Akira
Yamamoto
a,
Yuto
Mizuno
a,
Kentaro
Teramura
*abc,
Saburo
Hosokawa
ab,
Tetsuya
Shishido
bd and
Tsunehiro
Tanaka
*ab
aDepartment of Molecular Engineering, Graduate School of Engineering, Kyoto University, Kyoto daigaku Katsura, Nishikyo-ku, Kyoto 615-8510, Japan. E-mail: teramura@moleng.kyoto-u.ac.jp; Fax: +81 75 383 2561; Tel: +81 75 383 2559
bElements Strategy Initiative for Catalysts & Batteries (ESICB), Kyoto University, 1-30 Goryo-Ohara, Nishikyo-ku, Kyoto 615-8245, Japan
cPrecursory Research for Embryonic Science and Technology (PRESTO), Japan Science and Technology Agency (JST), 4-1-8 Honcho, Kawaguchi, Saitama 332-0012, Japan
dDepartment of Applied Chemistry, Graduate School of Urban Environmental Sciences, Tokyo Metropolitan University, 1-1 Minami-Osawa, Hachioji, Tokyo 192-0397, Japan
First published on 18th September 2014
Porphyrin-derivative-modified TiO2 photocatalysts showed high photocatalytic activity for the selective catalytic reduction of NO with NH3 in the presence of O2 under visible-light irradiation. Tetra(p-carboxyphenyl)porphyrin (TCPP) was the most effective photosensitizer among the five porphyrin derivatives investigated. NO conversion and N2 selectivity of 79.0% and 100%, respectively, were achieved at a gas hourly space velocity of 50000 h−1. UV–Vis and photoluminescence spectroscopies revealed the presence of two species of TCPP on the TiO2 surface; one was a TCPP monomer and the other was an H-aggregate of the TCPP molecules. It was concluded that the TCPP monomer is an active species for the photo-assisted selective catalytic reduction (photo-SCR). Moreover, an increase in the fraction of H-aggregates with increasing TCPP loading amount resulted in a decrease in the photocatalytic activity of the photo-SCR.
Expansion of the adsorption wavelength to the visible-light region is an effective way of improving the photocatalytic activity. TiO2 photocatalysts do not absorb visible light because of their wide bandgap (>3.2 eV). Surprisingly, the photo-SCR proceeds to some extent under visible-light irradiation over the TiO2 photocatalysts. This is due to the direct electron transfer from the electron donor level of the N 2p orbital of the adsorbed NH3 to the conduction band of the Ti 3d orbital of TiO2 (in situ doping).12,13 However, the photocatalytic activity under visible-light irradiation is not sufficient for the application of the photo-SCR technology to the system at a high GHSV region. Thus, the proposed study aims to increase the photocatalytic efficiency under visible-light irradiation.
Porphyrin derivatives have absorption bands in the visible region owing to the π–π* transitions. Porphyrin derivatives are widely used as sensitizers in dye-sensitized solar cells (DSSCs)14–17 and dye-sensitized photocatalysts18–20 under visible-light irradiation owing to the following properties: 1) they exhibit intense absorption bands in the visible-light region, and 2) their photochemical and electrochemical properties can be tuned by the modification of the substituents and selection of the central metal. In previous studies, the porphyrin-sensitized photocatalysts were used for performing liquid phase reactions such as hydrogen production from water20 and degradation of organic compounds.18,19,21 However, there are only a few reports on the reactions involving porphyrin-sensitized photocatalysts in the gas phase. Recently, Ismail et al. reported that the porphyrin-sensitized mesoporous TiO2 films exhibited an improved photocatalytic activity for the photodegradation of acetaldehyde in the gas phase under visible-light irradiation.22 The porphyrin derivative-modified photocatalyst works efficiently as a visible-light response photocatalyst in the gas phase. In this study, we used five types of porphyrins for the modification of the TiO2 photocatalyst and investigated their performance in the photo-SCR using a gas flow reactor at a high GHSV of 50000 h−1.
Fig. 2 shows the UV–Vis DR spectra of the various porphyrin-modified TiO2 photocatalysts. The unmodified TiO2 photocatalyst did not absorb the visible light above 400 nm. The modification of the porphyrin derivatives increased the absorption in the visible-light region. The absorption at 420 nm (Soret band) decreased in the following order: TCPP-TiO2 > TPP-TiO2 ≒ TSPP-TiO2 > TMPP-TiO2 > TAPP-TiO2 > TiO2. The order of the absorption is consistent with that of the NO conversion. The photocatalytic activities of NO were strongly dependent on the absorbance in the visible-light region, which suggested that the porphyrin derivatives functioned as photosensitizers under visible-light irradiation.
