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Thiolate-protected Au38(SR)24 nanocluster: size-focusing synthesis, structure determination, intrinsic chirality, and beyond

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Published/Copyright: January 17, 2014

Abstract

Thiolate-protected Au nanoclusters with core diameters smaller than 2 nm have captured considerable attention in recent years due to their diverse applications ranging from biological labeling to photovoltaics and catalysis. This new class of nanomaterials exhibits discrete electronic structure and molecular-like properties, such as HOMO-LUMO electronic transition, intrinsic magnetism, chiroptical properties, and enhanced catalytic properties. This review focuses on the research into thiolate-protected Au38(SR)24 – one of the most representative nanoclusters, including its identification, size-focusing synthesis, structure determination, and intrinsic chirality. The properties of two size-adjacent Au nanoclusters [Au40(SR)24 and Au36(SR)24] are also discussed. The experimental and theoretical methodologies developed in studies of the Au38(SR)24 model nanocluster open up new opportunities in the synthesis and properties investigation of other atomically precise Aun(SR)m nanoclusters.

Introduction

Ultrasmall Au nanoparticles (ca. 1-2 nm core size), often called Au nanoclusters, have become one of the important types of nanomaterials targeted in current nanoscience research [125]. Unlike their larger counterpart – crystalline Au nanoparticles with size above 2 nm, whose optical properties are dominated by surface plasmon resonances due to excitation of electrons in the continuous conduction band, Au nanoclusters instead exhibit discrete electronic structure and molecular-like properties [2636],such as HOMO-LUMO electronic transition [1, 37, 38], intrinsic magnetism [29, 39], chiroptical properties [4042], and enhanced catalytic properties [4345]. Considering the extreme sensitivity of the properties of Au nanoclusters to the number of Au atoms in the particle, these ultrasmall nanoclusters are better represented as AunLm, where n is the number of Au atoms and m the number of ligands (such as thiolate, –SR).

Early work on thiolate-protected Au nanoparticles was pursued in the 1990s [4649]. Brust et al. developed a two-phase protocol for preparing thiolate-protected Au nanoparticles. However, the nanoparticles obtained at that time were quite polydisperse (typically ranging from ~2 to 5 nm) [46]. Mirkin et al. developed thiolated-DNA for functionalization of Au nanoparticles, which are extremely robust and have acquired wide applications in sensing, biological labeling, and biomedicine [47]. In 1996, Whetten et al. synthesized a series of narrow size distributed nanoparticles in the range of 1.0–3.5 nm by solvent fractionation, and several distinct critical sizes were identified by laser desorption-ionization mass spectrometry (LDI-MS) [48]. The atomically monodisperse Au nanoclusters were not obtained at that time.

Au38(SR)24 nanoclusters as the first Au nanoclusters that were observed to show the molecular-like properties [26, 27] have been extensively studied. The history of Au38(SR)24 can be traced back to 1997 [26]. A series of ultrasmall Au nanoparticles were isolated using solvent fractionation. The smallest Au nanoparticles have a Au core mass of ~8 kDa determined by LDI-MS (Au core refers to AuxSy). However, due to the limitation of characterization techniques, the formula of ~8 kDa species was not determined. Whetten et al. estimated the ~8 kDa species consists of ~38 Au atoms [26]. After that, a sample of ~8 kDa Au:SC6H13 species was analyzed by X-ray photoemission spectroscopy (XPS), indicating it had an elemental composition of 62 % Au and 38 % S. If the Au core has 38 Au atoms, the number of thiol ligands should be 23–24 [50]. The first theoretical model of Au38(SR)24 was proposed based on the assignment of this formula [50].

In 1998, Chen et al. observed the molecular-like charging properties for Au38(SR)24, where the HOMO-LUMO energy gap is nearly 0.9 eV [27]. It is noted that some early work (prior to 2007) from Murray and co-workers erroneously assigned another ultrasmall nanocluster – Au25(SR)18 as Au38(SR)24 due to their similar molecular like properties and Au/S ratio [5155]. Advances in electrospray ionization-mass spectrometry (ESI-MS) and matrix-assisted laser desorption ionization-mass spectrometry (MALDI-MS) facilitated the successful determination of intact cluster ions without fragmentation. These techniques provided the exact composition assignment with atomic precision [56, 57]. Now it is easy to distinguish these two nanoclusters (Au25 and Au38).

