Environ. Sci. Technol. 2008, 42, 4540–4545 AgNO3-Induced Photocatalytic Degradation of Odorous Methyl Mercaptan in Gaseous Phase: Mechanism of Chemisorption and Photocatalytic Reaction T O N G - X U L I U , †,‡ X I A N G - Z H O N G L I , * ,† AND FANG-BAI LI‡ Department of Civil and Structural Engineering, The Hong Kong Polytechnic University, Kowloon, Hong Kong, and Guangdong Key Laboratory of Agricultural Environment Pollution Integrated Control, Guangdong Institute of Eco-Environment and Soil Science, Guangzhou 510650, People’s Republic of China Received December 13, 2007. Revised manuscript received February 04, 2008. Accepted March 31, 2008. In this study, AgNO3 films prepared by a simple dip-coating method were used to remove gaseous methyl mercaptan (CH3SH) for odor control. The AgNO3 films were characterized by means of X-ray diffraction (XRD), Fourier transform infrared spectroscopy (FTIR), scanning electron microscopy/energydispersiveX-rayspectrometry(SEM/EDX),andX-rayphotoelectron spectroscopy (XPS) before and after the reaction, and asobtained products were identified by means of gas chromatography/mass spectrometry (GC/MS) and ion chromatography. The experiments demonstrated that the AgNO3 film can induce a quick chemisorption of gaseous CH3SH to form AgSCH3 and other intermediate products such as R-Ag2S, Ag4S2, and AgSH on its surface. Under UVA illumination, these sulfur products can be photocatalytically oxidized to AgSO3CH3 and Ag2SO4. Then AgSO3CH3 and Ag2SO4 will continue the chemisorption of gaseous CH3SH, similar to AgNO3, to form AgSCH3 again and release two final products, HSO3CH3 and H2SO4. Hence it is a AgNO3-induced photocatalytic reaction for odorous CH3SH degradation in gaseous phase. This fundamental research about the mechanism of chemisorption and photocatalytic reaction provides essential knowledge with potential to further develop a new process for gaseous CH3SH degradation in odor control. Introduction Mercaptans are highly toxic and corrosive as a group of offensive odorous compounds with low odor detection thresholds. Among them, methyl mercaptan (CH3SH) may be a representative member with a very low odor threshold of around 0.4 ppb (1). Several techniques have been studied for removing CH3SH from a gaseous phase such as catalytic oxidation, adsorption, catalytic incineration, radiolytic decomposition, and biological degradation (2, 3). Recently, Satokawa et al. (4) reported that Ag-exchanged Y zeolite * To whom correspondence should be addressed. Tel: +85227666016; fax: +852-23346389; e-mail: [email protected]. † The Hong Kong Polytechnic University. ‡ Guangdong Institute of Eco-Environment and Soil Science. 4540 9 ENVIRONMENTAL SCIENCE & TECHNOLOGY / VOL. 42, NO. 12, 2008 (Ag-Y) was a favorable adsorbent to remove sulfur compounds from pipeline natural gas fuel under ambient conditions even in the presence of water vapor, which can be a new desulfurization process for polymer electrolyte fuel cells (PEFC). A few reports also demonstrated that some Agexchanged zeolites are effective for removing sulfur compounds such as dimethylsulfide, tetrahydrothiophene, and thiophenes (5). Shimizu et al. (6) studied the removal of tertbutanethiol under ambient conditions with silver nitrate supported on silica and silica-alumina, including its reaction mechanism. Unfortunately, silver nitrate, as an adsorbent, can be easily saturated and disabled. Alternatively, it has been confirmed that mercaptans can be strongly adsorbed by some metals such as gold or silver to form self-assembled monolayers (SAMs) and undergo quick degradation upon exposure to UV light irradiation in air to form sulfonate or sulfate groups eventually (7). However, such a feature attracted intensive research interests to study some fundamental interfacial interactions among adhesion, wetting, molecular recognition, and other biological interactions and also the fundamental research of novel microstructured organic materials and devices (8). To the best of our knowledge, there is a lack of research on the photocatalytic oxidation of thiolates using silver for odor treatment based on the above-mentioned characters. In this study, a novel approach to photocatalytic oxidation of the thiolates with silver under UV illumination was proposed to remove CH3SH for odor control. The possible mechanism of chemisorption and photocatalytic reaction in this new process was studied in detail. Experimental Section Preparation of AgNO3 Film Sheets. AgNO3 (analytical grade) was purchased from Johnson Matthey Chemicals Ltd. and used to prepare AgNO3 films on Whatman glass fiber sheets with an area of 18 cm × 26 cm, in which the AgNO3 solution (0.01 g of AgNO3 in 25 mL of distilled water) was uniformly dripped on the glass fiber sheet with a catalyst loading of 0.21 g m-2. Then the prepared AgNO3 films were dried in an oven at 70 °C for 24 h in the dark. Experimental Setup. All experiments of adsorption and photocatalytic oxidation of CH3SH in a gaseous phase were conducted in a batch photoreactor system equipped with three UVA lamps (light intensity ) 1.24 mW cm-2) and a CH3SH analyzer (Detcon DM-100-CH3SH) with a detection limit of 0.1 ppm. The synthetic odorous gas was prepared by mixing CH3SH and zero air gases in a gas mixing chamber and its humidity was controlled at 52% ( 2%, before it was introduced into the photoreactor. A detailed description of the experimental setup is present in the Supporting Information as Figure S1. Experimental Procedure. (1) In the experiments of chemisorption and photocatalytic reaction, the CH3SH gas with an initial concentration of about 40 ppm (about 55 µmol) was purged into the photoreactor and was kept in the dark until it reached a gas-solid adsorption/desorption equilibrium. Then UVA light was turned on and photoreaction took place. After the CH3SH concentration was reduced to below 0.1 ppm, the light was turned off and the fresh CH3SH gas was injected into the photoreactor to make the same initial concentration again. The above experimental procedure was repeated for five cycles to monitor the variation of CH3SH concentration inside the photoreactor (2). To characterize the AgNO3 films affected by the chemisorption and photocatalytic reaction, four AgNO3 films were prepared by equally coating glass sheets with 0.15 g of AgNO3 and then drying the 10.1021/es7031345 CCC: $40.75 2008 American Chemical Society Published on Web 05/14/2008 sheets at 70 °C for 12 h. One of the AgNO3 films was used as a blank sample, named “AgNO3”. The other three AgNO3 films were exposed to CH3SH for 4 h in the dark to reach a gas/solid adsorption equilibrium. One of them was named “Ag-MM-dark” and the other two, which reacted with CH3SH under UVA illumination for 5 and 165 h, respectively, were named “Ag-MM-UVA5” and “Ag-MM-UVA165” (3). Since the adsorbed CH3SH on the AgNO3 film can be oxidized to some ionic species such as CH3SO3- and SO42- under UVA illumination, an experiment to separate chemisorption and photocatalytic reactions was conducted with the following procedure: (i) A AgNO3 film sheet consisting of seven small pieces was placed in the photoreactor, in which each piece of AgNO3 films had a size of 4 cm2 and 0.05 g of AgNO3 equally and could be individually taken out during the photocatalytic reaction as required. (ii) The synthetic CH3SH gas was purged into the photoreactor to make up an initial CH3SH concentration of 100 ppm, and the CH3SH was chemically adsorbed by the AgNO3 film in the dark. This step was repeated 5 times until the surface of AgNO3 film was fully covered by adsorbed CH3SH. According to the CH3SH concentrations before and after each chemisorption in the photoreactor, the amount of adsorbed CH3SH on the AgNO3 film was determined to be 96 µmol/piece. (iii) After chemisorption, the photoreactor was refilled with fresh air to expel all residual CH3SH gas and then UVA lamps were turned on to conduct the photocatalytic reaction for up