Limin
Wu
,
Jingfang
Zhou
* and
Haolan
Xu
*
Future Industries Institute, University of South Australia, Mawson Lakes Campus, SA 5095, Australia. E-mail: jingfang.zhou@unisa.edu.au; haolan.xu@unisa.edu.au
First published on 25th August 2016
Au nanoparticles with a small size, narrow size distribution and extraordinary colloidal stability were synthesized via a modified Brust–Schiffrin two phase method. Hydrophobic phosphorus based room temperature ionic liquids (RTIL) were introduced into the toluene phase and solely used as both phase-transfer agent and stabilizer, which significantly simplified the two-phase synthetic system. The synthesized Au nanoparticles are stable for more than two years. Even the thoroughly dried Au NPs can be easily re-dispersed in toluene. Surface characterizations of the Au@RTIL nanoparticles revealed that the amount of the adsorbed RTIL molecules and their degree of order on Au surfaces as well as their interactions with Au surfaces determine the size and stability of the Au@RTIL nanoparticles. The synthetic method and the mechanism presented here are of great importance to the development of the BS method, as well as the Au nanoparticle synthesis and applications.
The BS method involves transfer of AuCl4− from water phase to toluene phase, reduction of Au(III) to Au metal and stabilization of the generated Au NPs. Typically, tetraoctylammonium bromide (TOAB) is used as phase-transfer agent. However, TOAB is not an excellent stabilizer especially when its concentration is low. Sole utilization of TOAB in BS synthesis can't produce high quality Au NPs. To obtain highly monodisperse and stable Au NPs, additional stabilizer such as alkanethiols which can form strong bond with Au surface is required.14 However, the co-existence of TOAB, alkanethiols and NaBH4 in BS phase synthesis has raised ongoing debate regarding the mechanism of the Au nucleation and growth because all these reagents involve in the formation of precursor complexes, reduction, crystal growth and NP stabilization.20–23 Therefore, simplifying the BS synthesis and the corresponding growth mechanism is highly required.24,25 An ideal strategy is to use only one reagent to simultaneously play the roles of phase transfer agent and stabilizer during the synthesis. Herein, we develop a modified BS method to synthesize Au NPs in two-phase without utilization of TOAB and alkanethiols. Hydrophobic room temperature ionic liquids (RTILs) were selected to substitute and play the roles of TOAB and alkanethiols. RTILs are organic salts in liquid state at room temperature. RTILs are recognized as green and environment friendly liquid due to the very low vapour pressure, non-flammability, excellent thermal stability etc.26,27 It has been reported that some RTILs such as BMIM–PF6 can efficiently extract AuCl4− from aqueous solution.28 Concurrently, some water-soluble RTILs have been proven to be novel stabilizers for NPs in aqueous medium.29–31 The RTILs can form a robust protective layer to provide both steric and electrostatic repulsion against aggregation of NPs. Inspired by these two merits, we introduce hydrophobic RTILs into toluene phase in BS method to serve both as phase transfer agent and stabilizer for Au NPs synthesis. This strategy renders a relative simple synthetic system and produces high quality Au NPs.
Fourier transform infrared spectra (FTIR) were determined with a Nicolet 6700 at a resolution of 2 cm−1. The Au@RTIL NPs were deposited on to a NaCl disc followed by evaporation of toluene solution. Thermal Gravity Analysis (TGA) was performed with an Auto 2950 HR V6.1 A. The temperature range used was from 300 to 873 K.
Time-of-Flight Secondary Ion Mass Spectrometry (ToF-SIMS) experiments were performed using a Physical Electronics Inc. PHI TRIFT V nanoTOF instrument equipped with a pulsed liquid metal 79+Au primary ion gun (LMIG), operating at 30 keV energy. Experiments were performed under a vacuum lower than 5 × 10−6 Pa. “Bunched” Au1 instrumental settings were used to optimise mass resolution for the collection of +SIMS and −SIMS spectra. Surface analyses were performed at a number of locations per sample, typically using a 100 × 100 micron raster area. Five locations per sample were analysed to ensure a representative signal from the sample surface. Spectra were interrogated using WincadenceN software (Physical Electronics Inc.).
