Oksana
Zaluzhna
a,
Chris
Zangmeister
b and
YuYe J.
Tong
*a
aDepartment of Chemistry, Georgetown University, 37th & O Streets, NW, Washington DC 20057, USA. E-mail: yyt@georgetown. edu
bNational Institute of Standards and Technology, 100 Bureau Drive, Gaithersburg, MD 20899, USA
First published on 18th June 2012
We report the first successful synthesis of Au and Ag nanoparticles (NPs) with alkylselenocyanates as the source of protecting ligands. The resultant NPs were characterized to better understand the interfacial chemistry between the metal core and ligand by comparing and contrasting with the corresponding 2D self-assembled monolayers (SAMs).
Ciszek et al. have recently used organic thiocyanates as alternative precursors for forming 2 dimensional (2D) SAMs primarily on Au but also on Ag and Pt and determined that thiocyanates assemblies resemble thiolate SAMs.27,28 It was demonstrated that the surface coverage remains better for widely-used thiols-generated SAMs than for thiocyanates-generated SAMs, yet thiocyanate-generated SAMs showed superior stability on the surfaces and avoided undesired polymerization processes.27,29,30 Among others, the main challenge in characterizing the thiocyanate-generated SAMs was to identify and quantify the possible presence of (CN) species. The authors argued that the surface morphology played a significant role in the expulsion of (CN)ads from metal surfaces, i.e., SAMs on evaporated Au surface had less residual nitrogen than the stripped template.28,29
Inspired by the work discussed in the previous paragraph, we used the same type of ligand to synthesize metal (Au and Ag) NPs via the BSM and reported the successful outcome in this Communication. To our best knowledge, the only work that has dealt with organo selenocyanates as a starting precursor for generating potential protecting ligands for NPs was the work by Lim et al. but in a very different context.31 They investigated the adsorption of nitrophenyl selenocyanate on the surface of pre-formed Au NPs stabilized by citrate via ligand exchange and compared it with benzeneselenol.31 Despite the lack of TEM image evidence, the authors assumed that the size of the colloidal ensemble remained unchanged following the ligand exchange, i.e., 15 nm spherical NPs.31 In this Communication, we focus on using the general BSM to synthesize metal (Au and Ag) NPs with alkylselenocyanates as the starting molecular precursor for the final stabilizing ligand and to compare and contrast the formation chemistry of the 3D SAM analogues to that of the corresponding 2D SAMs.
Several alkylselenocyanates ligands, such as C6H13SeCN, C8H17SeCN, and C12H25SeCN, were synthesized32 (see the Electronic Supporting Information, ESI†) and characterized via1H NMR (Fig. S1), 13C NMR (Fig. S2), IR (Fig. S3), Raman (Fig. S4), and 77Se NMR (Fig. S5). For the purpose of this Communication, only dodecylselenocyanate, i.e., C12H25SeCN or briefly C12SeCN, as the starting ligand will be discussed as a representative case to illustrate our main findings. Both one-phase (1p) and two-phase (2p) BSMs were employed to synthesize the Au NPs. While the 2p BSM was successful in producing Au NPs (Fig. S6, ESI†), the 1p BSM produced more homogenous NPs with C12SeCN. Therefore, the latter will be the focus of the study and discussion here. For details on other syntheses, readers are referred to the ESI,† specifically Fig. S7 for the results of other 1p syntheses.
TEM, UV-Vis, and size distribution data are presented in Fig. 1 for the C12Se-protected Au NPs synthesized by the 1p BSM (we will omit CN in naming NPs below because CN was a very minor species there, vide infra). The resultant NPs were homogenous, with an average particle size of 2.0 ± 0.3 nm (Fig. 1a), and exhibited a narrow size distribution (Fig. 1b). The UV-Vis did not display a clear surface plasmon resonance peak around 500–520 nm due to the small size of NPs (Fig. 1c).33
Fig. 1 (a) TEM image, (b) size distribution histogram, and (c) UV-Vis spectrum of the 2.0 ± 0.3 nm C12Se–Au NPs. |
The obtained NPs were characterized via1H NMR, IR, and XPS. Fig. 2 displays the 1H NMR results for the NPs (Fig. 2a) and the free ligand (Fig. 2b). The triplet peak corresponding to the protons in –H2C–SeCN at 2.09 ppm in the free ligand (Fig. 2b) disappeared in the NP spectrum (Fig. 2a), indicating that the organic moiety is bound to the metal surface via Se. Also, note that the broadening and down-field shift of the alkyl chain peaks at 1.0 to 1.5 ppm is indicative of the ligand bound to the NPs.34 Unfortunately, 13C NMR lacked the sensitivity to determine the presence of CN species within the NPs sample, as illustrated by the difficulty to observe the CN peak even in the free RSe–CN ligand (Fig. S2b†).