to 165 h. The AgNO3 film samples were taken out piece by piece at different time intervals for further analysis. The experiment was repeated twice, and the film samples were extracted in 20 mL of 1 M nitrate solution at 25 °C for 48 h and then filtered through a 0.22-µm Millipore filter. The dissolved ions in the nitrate solution were analyzed by ion chromatography (IC). Analytical Methods. X-ray diffraction (XRD), Fourier transform infrared spectroscopy (FTIR), energy-dispersive X-ray spectrometry (EDX), and X-ray photoelectron spectroscopy (XPS) were employed to fully characterize the AgNO3 films. Gas chromatography/mass spectrometry (GC/MS) and IC analyses were used to identify the intermediate products. Details of the analytical conditions are included in the Supporting Information. Results and Discussion Chemisorption and Photocatalytic Reaction of CH3SH on AgNO3 Film. Experimental results about the reduction of CH3SH in gaseous phase versus time in five cycles, including the first cycle in the dark and the following four cycles under UVA illumination, are shown in Figure 1a. The results showed that CH3SH after the first injection disappeared quickly in the dark due to chemisorption, but its adsorption rate during the dark period gradually reduced in the following four cycles significantly. The results also revealed that the reduction of CH3SH under UVA illumination was well maintained in the following four cycles with a similar pattern. To distinguish the CH3SH reduction on the AgNO3 film by chemisorption alone from the chemisorption/photoreaction, the experimental data were further calculated to determine the firstorder rate constants (k) of CH3SH reduction in the dark and under UVA illumination. The k values for chemisorption alone under dark conditions varied from k ) 0.3202 min-1 in the first cycle and k ) 0.0347 min-1 in the second cycle down to k < 0.01 min-1 in the following cycles. These results indicate that the chemisorption of CH3SH on the AgNO3 film was quickly saturated after the first cycle. However, consistent k values under UVA illumination in the four cycles were determined to be 0.0567, 0.0588, 0.0615, and 0.0573 min-1, respectively, which indicated that the saturated AgNO3 film could be refreshed under UVA illumination due to the photocatalytic reaction. Hence, a combination of chemisorption and photocatalytic reaction on the AgNO3 film would FIGURE 1. (a) Time course of the decomposition of CH3SH with silver in the photoreactor. (b) Odor removal efficiency with initial CH3SH concentration of 3 ppm for up to 60 min. be a good approach to reduce CH3SH from gaseous phase continuously. To evaluate the efficiency of odor removal at a lower strength, one more experiment was conducted under the same experimental conditions with an initial CH3SH concentration of 3 ppm for 60 min. Since the applied CH3SH analyzer has a detection limit of 0.1 ppm, an olfactometry analysis using a forced-choice dynamic olfactometer (Olfactomat-n2) with a detection limit of 10 ou/m3 in accordance with the European Standard Method (EN13725) was employed to determine odor concentration when CH3SH concentration was below 0.1 ppm. The experimental results as shown in Figure 1b revealed that the initial odor concentration of 8228 ou/m3 ([CH3SH]0 ) 3 ppm) was quickly reduced to 402 ou/m3 at 15 min, 116 ou/m3 at 30 min, and <10 ou/m3 (equal to [CH3SH] < 4 ppb) at 60 min, respectively. These results demonstrated a good performance of odor reduction in such a system. GC/MS Analysis. The intermediate and final products were identified by various analyses. Some gaseous products were first tested by GC/MS. While dimethyl disulfide (CH3SSCH3, m/z ) 94) was identified in the sample collected before photoreaction, sulfonate (C2H6SO2, m/z ) 94) with minor amounts of other sulfonate species including C2H6S2O2 (m/z ) 126) and C2H6S2O4 (m/z ) 158) were detected in the sample after 250 min of photoreaction. SO2 Analysis. The gaseous samples (about 3 L each) after photocatalytic reaction were also analyzed by a photoluminescence-type SO2 analyzer to determine SO2 concentraVOL. 