Open Access Article
Yohei Konishi,
Ichiro Tanabe† and
Tetsu Tatsuma*
Institute of Industrial Science, University of Tokyo, 4-6-1 Komaba, Meguro-ku, Tokyo 153-8505, Japan. E-mail: tatsuma@iis.u-tokyo.ac.jp; Fax: +81-3-5452-6338; Tel: +81-3-5452-6336
First published on 5th July 2013
The mechanism of plasmon-induced charge separation of gold nanoparticles (Au NPs) on TiO2 was investigated with the help of anionic ligands. Au NPs are oxidized in the presence of KX (X = SCN, Br or Cl), chiefly via direct oxidation to [AuX4]−. The reactivity of Au NPs depends on the solution pH, the type of anion ligands and the excitation wavelength, suggesting that the photopotential of Au NPs during plasmon-induced charge separation depends on both the flatband potential of TiO2 and the energy of irradiated photons. The results indicate that the reactivity and efficiency of the plasmon-induced charge separation and accompanying reactions can be tuned and optimized by changing those factors.
We have reported that TiO2 electrodes modified with Au3,4 or Ag4,18 NPs exhibit negative potential shifts and anodic currents under illumination. In contrast, Au9,19 or Ag9,20 NPs coated with TiO2 exhibit positive potential shifts and cathodic currents. On the basis of these results, we concluded that the charge separation is caused by electron transfer from metal NPs to TiO2, which is also supported in related studies by other groups.7,8,10,11,21–23
As mentioned above, Au NPs are generally so stable that the plasmon-induced charge separation does not cause their oxidative dissolution.3 In our previous research, however, we have achieved the plasmon-induced oxidative dissolution of Au NPs with the aid of I− (KI aqueous solution) and developed a multicolour change material, which is more resistive to white light than a Ag-based material.24 However, it is yet to be elucidated whether the Au dissolution is predominantly due to direct oxidation (Au + 4I− → [AuI4]− + 3e−, E° = +0.56 V vs. NHE) or indirect oxidation via I3− (3I− → I3− + 2e−, E° = +0.55 V, then 2Au + 3I3− → 2[AuI4]− + I−), because the potential of the former reaction is close to that of the latter (Fig. 1a). To obtain further information about this, here we used other ligands, i.e. Br−, Cl− and SCN−. In the case of Br− and Cl−, the potentials of the direct oxidation are far more negative than the oxidation potentials of the halide ion to tri-halide ion. Also, in a solution of SCN−, the indirect mechanism would not hold as SCN3− is known to be unstable in aqueous media.25 In addition, examination of the reactions in the presence of different ligands and at different pH values sheds light on the photopotentials of Au NPs during the plasmon-induced charge separation.
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| Fig. 1 (a) Values of the standard electrode potential E° for oxidative coordination of Au with anionic ligands (X−) and oxidation of the anions to X3−. (b) Mechanism of spectral dip formation for the Au NP–TiO2 system. (c) Potential shifts of Au NPs and TiO2 due to the plasmon-induced charge separation in an open circuit system. | ||
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9 by volume, 32 mL cm−2) was cast on the TiO2 film and left for 15 min, followed by rinsing with water. The mixture was cast again and the film was irradiated with UV light (260–370 nm, 25 mW cm−2) for 10 s. Electrons in the TiO2 valence band (VB) are excited to the conduction band (CB), and used for the reduction of [AuCl4]− to Au NPs. The corresponding generated holes in the VB are consumed by oxidation of ethanol.
For monochromatic light irradiation (4 mW cm−2) in 0.5 M KCl at pH 7, 8 or 9 (adjusted with KOH), a band-pass filter (full width at half maximum = 10 nm) for 700 nm (Asahi Spectra) or 800 or 900 nm (CVI Melles Griot) was used with the Xe lamp (700 nm) or the halogen lamp (800 and 900 nm).