After successful crystal structure determination of Au25(SR)18 by the Murray [58] and Jin [37] groups in 2008, some researchers doubted whether the Au38(SR)24 really existed. Shortly after that, the formula of Au38(SR)24 was unambiguously identified by the Tsukuda group with ESI-MS. A series of Au38(SCnH2n+1)24 (n = 6, 10, 12, and 18) clusters were isolated using recycling size-exclusion chromatography (SEC) [59] or solvent fractionation [60]. The hexanethiolate-protected Au38 clusters were also prepared by etching polydispersed Au clusters with excess thiol; the formula was assigned as Au38(SC6H13)22 due to the loss of ligands in MALDI-MS characterization [61]. However, the above synthesis suffered from a complicated purification process and low yield (<1 %). In order to study the fundamental properties and explore the potential applications of Au38(SR)24 nanoclusters, it was therefore highly desirable to achieve a more efficient large-scale synthesis.

Size-focusing synthesis of Au38(SR)24 nanoclusters

On the basis of the early work from various groups, a new size-focusing method was developed to synthesize Au38(SR)24 nanoclusters with high yield (~25 %, Au atom basis) [6264]. This method was based on the thermal thiol etching process, as shown in Fig. 1a. In the first step, glutathione (GSH) protected Aun(38≤n≤~100) nanoclusters were prepared by reducing Au(I)-SG in acetone solution; in the second step, the size-mixed Aun(SG)m nanoclusters reacted with excess phenylethylthiol (PhC2H4SH) for ~40 h at 80°C and monodisperse Au38(SC2H4Ph)24 clusters were finally obtained [63].

Fig. 1 
          (a) Schematic diagram of a two-step procedure for synthesizing monodisperse Au38(SC2H4Ph)24 nanoclusters in high yield. (b) MALDI-mass spectrum of Aun(SR)m before and after thiol etching. Adopted with permission from ref. [63].
Fig. 1

(a) Schematic diagram of a two-step procedure for synthesizing monodisperse Au38(SC2H4Ph)24 nanoclusters in high yield. (b) MALDI-mass spectrum of Aun(SR)m before and after thiol etching. Adopted with permission from ref. [63].

Figure 1b shows the size-focusing mechanism by MS. The size-focusing process occurred over the etching-induced growth process. The formula and high purity of Au38(SC2H4)24 nanoclusters were further confirmed by ESI-MS, MALDI-MS, and SEC. The major advance of this method was the control of size distribution of Aun(SR)m mixture before the thermal thiol etching step. In previous procedures [60, 65], a mixture of Aun(SR)m resulted with the modified Brust method, and the size distribution of Aun(SR)m was quite broad. Even after thermal etching, it still contained several stable species in the solution, including Au38(SR)24, Au144(SR)60, and others. The separation process was nontrivial and time-consuming. To solve this problem, the initial size distribution of Aun(SR)m (i.e., “precursors” for the size-focusing step) was adjusted by controlling the type of thiol ligands and reaction solvent. The combination of glutathione as thiol ligands and acetone as solvent was finally chosen after screening various thiols and solvents [63]. The Aun(SG)m mixture cannot be dissolved in acetone. Therefore, after the nucleation of Aun(SG)m, the nanoclusters immediately precipitated out of solution and the further growth was inhibited. The size distribution of the formed Aun(SG)m ranged from Au38 to Au~100. In the subsequent thermal thiol etching process, those relatively large Au nanoclusters were found to be decomposed and converted to Au38(SR)24 nanoclusters. This process was largely driven by thermodynamic stability of Au38(SR)24, which was the most robust species in this particular size range. The final product only contained monodisperse Au38(SR)24 and Au(I)-SR polymer; no larger or smaller nanoclusters were detected. The Au(I)-SR polymer was poorly soluble in almost all solvents, hence easy to separate from the product. This method was highly reproducible [41, 6668] and versatile for various alkanethiols as ligands for Au38 nanoclusters, i.e., Au38(CnH2n+1)24 (n = 4, 6, 8, 12, 16) [69, 70]. The size-focusing method developed in the preparation of Au38(SR)24 cluster has been successfully applied in the synthesis of other magic-sized Aun(SR)m nanoparticles with molecular purity, including Au28(SR)20 [71], Au55(SR)31 [72], Au144(SR)60 [73, 74], and Au333(SR)79 [18], etc.