42, NO. 12, 2008 / ENVIRONMENTAL SCIENCE & TECHNOLOGY 9 4541 tion. However, the results showed that gaseous SO2 is not a main product in this process. IC Analysis. Two main products of methanesulfonic acid ion (CH3SO3-) and sulfate ion (SO42-) were detected and their concentrations versus experimental time are shown in the Supporting Information as Figure S2. The results showed that as illumination time was extended, the amount of CH3SO3- increased initially and then decreased gradually as an intermediate product, while the amount of SO42increased gradually all the time. These results confirmed that the adsorbed CH3SH on the AgNO3 film can be oxidized under UVA illumination to form CH3SO3- and then SO42-. However, it was also noted that the total amount of oxidized sulfur products (CH3SO3- + SO42-) on the last piece of AgNO3 film after 165 h was only 23.6 µmol, equivalent to 24.6% of the total sulfur of 96 µmol as CH3SH. Such a small portion of sulfur conversion from CH3SH to CH3SO3- and SO42- might result from two causes: (i) the conversion rate of AgSCH3 to CH3SO3 or SO42- by photocatalytic reaction on the solid surface of the AgNO3 film is much slower than the chemisorption of CH3SH; (ii) oxidized products such as Ag2SO4 accumulated on the surface of the AgNO3 film to slow down or block further photocatalytic reaction. Color of AgNO3 Film Surface. Four film samples (AgNO3, Ag-MM-dark, Ag-MM-UVA5, and Ag-MM-UVA165) were compared to observe the surface color changes due to the chemisorption and photocatalytic reaction. It was observed that the color of the AgNO3 film changed from white (AgNO3) to light yellow (Ag-MM-dark) after the chemisorption in the dark and further to dark brown (Ag-MM-UVA5 and Ag-MMUVA165) after the photocatalytic reaction under UVA illumination. These color changes indicate that an interactive reaction between the mercapto group of CH3SH and the Ag+ ion in the interlayer region, rather than simple adsorption, resulted in a significant change in the structure of silver and/ or sulfur species, possibly via chemical reactions between CH3SH and Ag+. SEM/EDX Analysis. Three samples, AgNO3, Ag-MMdark, and Ag-MM-UVA5, were examined by scanning electron microscopy (SEM)/EDX. Their SEM images are shown in Figure 2. It can be seen that the surface of the AgNO3 sample (Figure 2a) was very smooth. After the reaction with CH3SH in the dark, the surface of Ag-MM-dark sample became rough and was covered with some S-containing products (Figure 2b). To determine the sulfur content, the Ag-MM-dark sample was also analyzed by EDX and the ratio of S/Ag was determined to be 18/82. This result confirmed the existence of sulfur species on the AgNO3 surface due to the chemisorption reaction. The SEM image of Ag-MM-UVA5 surface (Figure 2c) showed that, after the photocatalytic reaction under UVA illumination, its surface was significantly eroded and densely covered by some deposits with much smaller particle sizes compared to those on the Ag-MM-dark sample. In addition, the EDX analysis showed that the Ag-MM-UVA5 sample had a higher S/Ag ratio of 30/70 than the Ag-MMdark sample, which means more sulfur products were formed on the film surface due to photocatalytic reaction. Furthermore, the surface of the Ag-MM-UVA5 sample was found to be more porous than the other two samples. XRD Analysis. The XRD patterns of four samples are shown in Figure 3 to compare their crystalline structures during different reactions. The XRD pattern of the AgNO3 sample (curve A) showed a typical AgNO3 structure corresponding to JCPDS 43-0649. The XRD pattern of Ag-MMdark (curve B) showed three diffraction lines at 2θ ) 31.3°, 34.8°, and 37.0°, representing R-Ag2S (JCPDS 14-72), and also other peaks at 2θ ) 11.7°, 13.5°, 15.1°, 22.5°, 29.7°, 44.3°, and 46.5°. Some similar studies (9) reported that the structure of silver sulfides