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| Fig. 2 (a) Extinction spectrum of Au NPs deposited photocatalytically on the TiO2 film. (b–d) Normalized difference extinction spectra of Au NPs on TiO2 after 600–700 (blue), 700–800 (red) and 800–1000 (purple) nm light irradiation (10 mW cm−2, 30 min) in 0.5 M aqueous solution of (b) KSCN, (c) KBr and (d) KCl. | ||
The Au NP-modified TiO2 sample was irradiated with 600–700, 700–800 or 800–1000 nm light (10 mW cm−2) in 0.5 M KSCN, KBr or KCl aqueous solution for 30 min. Normalized difference extinction spectra after the light irradiations are shown in Fig. 2b–d. In all these cases, extinction decreased preferentially at around the irradiation wavelengths and wavelength-selective extinction dips were formed. These spectral changes are explained in terms of selective oxidation and dissolution of resonant Au NPs to [AuX4]− (X: halogen or SCN) (Fig. 1b).24 The peaks at ∼540 nm in the difference spectra are attributed to smaller NPs formed eventually by the dissolution, which exhibit LSPR at ∼540 nm.24 Small Au NPs deposited by recombination of the [AuX4]− ions and electrons transferred to TiO2 may also be responsible for the peaks.24,26
In the case of X = SCN, the dip formation must be caused by the direct oxidation (Au + 4SCN− → [Au(SCN)4]− + 3e−), because SCN3− is unstable in aqueous media,25 as described above. The direct oxidation should also be the major pathway in the case of X = Br and Cl, because the potentials for the direct oxidation are more negative than those for the X3− generation (Fig. 1a). In particular, the potential for Cl3− generation is even more positive than that of water oxidation.
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| Fig. 3 Difference extinction spectra of Au NPs on TiO2 after irradiation with 800 and 900 nm (4 mW cm−2, 30 min) light in 0.5 M KCl ((a) pH 7, (b) 8 and (c) 9) and (d) KBr (pH 9) aqueous solutions. | ||
There are two possible explanations for the suppression of the photoreactions at high pH. (I) If the TiO2 CB level at the TiO2–Au NP interface Efb–Au is not affected by the CB level at the TiO2–solution interface Efb–sol, the rise of the latter could slow down electron transport from the TiO2–Au NP interface to other parts of TiO2 and thereby lower the charge separation efficiency. However, the dependence of the reactivity on the excitation wavelength only at higher pH is not explained by this hypothesis. (II) If Efb–Au is affected by Efb–sol because the area of the TiO2–Au NP interface is so small, the photopotential at Au NPs may depend on pH. The photopotential may also depend on the excitation wavelength.
In the plasmon-induced charge separation, some electrons in a resonant Au NP should be transferred to TiO2 through the Schottky barrier at the TiO2–Au NP interface.3,19 The barrier height ΔES is estimated to be ∼1.2 eV or higher, as the electron affinity of nanoparticulate anatase TiO2 and the work function of Au are ∼3.9 eV28,29 and 5.1–5.47 eV,30,31 respectively. Sönnichsen et al.32 described that LSPR decays partially via inter- or intraband transition. However, it may not be reasonable to assume that those excited states are long-lived enough to be involved in the electron transfer from Au NPs to TiO2, unless electrons pass through trap states, if any, at the TiO2–Au interface. If not, it is likely that the electron transfer is due to hot electron injection or external photoelectric effect. Under irradiation of photons with an energy of ΔEp eV that is higher than the Schottky barrier height ΔES (i.e. ΔEp ≥ ΔES), those types of electron transfer may shift the potential of Au NPs positively up to Efb–Au + ΔEp V (Fig. 1c). If this is the case, the spectral dip formation should be suppressed when the Efb–Au + ΔEp is more negative than EAu–Cl + ΔEop, where ΔEop is the overpotential needed for the redox reaction. That is, the photoinduced redox reaction could be suppressed at high pH and at a long wavelength even if ΔEp ≥ ΔES.
Actually, the reaction occurs under 700 and 800 nm light (ΔEp = 1.77 and 1.55 eV, respectively) at pH 7–9, where Efb–Au + ΔEp = +1.30–+1.63 V vs. NHE on the assumption that Efb–Au = Efb–sol. Also, it occurs under 900 nm light (ΔEp = 1.38 eV) at pH 7 (Efb–Au + ΔEp = +1.24) but not at pH 8 and 9 (Efb–Au + ΔEp = +1.13–+1.18). Therefore, the threshold exists at +1.18–+1.24 V. The difference between this threshold potential and the standard electrode potential for the formation of [AuCl4]− (+1.00 V vs. NHE) may be explained in terms of the reaction overpotential and/or the difference between Efb–Au and Efb–sol.
Footnote |
| † Present address: Department of Chemistry, School of Science and Technology, Kwansei Gakuin University, Sanda, Hyogo 669-1337, Japan. |
| This journal is © The Royal Society of Chemistry 2013 |