogenerated electron by the colloidal structure around the IS-FeOOH. Meanwhile, the substituted Fe species may inhibit the electron–hole recombination by transferring the photoinduced electron to the support as MSN could also acts as stable electron acceptors.49
As proven by SO, the photogenerated holes (h+VB) at the valence band, which have high oxidation potential, play two important roles in this degradation. Firstly, they permit the direct oxidation of 2-CP to reactive intermediates (eqn (2)):
| 2-CP + h+VB → oxidation of 2-CP | (2) |
Secondly, h+VB also react with surface-adsorbed hydroxyl groups (OH−) or water to yield surface-adsorbed hydroxyl radicals (˙OHads), which subsequently degrade the 2-CP, as shown by the decrease in degradation efficiency by PI47 (eqn (3)):
| OH− + h+VB → ˙OHads | (3) |
The addition of IP showed a rather lower degradation percentage, indicating a significant role of ˙OH in the system. In fact, ˙OH could be generated via direct photoconversion of H2O2 (eqn (4)) or by photogenerated electron-induced multistep reduction of O2 (eqn (5)–(7)) to degrade the 2-CP:50
![]() | (4) |
| O2 + e− → ˙O2− | (5) |
| ˙O2− + e− + 2H+ → H2O2 | (6) |
| H2O2 + e− → OH− + ˙OH | (7) |
In the case of PD, although the photo-induced electrons at the conduction band have been captured by PD, ˙OH could still be produced by direct photoconversion of H2O2 (eqn (4)). Therefore, this mechanism demonstrates the significant role of the silica support as an acceptor of photo-induced electrons to efficiently inhibit the recombination of electron–hole pairs that leads to enhanced degradation of 2-CP.
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| Fig. 10 Stability of 10 wt% IS-FeOOH/MSN catalyst after subsequent reactions [pH 5; H2O2 concentration is 0.156 mM, catalyst dosage 0.40 g L−1; initial concentration is 50 mg L−1]. | ||
The performance of IS-FeOOH/MSN was investigated for 2-CP UV-Vis light degradation. Previous report on the supported colloidal metal indicates that the presence of ionic surfactant in the catalyst system decreased the catalyst activity for gas-phase reaction.39 This study, however, indicates that the retention of colloidal metal over MSN support could trap the photogenerated electron. In the meantime, the substituted Fe species (Si–O–Fe) may inhibit the electron–hole recombination by transferring the photoinduced electron to the MSN support.49 The synergic effect between the dual types Fe species with the MSN was able to occur in regards to the support material that acts as a stable electron acceptor. The stability test shows that the IS-FeOOH/MSN catalyst is stable up to five cycles. Ferroudj and his co-workers has synthesized similar catalyst which is a maghemite iron supported on a silica and was shown to remarkably degrade dyes and nitrophenol.52 Meanwhile, a catalyst consists of iron species and MCM-41 as a support material was synthesized by Li and co-workers for desulfurization of dibenzothiphene.41 Both Ferroudj et al. and Li et al. reported high stability upon catalyst reusability up to 5 and 4 cycles, respectively, which is comparable with the reusability result of the catalyst in this study. It is believed that these IS-FeOOH/MSN catalysts may provide assistance in the development of colloidal properties in solid catalysts for various applications.
Footnote |
| † Electronic supplementary information (ESI) available. See DOI: 10.1039/c4ra13837f |
| This journal is © The Royal Society of Chemistry 2015 |