in these samples is not the same as R-Ag2S but Ag2S clusters, because the Ag-S distances of the Ag samples 4542 9 ENVIRONMENTAL SCIENCE & TECHNOLOGY / VOL. 42, NO. 12, 2008 FIGURE 2. SEM images of (A) AgNO3, (B) Ag-MM-dark, and (C) Ag-MM-UVA5. FIGURE 3. XRD patterns of (A) AgNO3, (B) Ag-MM-dark, (C) Ag-MM-UVA5, and (D) Ag-MM-UVA165. reacted with organic sulfur in the dark are shorter than the average Ag-S distance of crystalline R-Ag2S. So it can be speculated that the unknown peaks may be due to other Ag-S species such as Ag4S2, AgSH, and so on (9). The XRD pattern of Ag-MM-UVA5 (curve C) showed a similar pattern to the Ag-MM-dark sample but with lower intensity, indicating that the R-Ag2S and other Ag-S species on the film surface might disappear and some new products appeared on the surface. Furthermore, the XRD pattern of Ag-MM-UVA165 (curve D) demonstrated that most peaks related to R-Ag2S and other Ag-S species almost disappeared, while a new sharp peak appeared at 2θ ) 31.5°, which may be assigned FIGURE 4. FTIR spectra of (A) AgNO3, (B) Ag-MM-dark, (C) Ag-MM-UVA5, and (D) Ag-MM-UVA165. to β-Ag2SO4 (JCPDS 27-1403). This result confirmed that the Ag-S species formed by chemisorption can be degraded under UVA illumination. FTIR Analysis. The above four samples were further examined by FTIR and the analytical results are shown in Figure 4. Compared with the AgNO3 sample as a blank, some new peaks were found in the FTIR spectra of Ag-MM-dark and Ag-MM-UVA5. For example, the peaks at 684, 960, and 1305 cm-1 were attributed to the vibration of C-S, S-H, and C-H, respectively, in CH3SH (10). Hence, it can be concluded that surface-bound CH3S-Ag can be formed due to the chemisorption reaction. It was noted that the three peaks of Ag-MM-UVA5 were slightly stronger than those of the AgMM-dark sample, suggesting that the CH3S-Ag complex can also be formed under UVA illumination. After longer exposure times under UVA illumination (curve D), these peaks decreased obviously, indicating the breakdown of surfacebound CH3S-Ag. Furthermore, the spectrum of Ag-MMUVA5 showed that after the photocatalytic reaction between AgNO3 and CH3SH under UVA illumination, the new peaks at 1049 and 1205 cm-1 appeared, attributed to the vibrations of SdO and S-O relevant to SO42- or CH3SO3- groups (11). Curve D for Ag-MM-UVA165 also showed that the broad absorption bands with maxima at 616 and 1107 cm-1 can be assigned to the stretching mode of O-S-O and S-O bonds in the Ag2S-Ag2SO4 system (12), which are well matched with the result of XRD. This result further confirmed that surface-bound CH3S-Ag formed in the dark can be gradually oxidized into the sulfonate species under UVA illumination. XPS Analysis. Figure 5a shows XPS spectra of the S 2p3/2 region of three samples. The AgNO3 sample (curve A) exhibited no sulfur peaks. After exposure to CH3SH in the dark, the Ag-MM-dark sample (curve B) showed a peak at the binding energy of 162.6 eV, representing a characteristic of the sulfide species on silver. After the photocatalytic reaction under UVA illumination for 5 h, the Ag-MM-UVA5 sample (curve C) had an increased peak at 162.4 eV. In the meantime, a new peak at 168.2 eV was also found, attributed to the sulfonate species formed from the photocatalytic oxidation reaction. The increase of S 2p peak areas at 162.4 eV before and after photolycatalytic reaction suggests that the amount of sulfide species increased. It has been commonly assumed that the S-H bond scission occurs even at room temperature to form Ag-S species in the dark (13), which was consistent with our result about the formation of Ag-SCH3. Lewis et al. (14) postulated that the mechanism of SAMs photooxidation on Ag involved initial C-S bond cleavage followed by desorption of alkyl fragments and oxidation of surface-bound sulfur species. In this study, both reactions of C-S bond cleavage to form Ag-S species and new sulfonate formation actually occurred under UVA illumination simultaneously, while