The size of the Au@RTIL NPs can be controlled by simply adjusting the amount of RTILs. For example, TEM images of the Au@P14,6,6,6NTf2 NPs clearly demonstrated the effect of the molar ratio of P14,6,6,6NTf2 to AuCl4− (R) on particle sizes (in this research, the concentration of AuCl4− is fixed). When R is 1, the diameter of the Au NPs is measured to be 8.8 ± 2.9 nm (Fig. 2a). When R is increase to 2, 4, and 8, the diameter of the Au NPs decreases to 6.5 ± 2.2 nm (Fig. 2b), 5.8 ± 2.4 nm (Fig. 1a), and 3.9 ± 1.7 nm (Fig. 2c) respectively. Correspondingly, the UV-Vis spectra of these Au NPs also show noticeable peak shifting (Fig. 2d). The plasmon absorption bands of Au@P14,6,6,6NTf2 NPs locate at 518, 517, 515 and 506 nm when R is 1, 2, 4 and 8 respectively, indicating the particle size become smaller with the increase of P14,6,6,6NTf2. The increase of P14,6,6,6NTf2 provides more ligands to stabilize Au surfaces which allows the formation of smaller particles with larger overall surface area. However, it is found that further increase of R to 16 induced little change in particle size (Fig. S4†), indicating the saturation of RTIL for Au synthesis.
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Fig. 2 TEM images of the Au@P14,6,6,6NTf2 NPs synthesized when R is (a) 1, (b) 2, (c) 8, and (d) their UV-Vis spectra. |
The colloidal stability of the obtained Au@RTILs NPs was investigated by monitoring the plasmon absorption change of the Au NPs solutions along with the storage time. The original plasmon absorption spectra of the Au@RTIL NPs are shown in Fig. S5,† from which one can see the narrow absorption peaks at around 517–520 nm for Au@P14,6,6,6NTf2, Au@P14,6,6,6Br, and Au@P14,6,6,6PF6 NPs, indicating the small particle sizes (5–10 nm) and narrow size distribution of Au NPs. These results agree well with the size measured by TEM and DLS. The Au@P14,6,6,6NH(CN)2 NPs shows a wide absorption peak, confirming the wide size distribution. When these Au NPs were stored for 30 days, slight change in the absorption intensity and peak position were observed for the Au@P14,6,6,6NTf2, Au@P14,6,6,6Br, and Au@P14,6,6,6PF6 NPs (Fig. 3a). As comparison the Au NPs synthesized with sole TOAB shows rather poor colloidal stability. The Au@TOAB NPs aggregated and precipitated out quickly within 2 days (Fig. S6†). It is worth noting that the Au@P14,6,6,6NTf2 NPs are still stable even after 2 years storage (Fig. 3b). The toluene was thoroughly evaporated after such a long period of storage, leaving behind the dried Au@P14,6,6,6NTf2 NPs. However, when toluene was added into the vial, the dried Au NPs were readily re-dispersed in the toluene. No obvious aggregation or precipitation of NPs was observed. This outstanding colloidal stability and re-dispersibility of Au@RTILs NPs should be originated from the superior stability, non-volatility and liquid state of the adsorbed RTILs on the Au surfaces.
To verify the presence of RTILs on Au NPs surfaces and investigate their roles in stabilization, TGA, FTIR, and ToF-SIMS analysis were conducted. As shown in Fig. 4, TGA measurement clearly depicts the weight loss of all the Au@RTIL NPs. The Au@P14,6,6,6NTf2 NPs (black curve) exhibits a weight loss (ΔW) of about 7.72%. Accordingly, the number of RTIL molecules (N) on each Au NPs can be roughly estimated as:
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Fig. 4 TGA curves of the Au@P14,6,6,6NTf2, Au@P14,6,6,6Br, Au@P14,6,6,6PF6 and Au@P14,6,6,6NH(CN)2 NPs. |
To further investigate the adsorption of RTILs and their degree of order on Au NP surfaces, FTIR spectra of the Au@RTIL NPs and the corresponding pure RTIL molecules were recorded and compared. As shown in Fig. 5, pure P14,6,6,6NTf2 shows typical FTIR spectra which is the same with reported data.32 The symmetric and asymmetric stretching vibrations of C–H of methylene of P14,6,6,6NTf2 are located at 2856 and 2928 cm−1 respectively. In the low frequency region, peaks are observed at 1468 cm−1 (–CH2– asymmetric bending); 1351 cm−1 (SO stretching); 1193 cm−1, 1138 cm−1 (–CF3); 1058.22 cm−1 (S
O stretching). The FTIR spectrum of Au@P14,6,6,6NTf2 NPs exhibits methylene stretching modes with slight lower wave numbers at 2849 and 2917 cm−1, indicating highly ordered alkyl chains on the surface of Au NPs. A band splitting of 1468 cm−1 into two peaks positions at 1471 and 1461 cm−1 was observed, indicating the orthorhombic subcell packing of chains with small defects.33 Judging together with the TGA result (high RTIL cover density on Au NPs surfaces), it is reasonable to propose that the Au NPs are densely surrounded by P14,6,6,6NTf2 shells, which provides strong steric hindrance thus rendering the Au NPs excellent stability. The FTIR spectra of Au@P14,6,6,6Br (Fig. S7a†), and Au@P14,6,6,6PF6 NPs (Fig. S7b†) all show the characteristic peaks of the corresponding RTILs, confirming the presence of RTILs on the surface of Au NPs. Slight shift of methylene stretching modes to lower wave numbers are also observed in the Au@P14,6,6,6Br and Au@P14,6,6,6PF6 NPs, indicating the ordered alkyl chains on Au surfaces. Similarly, these orderly arranged RTIL molecules lead to the excellent stability of the Au NPs. In contrast, it is noticed that the peaks of Au@P14,6,6,6NH(CN)2 NPs are highly identical with that of the pure P14,6,6,6NH(CN)2 (Fig. S7c†), which implies the weak interactions between the Au NPs and P14,6,6,6NH(CN)2, and the loose packing of the alkyl chains on Au NPs. This agrees well with the low RTIL molecular cover density derived from the TGA measurement, explaining the relatively poor quality of the Au NPs synthesized in the presence of P14,6,6,6NH(CN)2.