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Fig. 2 UV–Vis diffuse reflectance spectra of (A) TiO2, (B) TCPP-TiO2, (C) TSPP-TiO2, (D) TPP-TiO2, (E) TMPP-TiO2, and (F) TAPP-TiO2. |
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Fig. 3 UV–Vis diffuse reflectance spectra of various loading amounts of TCPP-TiO2: (A) 0 μmol g−1, (B) 1.3 μmol g−1, (C) 6.3 μmol g−1, (D) 12.5 μmol g−1, (E) 37.5 μmol g−1, and (F) 62.5 μmol g−1. |
The peak positions of the Soret band and Q bands as a function of TCPP loading are shown in Table 1. The peak position of the Soret band of 1.3 μmol g−1 TCPP-TiO2-IMP (417 nm) corresponded to those of the TCPP molecules dissolved in CH3OH (418 nm). The TCPP molecules existed as a monomer in the CH3OH solution and the peak position of the TCPP monomer coincided with that reported previously.24 Thus, the TCPP molecules existed as monomers on the TiO2 surface at the low loading amount of 1.3 μmol g−1. The peak position of the Soret band was shifted from 417 to 407 nm (blue shift) when the loading amount of TCPP was increased from 1.3 to 62.5 μmol g−1. The origin of the blue shift can be explained on the basis of a “face to face” stacking pattern of TCPP (H-aggregate) according to Kasha's exciton theory.25 Thus, the blue-shifted peak observed at 407 nm can be attributed to the Soret exciton band in the H-aggregates of the TCPP. The gradual spectral shift can be explained as the result of the relative contribution of the monomers and H-aggregates. The H-aggregates were generated with an increase in the TCPP loading. The contribution of the H-aggregates became dominant for the Soret band of adsorption spectra of various loading amounts of TCPP-TiO2, which results in the gradual blue shift of the Soret band.
Sample | Loading of TCPP/μmol g−1 | Soret/nm | Qy(0,1)/nm | Qy(0,0)/nm | Qx(0,1)/nm | Qx(0, 0)/nm |
---|---|---|---|---|---|---|
TCPP-TiO2-IMP | 1.3 | 417 | 519 | 555 | 592 | 649 |
TCPP-TiO2-IMP | 6.3 | 416 | 520 | 557 | 592 | 651 |
TCPP-TiO2-IMP | 12.5 | 411 | 521 | 559 | 593 | 652 |
TCPP-TiO2-IMP | 37.5 | 411 | 522 | 562 | 595 | 654 |
TCPP-TiO2-IMP | 62.5 | 407 | 522 | 560 | 594 | 653 |
TCPP-TiO2-MIX | 12.5 | 419 | 529 | 565 | 600 | 658 |
TCPP-SiO2-IMP | 12.5 | 422 | 521 | 556 | 593 | 649 |
TCPP in MeOH | — | 418 | 515 | 549 | 590 | 646 |
On the other hand, the peak positions of the Q bands of 1.3 μmol g−1 TCPP-TiO2-IMP (519, 555, 592, and 649 nm) were slightly shifted to longer wavelengths compared to those of the TCPP monomer in CH3OH (515, 549, 590, and 646 nm). The slight red shift can be ascribed to the aggregation of TCPP24 and/or the interactions between the TCPP and a solid surface.26 The peak positions of the four Q bands of the TCPP-TiO2-IMP were shifted to longer wavelengths with an increase in the TCPP loading amount. The peak position of the Q bands of the H-aggregates of the TCPP is larger than that of the TCPP monomers.24 Thus, the red shift of the Q bands is due to the generation of the H-aggregates. Consequently, both the monomers and the H-aggregates of TCPP are generated on TiO2 and the fraction of the H-aggregates increased with increasing TCPP loading amount.
Fig. 4 shows the effect of various loading amounts of TCPP-TiO2-IMP on the photo-SCR. The conversion of NO increased with increasing TCPP loading amount up to 12.5 μmol g−1. The surface density of TCPP molecules on 12.5 μmol g−1 TCPP-TiO2-IMP is estimated to be 2.8 × 10−2 molecule nm−2. As shown in Fig. 3, increasing the loading amount of TCPP enhanced the capability of the visible-light absorption, which leads to the higher conversion of NO. On the other hand, the conversion of NO decreased when the TCPP loading was higher than 12.5 μmol g−1. UV–Vis spectroscopy revealed that the H-aggregates of TCPP were generated with an increase in the TCPP loading amount. The excited state lifetime of the H-aggregates was slightly shorter than those of the monomers.24,27 The generation of H-aggregates with a short excited state lifetime decreased the electron transfer efficiency from the excited state of TCPP to the conduction band of TiO2 due to non-radiative deactivation, which possibly resulted in the decrease of the photo-SCR activity.