the former was faster than the latter. This phenomenon is well matched with Lewis’s hypothesis. So far, the status of the Ag cations was not accurately determined. Most studies on silver systems indicated an anomalous negative shift in binding energy (BE) of the Ag 3d peaks depending on the extent of oxidation state, while a few studies showed no BE shift with the increased oxidation state (15). From Figure 5b, Ag 3d5/2 (around 368-369 eV) and Ag 3d3/2 (around 374-375 eV) peaks were compared among three samples and the relevant data are also listed in Table S1. Curve B shows that the two peaks shifted toward higher energy by 0.3 eV for Ag 3d5/2 and 0.1 eV for Ag 3d3/2, which might indicate the change in the oxidation state of Ag from Ag+ (AgNO3) to Ag+ (Ag-S species) due to the chemisorption reaction. Curve C showed that the BE of AgNO3 shifted toward higher energy by 0.1 eV for Ag 3d5/2 and 0.1 eV for Ag 3d3/2, which might result from the newly generated Ag2SO4 or AgSO3CH3 after the photocatalytic reaction. The XPS results of O 1s and N 1s peaks as shown in Figure 5c,d may be helpful to explain the complicated behavior of the Ag 3d peaks. The N 1s peak at 406.2 eV for AgNO3 (curve A) was similar to that for Ag-MM-dark (curve B) at 406.3 eV, while the peak intensity decreased to a certain extent. For Ag-MM-UVA5 (curve C), the N 1s peak disappeared completely, which might result from the decomposition of NO3under UVA illumination. The O 1s peak at 532.3 eV for AgNO3 (curve A) was very similar to that for Ag-MM-dark at 532.1 eV (curve B), while the peak intensity decreased to some degree. These results were in good agreement with those of N 1s peaks. This was unambiguously assigned to the decomposition of AgNO3 reacted with CH3SH in accordance with other studies (6). Furthermore, a new O 1s peak at 531.3 eV for Ag-MM-UVA5 (curve C) should be attributed to the oxidized sulfur species, since the desorption of sulfone species and the sulfide-to-sulfone transformation can affect the O 1s XPS spectra as well (16). From the analyses of N and O, the NO3- in AgNO3 can be replaced by CH3SH to form Ag-SCH3 complex, which will be oxidized to AgSO3CH3 and Ag2SO4 during the photocatalytic reaction. After the NO3disappeared, the Ag-SCH3 complex can still be formed by the replacement of CH3SH on AgSO3CH3 and Ag2SO4. All the intermediate products detected by different methods are summarized in Supporting Information Table S2. Mechanism of Chemisorption. Silver nitrate supported on silica or silica-alumina is found to be an effective adsorbent for the vapor-phase adsorptive removal of tertbutanethiol under ambient conditions. The mechanism of silver sulfides formation was proposed as AgNO3 + C4H9SH f AgSH f Ag2S f Ag4S2, indicating that most of the silver species are present as Ag2S-like species (6). The XRD, FTIR, and XPS results in this study supported the existence of Ag-S species as the primary products after AgNO3 was exposed to gaseous CH3SH in the reactor. The investigation on the SAMs showed that the S-H bond of alkanethiols dissociates on an Ag or Au surface to form an alkanethiolate species, which can be strongly attached by chemisorption onto the metal surface through the S atom as an anchor (17). As a shorterchain molecule with S-H, CH3SH should also have a similar character. Some studies (18) reported that metal M and M+ (Cu, Ag, or Au) all could react with mercaptans or other sulfur compounds through the following equation: M+ + CH3SH f M-CH3 + H+ (1) In this study the CH3SH-Ag was formed on the surface of AgNO3 film in the dark according to eq 1, in which the S-H bond of CH3SH was cleaved due to the activation by Ag+ (19). The results of FTIR and GC/MS suggested that the CH3S-SCH3 was formed due to scission of the S-H bond. VOL. 42, NO. 12, 2008 / ENVIRONMENTAL SCIENCE & TECHNOLOGY 9 4543 FIGURE 5. XPS spectra of (a) Ag 3d, (b) S 2p, (c) N 1s, and (d) O 1s for the samples (A) AgNO3, (B) Ag-MM-dark, and(C) Ag-MM-UVA5. In the