Fig. 2 1H NMR spectra of (a) C12Se–Au NPs, and (b) pure C12SeCN ligand. |
The IR characterization was performed to determine whether the CN species were present on the Au NPs surface. As shown in Fig. 3, the cyanide peak at 2150 cm−1 (Fig. 3b) that was present in the free ligand disappeared completely in the NPs sample (Fig. 3a). That is, within the detection limit of IR, no residual CN was observed after the formation of Au NPs. The disappearance of the Se–C (trans) vibrational band at 630 cm−1 in the Au NPs sample is also indicative of the formation of Se–Au bond. The characteristic triplet peaks of methylene/methyl stretching frequencies appear at νs(CH2) 2852 cm−1, νas(CH2) = 2924 cm−1, and νas(CH3) = 2956 cm−1, respectively. These should be compared to the corresponding values of 2D SAMs:30 νs(CH2) = 2880 cm−1, νas(CH2) = 2935 cm−1, and νas(CH3) = 2965 cm−1. The smaller (red-shifted) frequencies observed on the Au NPs suggest that the alkylselenoate formed a more ordered monolayer structure on the NPs than on the Au(111) surface.35
Fig. 3 IR spectra of (a) C12SeCN–Au NPs, and (b) pure C12SeCN ligand. |
For their work on 2D SAMs, Ciszek et al. detected the presence of a very small amount of residual CN by using XPS and proposed the existence of two kinds of cyanides within the samples: the adsorbed cyanide (CNads) and an intermediate form absorbed on the surface during the etching of the metal (Au(CN)) intermediate species with vibrational IR band at ∼2160 cm−1,28 although their respective quantification was proved to be challenging. Choi et al. had also found it challenging to identify and quantify the presence of cyano species in their octylthiocyanate-generated SAMs on Au(111).29 They predicted that the CN bands could be more readily observed on the surface of Au via SERS, though the amount of CN was impossible to be determined.29,31 Our IR results also suggest that there is little, if any, cyanide species present in the NPs sample, since no observable CN vibrational peaks were present in the spectra.
XPS analysis, as a more sensitive tool of elemental analysis, was used to further analyze the ligand-metal characteristics (Fig. 4 and Fig. S8 in the ESI†). Fig. 4a displays the XPS spectra of Se 3d5/2 with a binding energy of 55.3 eV, which has been observed for the C12Se–Au NPs synthesized with dialkyl-diselenides as the starting ligand.15,24 The same binding energies for the Au 4f7/2 doublet (87.75 eV and 84.05 eV respectively, Fig. S8) were also observed. Altogether, these binding energies lead to the conclusion that the organic moiety is indeed bound to the Au surface via the chalcogen and the Au NPs synthesized with alkylselenocyanate and dialkyl-diselenide are essentially the same.
Fig. 4 XPS of (a) Se d5/2, and (b) N 1s region in C12SeCN–Au NPs. |
Furthermore, XPS was used to investigate the existence of (CN) species within the Au NPs. As mentioned previously, Ciszek et al. proposed the existence of two types of cyanides within the SAMs samples, i.e., CNads on Au (with XPS binding energy of N 1s electron = 397.9 eV) and Au(CN) intermediate species (with XPS binding energy of N 1s = 399.5 eV).28 For our study, a weak and noisy N 1s XPS signal was observed at ∼399 eV in our samples (Fig. 4b) as one broad peak in the spectra. Unfortunately, the weak signal and peak broadening (Fig. 4b) on the C12Se–Au NPs sample made the differentiations of the two possible cyano species impossible. Based on these results, we can ascertain that the Au NPs synthesized with alkylselenocyanate are predominantly protected by alkylselenolate, while (CN) species exist in a trace amount that cannot be determined quantitatively.
Additionally, TGA was performed on the NPs and showed a two-step mass loss (Fig. S9†). The first step occurred at ∼180 °C of about 30% mass loss, and the second at ∼350 °C of about 13% mass loss. The first mass-loss temperature corresponded closely to the loss of the organic alkyl chain with Se as an anchoring element, as previously reported in the literature.24 The second mass loss, on the other hand, warrants more investigation, since the mass loss is too large to correspond to the cyano species.
We also carried out similar, but less extensive synthesis of Ag NPs with C12SeCN using 2p BMS. Despite being proved much more challenging to synthesize than Au NPs in terms of reproducibility of size homogeneity, Fig. 5 presents the TEM image, size distribution histogram, and UV-Vis spectrum of our best sample. While the size of the synthesized Ag NPs (2.9 ± 0.3 nm) is larger than that of the corresponding Au NPs (2.0 ± 0.3 nm), very similar IR (disappearance of the C–N and the Se–C stretching bands in the Ag NPs, Fig. S10) and TGA (the two-step desorption, Fig. S11) were observed. The vibrational frequencies of the methyl/methylene triplet were 2846 cm−1, 2916 cm−1, and 2954 cm−1, respectively. These frequencies are further red-shifted as compared to those on the Au NPs, suggesting that even more ordered monolayer was formed on the Ag NPs.35 All these data indicate that the ligand monolayer on the Ag NPs shares more structural and chemical similarity than difference with its counterpart on the Au NPs.
Fig. 5 (a) TEM image, (b) size distribution histogram, and (c) UV-Vis spectrum of the 2.9 ± 0.3 nm C12Se–Ag NPs. |
Footnote |
† Electronic Supplementary Information (ESI) available: Experimental details and data: Fig. S1–S11. See DOI: 10.1039/c2ra20729j/ |
This journal is © The Royal Society of Chemistry 2012 |