The truly monodisperse Au38(SC2H4Ph)24 nanocluster displays distinct molecular-like optical and electrochemical properties [63]. The UV-vis-NIR absorption spectrum exhibits a series of peaks at 1050 nm (1.18 eV), 750 nm (1.66 eV), 620 nm (2.00 eV), 560 nm (2.21 eV), 520 nm (2.39 eV), and 490 nm (2.53 eV), as shown in Fig. 2a. By extrapolating the lowest energy absorption peak to zero absorbance, the optical energy gap (HOMO-LUMO gap) is determined to be 0.92 eV (Fig. 2a inset). The highly structured optical spectrum serves to give convenient “fingerprints” for one to quickly identify Au38(SR)24 nanoclusters (e.g., in routine synthesis). Figure 2b shows differential pulse voltammogram (DPV) of Au38(SC2H4Ph)24 nanoclusters. The electrochemical energy gap is ~1.2 V, i.e., the gap between the first oxidation wave (ox1, +0.48 V) and the first reduction wave (re1, -0.71 V). The charging energy can be estimated from the difference between the first oxidation wave (ox1, +0.48 V) and the second oxidation wave (ox2, +0.68 V), i.e., 0.68 –0.48 = 0.2 V. The HOMO-LUMO gap is thus 1.0 V after subtracting the charging energy from the electrochemical energy gap, which is very close to the optical energy gap (0.92 eV).

Fig. 2 
          (a) UV-vis-NIR absorption spectrum of Au38(SC2H4Ph)24 nanoclusters; the inset shows the spectrum on the energy scale (eV). (b) Differential pulse voltammogram (DPV) at room temperature. Adapted with permission from ref. [63].
Fig. 2

(a) UV-vis-NIR absorption spectrum of Au38(SC2H4Ph)24 nanoclusters; the inset shows the spectrum on the energy scale (eV). (b) Differential pulse voltammogram (DPV) at room temperature. Adapted with permission from ref. [63].

Structure determination of Au38(SR)24 nanoclusters

These atomically precise nanoclusters allow for the growth of X-ray quality single crystals and subsequent determination of their total structure (core plus surface) by X-ray crystallography [2, 37, 58, 75, 76]. Understanding the total structure, in particular the surface atom arrangement, is of paramount importance in order to study the catalytic properties of metal nanoclusters for future design of highly efficient catalysts [43, 7780]. In order to determine the total structure by single crystal X-ray diffraction, crystallization of nanoclusters is the critical step, but unfortunately the growth of single crystals, in general, has long been a huge challenge. Significantly, the Au38(SR)24 nanoclusters with molecular purity achieved by the size-focusing methodology have led to successful crystallization [81]. The unit cell of Au38(SCH2CH2Ph)24 crystals contains a pair of enantiomeric nanoparticles (left- and right-handed, Fig. 3).

Fig. 3 
          Crystal structure of Au38(SC2H4Ph)24 nanoclusters. Adapted with permission from ref. [81]. A single crystal (~0.2 mm) was shown in the photograph (upper right).
Fig. 3

Crystal structure of Au38(SC2H4Ph)24 nanoclusters. Adapted with permission from ref. [81]. A single crystal (~0.2 mm) was shown in the photograph (upper right).

The left-handed isomer is chosen for a detailed analysis of the Au38 structure. As shown in Fig. 4, the nanocluster shows a prolate shape (diameter ~0.8 nm, length ~1.1 nm, Au center-to-center distances). The core of Au38(SR)24 consists of a face-fused biicosahedral Au23 motif (13 + 13 – 3 = 23), Fig. 4a. The fusion of the two icosahedra occurs along a common C3 axis. The rod-like Au23 kernel is structurally strengthened by three monomeric staples (–SR-Au-RS–) (Fig. 4b). Then, the top icosahedron is further capped by three dimeric staples (–SR-Au-SR-Au-RS–) (Fig. 4c), which are arranged in a rotating fashion, like a tri-blade “propeller”. A similar arrangement of the other three staples is found on the bottom icosahedron, but the bottom “propeller” rotates by ~60° relative to the top one, forming a staggered dual-propeller configuration (Fig. 4d). The entire nanoparticle becomes chiral due to the rotative arrangement of the dimeric staples, that is, one enantiomer is clockwise and another is anti-clockwise. The determination of the crystal structure of the Au38(SR)24 nanoparticle paves the way for the deep understanding of its electronic and catalytic properties.