ToF-SIMS is a surface-sensitive method that provides elemental, chemical state, chemical fragment and molecular information from the solid surfaces. The average depth of analysis is approximately 1 nm. Herein the ToF-SIMS spectra of Au@P14,6,6,6NTf2, Au@P14,6,6,6Br, and Au@P14,6,6,6PF6 NPs were recorded to investigate the possible chemical interactions between the Au surface and RTILs molecules. Fig. 6 is the ToF-SIMS spectrum of Au@P14,6,6,6NTf2 NPs which reveals the presence of CH− (m/z = 13), O− (m/z = 16); C2H5+ (m/z = 29); Cl− (m/z = 35, 37); Au− (m/z = 197); Au+Cl− and AuCl2− (m/z = 232, 267) and CnH2n+2P (m/z = 397–485). The detected fragments of Au+Cl− and AuCl2− confirm the strong chemical interaction/bond between Au and Cl. The Cl is from the precursor AuCl4− but not the anion of RTIL, because the P14,6,6,6NTf2 does not contain any Cl. The fragment CnH2n+2P is from the cation (P14,6,6,6) of the RTIL. Therefore, it is safe to propose that in the Au@P14,6,6,6NTf2 NPs, the anion Cl− directly bonds to the Au surface and the cation of the RTIL (P14,6,6,6) with long carbon chain orderly arranges in the outer layer which produce a robust steric hindrance to stabilize the Au NPs. The ToF-SIMS spectrum of Au@P14,6,6,6PF6 NPs (Fig. S8†) also clearly show the fragments of Au+Cl−, AuCl2−, and CnH2n+2P(M+) from cation P14,6,6,6, indicating the similar surface layer structure with that of Au@P14,6,6,6NTf2 NPs. However, the ToF-SIMS spectrum of Au@P14,6,6,6Br NPs presents no fragments of Au+Cl− and AuCl2−, but the fragments of AuBrH−, AuBrH2−, AuBrH3− (m/z = 276–279); C2H2AuBr−, C2H4AuBr− (m/z = 304), C5H2AuBr−, C5H4AuBr− (m/z = 338, 340) (Fig. S9†). This confirms the existence of large amount of AuBr− fragments, indicating the strong chemical interaction/bond between Br and Au surfaces. The Br is from the anion of P14,6,6,6Br. The peak of CnH2n+2P(M+) from the cation of P14,6,6,6Br is also detected. According to these surface characterizations, it is clear that Au has strong chemical interaction with halide ions. As reported, there are unoccupied molecular orbital on the surface of the noble metal NPs. Halide ions with outermost lone pair electrons are strongly adsorbed on the Au surface creating a negatively charged layer.34 When the anion of RTIL is Br−, it directly binds to Au surfaces. The cation of RTIL orderly arranges in the outer layer. Therefore, both the cation and anion of RTIL involve in stabilizing Au NPs, leading to the outstanding stability. When the anion of RTIL is not Br−, the Cl− from the AuCl4− strongly binds to the Au surfaces, while the cation of the RTIL orderly arranges outside. This structure can also bring excellent colloidal stability. However, if the cations of RTIL are loosely packed in the outer layer, the stability of the Au NPs is relatively poor. The proposed surface layer structure of the as-prepared Au@RTIL NPs is shown in Fig. 7.
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Fig. 7 Schematic illustration of the proposed stabilization mechanism of an Au@RTIL NP. Note the anion of RTIL may be absent in the surface layers. |
Footnote |
† Electronic supplementary information (ESI) available: Digital photographs, TEM images, DLS size distribution, UV-Vis spectra, ToF-SIMs spectra of Au NPs, and table of RTILs. See DOI: 10.1039/c6ra17663a |
This journal is © The Royal Society of Chemistry 2016 |