meantime, C-S bond cleavage could also occur, because (i) S-S scission in disulfides and C-S scission in monosulfides occur generally in organic sulfides adsorbed on silver under mild conditions (20), and (ii) the Ag-S bond is more ionic than the C-S bond, based on the electronegativity differences between S and Ag (21). Accordingly, the organic disulfides and monosulfides are decomposed on silver, where a C-S bond is replaced by a strong Ag-S bond. Therefore, the chemisorption reaction in this process should follow eq 2, involving the cleavage of S-H and C-S bonds to form Ag-SCH3 and other Ag-S species (Ag2S, Ag4S2, or AgSH) adsorbed on the surface. FIGURE 6. Proposed pathway of CH3SH degradation on AgNO3 films by chemisorption and photocatalytic reaction. AgNO3 + CH3SH f Ag-SCH3 + HNO3 f Ag-S species (Ag2S, Ag4S2, or AgSH) (2) Mechanism of Photocatalytic Reaction. In this study, it was found that the above products formed on the AgNO3 film by chemisorption could be further oxidized under UVA illumination significantly. To the best of our knowledge, the mechanism of photocatalytic reaction of desulfurization in such an Ag-UVA system has not been well studied. The complex formed by SAMs on the AgNO3 film surface could be corroded by UVA light. The mechanism of photocatalytic reaction under UVA illumination involves two competitive reactions: oxidation, in which the Ag-SCH3 complex was photocatalytically oxidized to form AgSO3CH3 and further Ag2SO4, and S-C bond scission, in which the Ag-SCH3 complex was induced by UV light and it led to an increase in the amount of Ag-S species such as Ag2S, Ag4S2, or AgSH on the film surface as for chemisorption in the dark. However, the oxidation of Ag-S species to SO42- is a much slower reaction than the S-C bond scission, based on the observations of Lewis et al. (14). Hence, a large fraction of Ag-S 4544 9 ENVIRONMENTAL SCIENCE & TECHNOLOGY / VOL. 42, NO. 12, 2008 species accumulated on the film surface, which was obviously more than the amount of oxidized sulfur. It has been reported (22) that the alkylsulfonate groups (R-SO3) and sulfate (SO42-) formed by the photooxidation were only weakly bound to the Ag substrate and can be readily displaced from the surface by other thiol molecules. So the oxidized products (Ag2SO4 and AgSO3CH3) could react with CH3SH again through eqs 3 and 4 as follows: Ag2SO4 + CH3SH f Ag-SCH3 + H2SO4 (3) AgSO3CH3 + CH3SH f Ag-SCH3 + HSO3CH3 (4) To have full understanding of the above reactions, the mechanism of chemisorption and photocatalytic reaction in this system is proposed as shown in Figure 6. In the dark, AgNO3 can adsorb CH3SH immediately to form Ag-SCH3 that is then decomposed by the scission of C-S to generate the Ag-S species (Ag2S, Ag4S2, AgSH, etc). Under UVA illumination, Ag-SCH3 and other Ag-S species can be oxidized into AgSO3CH3 and Ag2SO4 that can also react with CH3SH to form Ag-SCH3 again and release two final products of HSO3CH3 and H2SO4. It can be seen that with three core intermediates of Ag-SCH3, AgSO3CH3, and Ag2SO4, the chemisorption and photocatalytic reaction are continuously preceded under UVA illumination to degrade gaseous CH3SH into two aqueous acids as its final products. Therefore, this AgNO3-UVA light system may provide a new approach to degrade some thiolates in odorous gases by the AgNO3induced photocatalytic reaction. Acknowledgments We thank the Hong Kong Government Research Grant Committee for financial support of this work (RGC PolyU 5226/06E). Supporting Information Available Detailed description of experimental setup, details of analytical conditions, CH3SO3- and SO42- concentrations versus experimental time, comparison of Ag 3d5/2 and Ag 3d3/2 peaks among three samples, and summary of intermediate products detected by different methods. This material is available free of charge via the Internet at http://pubs.acs.org. Literature Cited (1) Hartikainen, T.; Martikainen, P. 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