Fig. 4 
          Structure analysis of Au38(SR)24 nanoclusters. (a) Au23 core, (b) Au23 core with three monomeric Au(SR)2 staples, (c) Au23 core with three dimeric Au2(SR)3 staples, (d) overall Au38S24 framework. Color labels: yellow, S; all the other colors are for Au atoms in different positions. The carbon tails (–CH2CH2Ph) are not shown for clarity. Adapted with permission from ref. [81].
Fig. 4

Structure analysis of Au38(SR)24 nanoclusters. (a) Au23 core, (b) Au23 core with three monomeric Au(SR)2 staples, (c) Au23 core with three dimeric Au2(SR)3 staples, (d) overall Au38S24 framework. Color labels: yellow, S; all the other colors are for Au atoms in different positions. The carbon tails (–CH2CH2Ph) are not shown for clarity. Adapted with permission from ref. [81].

It is worth mentioning that several candidate structures had been proposed by theoretical chemists. In 1999, Häkkinen et al. proposed a structure of Au38(SR)24 by placing 24 isolated thiolates on the surface of a truncated octahedron containing 38 Au atoms [50]. After that, Garzon [40, 82, 83] Jiang [84, 85], Tsukuda [60], Zeng [86], and Aikens [87] proposed several structures with symmetric or disordered Au core. The energy difference between Häkkinen’s original model in 1999 to Zeng’s model in 2008 is ~9 eV, a substantial reduction in energy (i.e., Zeng’s model being significantly more stable) [88]. Of them, the models predicted by Zeng and Aikens showed good agreement with the crystal structure. Recently, a theoretical explanation for the unusual stability of Au38(SR)24 cluster was reported [89]. Based on the super valence bond model, the 23c-14e double-icosahedral Au23(+9) core of Au38(SR)24 is proved to be a superatomic molecule, which is analogous to the F2 molecule in both molecular orbital (MO) diagrams and bonding patterns [89].

Zhang and co-workers reported solution-phase X-ray absorption spectroscopy (XAS) studies of Au38(SR)24 nanoclusters. Distinct solvation effects on the structure and bonding of Au-thiolate clusters were observed [90]. With respect to bimetal nanoclusters, two-Pd-atom doping of Au38(SC2H4Ph)24 has been reported [91, 92], and highly pure Pd2Au36(SC2H4Ph)24 clusters were successfully isolated, in which two Pd atoms were doped at the two center positions of Au38(SC2H4Ph)24. The stability investigation revealed that Pd2Au36(SC2H4Ph)24 was more robust than the homo-Au cluster Au38(SC2H4Ph)24 against degradation in solution and core etching by thiols [92]. In addition, the studies of selenolate-protected Au38 clusters found that a highly pure form of Au38(SeC12H25)24 could be synthesized by replacing all the SC2H4Ph ligands of Au38(SC2H4Ph)24 with SeC12H25, and selenolate-protected Au38 clusters showed the same degree of stability as thiolate-protected Au38 clusters [93].

Chirality of Au38(SR)24 nanoclusters

The Au38(SCH2CH2Ph)24 nanocluster shows intrinsic chirality. The chirality of Au38(SR)24 originates from the dual-propeller-like distribution of the six dimeric Au2(SR)3 staples, with one enantiomer exhibiting clockwise (L-) and the other anti-clockwise (R-) arrangements [81]. To probe the internal chiral structure of Au nanoclusters, circular dichroism (CD) is, generally speaking, a good method, but the racemic pair of Au nanoclusters results in a net zero signal. That was why the chiral structure of Au38 nanoclusters was not revealed until the determination of their crystal structure. The determination of crystal structures of nanoclusters is still highly challenging since it is very difficult to culture high-quality single crystals of Au nanoclusters. It is thus highly desirable to develop an analytical method to detect the intrinsic chirality, especially in racemic mixtures. Recent research showed that NMR spectroscopy was capable of probing the nature of chiral nanoclusters using the diastereotopicity induced in the α-CH2 protons of the –SCH2CH2Ph chains (Fig. 5) [94].