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Fig. 4 Dependence of conversion of NO on TCPP loading on TiO2 (catalyst amount: 110 mg, NO: 1000 ppm, NH3: 1000 ppm, O2: 2%, GHSV: 50![]() |
Entry | Catalyst | Inlet gas conc. (ppm) | N2 conc.a (ppm) | ||
---|---|---|---|---|---|
NO (ppm) | NH3 (ppm) | O2 (%) | |||
a Concentration of N2 in the outlet gas. Catalyst amount: 110 mg (TiO2, TCPP-TiO2), 50 mg (TCPP-SiO2), b TCPP loading: 12.5 μmol g−1. | |||||
1 | TCPP-TiO2-IMPb | 1000 | 1000 | 2 | 790 |
2 | TCPP-TiO2-IMPb | 0 | 1000 | 2 | 57 |
3 | TCPP-TiO2-IMPb | 1000 | 0 | 2 | 24 |
4 | TCPP-TiO2-IMPb | 1000 | 1000 | 0 | 42 |
5 | TCPP-TiO2-IMPb | 1000 | 1000 | 5 | 780 |
6 | TCPP-TiO2-IMPb | 1000 | 1000 | 10 | 771 |
7 | TCPP-SiO2-IMP2b | 1000 | 1000 | 2 | 63 |
8 | TCPP-TiO2-MIXb | 1000 | 1000 | 2 | 140 |
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Fig. 5 UV–Vis diffuse reflectance spectra of (A) TCPP-TiO2(IMP), (B) TCPP-SiO2, and (C) TCPP-TiO2(MIX) and adsorption spectra of 3.4 × 10−6 mol L−1 TCPP in methanol (D). |
Fig. 6 shows the photoluminescence spectra of TCPP-TiO2-IMP, TCPP-SiO2-IMP, TCPP-TiO2-MIX, and TCPP monomer in CH3OH. Two emission bands were observed in the TCPP monomer in CH3OH solution (650 and 714 nm), which coincided with the previously reported values.24 The emission bands at 650 and 714 nm can be attributed to the transition from the vibrational ground state of S1 to the vibrational ground state of S0 (Qx(0,0) transition) and to the vibrational excited state of S0 (Qx(0,1) transition) of the TCPP monomer, respectively.24,28 The peak positions of the emission bands in the TCPP-TiO2-IMP (654 and 715 nm) were almost similar to those of the TCPP monomer in CH3OH. It is reported that the emission bands of the H-aggregates of TCPP have lower intensity and are shifted to longer wavelengths than those of the monomers,29 which is totally different from the emission spectrum of the TCPP-TiO2-IMP. Accordingly, the emission bands of TCPP-TiO2-IMP were mainly composed of the TCPP monomer emissions.
Two emission bands were observed at 658 and 713 nm, and the peak positions were similar to those of the TCPP in CH3OH (650 and 714 nm) and TCPP-TiO2-IMP (654 and 715 nm) (Fig. 6). Thus, the TCPP species on SiO2 possesses a monomeric state, which is similar to that on TiO2. The low activity of TCPP-SiO2-IMP can be explained by an electron transfer mechanism, which is the key step in the DSSCs and dye-sensitized photocatalysts. In the first step of the photo-SCR over the TCPP-TiO2-IMP, the TCPP is excited by the visible-light irradiation. In the next step, the electron transfer occurs from the photo-excited TCPP to the conduction band of TiO2. However, the electron transfer cannot occur from the photo-excited TCPP to the conduction band of SiO2 because the energy level of the SiO2 conduction band is much higher than that of the lowest unoccupied molecular orbital (LUMO) of TCPP, which results in the low activity of the TCPP-SiO2-IMP. Hence, the photo-SCR over TCPP-TiO2-IMP under visible-light irradiation proceeds via the electron transfer from the photo-excited TCPP to the conduction band of TiO2.
No emission peak was observed for the TCPP-TiO2-MIX and TCPP powder (Fig. 6). The interaction between the TCPP molecules might lead to the non-radiative deactivation of the photo-excited states of TCPP, resulting in the luminescence quenching for the TCPP-TiO2-MIX and TCPP powder. These results explain the low activity of the TCPP-TiO2-MIX, i.e. although the TCPP molecules on the TCPP-TiO2-MIX absorb visible light, they do not function as a photosensitizer under visible-light irradiation because of the fast non-radiative quenching.
Footnote |
† Electronic supplementary information (ESI) available. See DOI: 10.1039/c4cy00598h |
This journal is © The Royal Society of Chemistry 2015 |