Fig. 5 
          (a) 1D NMR of Au38(SCH2CH2Ph)24 nanoclusters (1H-13C HSQC). The α-CH2 and β-CH2 are as labeled (see the top of panel A); 1–4 denote the four sets of ligands; a and b represent each diastereotopic proton for each carbon (α- or β-CH2) in the four sets of ligands. (b) Diastereotopicity in the CH2 protons of the ligands on nanoclusters (chiral metal-core-induced diastereotopicity). Adapted with permission from ref. [94].
Fig. 5

(a) 1D NMR of Au38(SCH2CH2Ph)24 nanoclusters (1H-13C HSQC). The α-CH2 and β-CH2 are as labeled (see the top of panel A); 1–4 denote the four sets of ligands; a and b represent each diastereotopic proton for each carbon (α- or β-CH2) in the four sets of ligands. (b) Diastereotopicity in the CH2 protons of the ligands on nanoclusters (chiral metal-core-induced diastereotopicity). Adapted with permission from ref. [94].

The intrinsically chiral Au38(SCH2CH2Ph)24 and nonchiral Au25(SCH2CH2Ph)18-TOA+ nanoclusters were used as two model systems to investigate how the NMR spectroscopy correlates with the nature of chirality in nanoclusters.

From 1D to 2D NMR of Au38(SCH2CH2Ph)24 nanoclusters, four sets of PhCH2CH2S– ligands were detected, corresponding to four different chemical environment of ligands. Of them, three sets of –SR ligands come from the dimeric –SR-Au-SR-Au-SR– staples and one set of –SR ligands comes from the monomeric –SR-Au-SR– [94]. The chiral Au38(SR)24 clusters showed different 1H signals for the two germinal protons in the α-CH2 group of the ligand, and the same for the β-CH2, so-called diastereotopicity. For α-CH2, a chemical shift difference of up to ~0.8 ppm for each germinal proton was observed (Fig. 5a). As for the nonchiral Au25(SCH2CH2Ph)18-TOA+ clusters, we found that two chemically inequivalent sets of –SCH2CH2Ph ligands, which were corresponding to the interior and exterior sites of the ligands in the dimeric staples. However, no diastereotopicity was detected. Two protons of each CH2 group are chemically equivalent, indicating nonchiral Au25 core [94]. This diastereotopicity principle will allow for future identification of intrinsically chiral nanoclusters prior to crystal structure determination.

The separation of enantiomers of Au38(SCH2CH2Ph)24 by high-performance liquid chromatography (HPLC) column was reported by Bürgi and co-workers [41]. The racemic Au38(SCH2CH2Ph)24 nanoclusters were separated by using a chiral cellulose-based analytical HPLC column and hexane/isopropanol (80:20) as eluent at room temperature. As shown in Fig. 6a, two well-separated peaks are observed at 8.45 and 17.45 min, corresponding to enantiomers 1 and 2. The UV-vis spectra of racemic clusters, enantiomers 1 and 2 are identical (Fig. 6b). The CD spectra of enantiomers 1 and 2 show perfect mirror images, and 11 clear signals are observed between 230 and 800 nm (Fig. 6c) [41]. These CD peaks match well with transitions in the absorption spectrum at room temperature [63] and at low temperature [95]. The strong anisotropy factor (up to 4×10–3) indicates that the intrinsic chirality due to ligand and surface Au atom arrangements can contribute significantly to the net optical activity (Fig. 6d) [41].

Fig. 6 
          (a) HPLC-chromatogram and (b) UV-vis spectra of HPLC-separated rac-Au38(SCH2CH2Ph)24. (c) CD spectra of enantiomers 1 (black) and 2 (red) and the racemic Au38(SCH2CH2Ph)24 (blue) before separation; (d) corresponding anisotropy factors of enantiomers 1 and 2 and of the racemate. Adapted with permission from ref. [41].
Fig. 6

(a) HPLC-chromatogram and (b) UV-vis spectra of HPLC-separated rac-Au38(SCH2CH2Ph)24. (c) CD spectra of enantiomers 1 (black) and 2 (red) and the racemic Au38(SCH2CH2Ph)24 (blue) before separation; (d) corresponding anisotropy factors of enantiomers 1 and 2 and of the racemate. Adapted with permission from ref. [41].

Bürgi et al. also reported the racemization of intrinsically chiral Au38(SCH2CH2Ph)24 nanoclusters at modest temperature (40–80°C) [96]. The drastic surface rearrangement took place without significant decomposition. The determined activation energy for the inversion reaction was only 28 kcal/mol, which indicated that the process occurred without complete break of the Au–S bond [96]. The ligand exchange between chiral R-1,1′-binaphthyl-2,2′-dithiol (R-BINAS) and racemic Au38(SCH2CH2Ph)24 was investigated. It was found that this process was diastereoselective with a preference of R-BINAS for the left-handed enantiomer [66]. The partial exchange of dithiol (R-BINAS) made the Au-thiolate interface more rigid and effectively stabilized the cluster against inversion [97].

Size-adjacent nanoclusters – Au40(SR)24 and Au36(SR)24

Au38(SR)24 is not the only cluster in the core mass ~8 kDa species. Indeed, Au40(SR)24 is another member in the ~8 kDa species. In the size-focusing synthesis of Au38(SCH2CH2Ph)24, by applying a shorter thermal thiol etching time (~18 h), instead of ~40 h, Au40(SCH2CH2Ph)24 was found to co-exist with Au38(SCH2CH2Ph)24 and can be isolated by SEC [98]. On the other hand, the complete ligand exchange from –SCH2CH2Ph to –SPh-t-Bu induced the significant size and structure conversion from Au38(SCH2CH2Ph)24 to Au36(SPh-t-Bu)24 [99, 100].

The synthesis and isolation of Au40(SCH2CH2Ph)24 clusters required three main steps [98]. Aun(SG)m mixture (38≤n≤~100) was first prepared by reducing Au(I)-SG polymer with NaBH4 in an acetone solution. Then, the obtained Aun(SG)m mixture was etched with excess thiol (PhCH2CH2SH) at 80°C for ~18 h. The starting polydispersed Aun(SR)m clusters were gradually converted to Au38(SCH2CH2Ph)24 and Au40(SCH2CH2Ph)24 clusters due to higher stability of these two clusters than other sizes in the distribution. Without further etching, both Au38(SCH2CH2Ph)24 and Au40(SCH2CH2Ph)24 were present in the product and successful separation was achieved by SEC [98]. Figure 7a shows a typical SEC chromatograph of ~18 h etched product, in which two peaks (centered at 14.0 and 14.4 min) were observed. The MALDI-MS and on-line recorded UV-vis spectra indicated that 12.5 to 14.0 min eluate was pure Au40(SCH2CH2Ph)24, the 14.4 to 15.6 min eluate was pure Au38(SCH2CH2Ph)24, and the in-between eluate is the mixture of these two species [98]. Similarly, Bürgi also reported the SEC for semipreparative scale separation of Au38(SR)24 and Au40(SR)24 [101].

Fig. 7 
          (a) SEC chromatograms of nanoclusters (b) MALDI mass spectra of the crude product(a) and isolated Au40(SR)24 (b) and Au38(SR)24 (c) nanoclusters. Adapted with permission from ref. [98].
Fig. 7

(a) SEC chromatograms of nanoclusters (b) MALDI mass spectra of the crude product(a) and isolated Au40(SR)24 (b) and Au38(SR)24 (c) nanoclusters. Adapted with permission from ref. [98].

The optical properties of isolated Au40(SC2H4Ph)24 clusters were also investigated. Au40(SC2H4Ph)24 does not show prominent peaks in the absorption spectrum, in which only three steps at ~2.2, 3.2, and 4.4 eV were observed. The HOMO-LUMO gap is estimated to be ~1.0 eV from optical absorption [98]. The enantioseparation of Au40(SCH2CH2Ph)24 was successfully achieved by using chiral HPLC [102]. The chiroptical responses of two separated enantiomers with achiral thiolate ligands (PhCH2CH2SH) demonstrated that Au40(SR)24 also has an intrinsically chiral structure [102]. Based on the experimental characterization of Au40(SR)24 via ligand exchange, chiroptical spectroscopy, and transmission electron microscopy, Häkkinen et al. proposed two models for the structure of Au40(SR)24 cluster [103]. Both of them contained a Au26 core, six monomeric –RS-Au-SR– staples, and four dimeric –RS-Au-SR-Au-SR– staples. It is worth mentioning that Jiang also studied the structures of Au40(SR)24 based on the staple-fitness concept and found a most promising model which contains a Au25 core with three monomeric staples and six dimeric staples. The alternative model with Au25 core is more stable than the previously proposed model with Au26 core [9].

Of note, we found that the isolated Au40(SCH2CH2Ph)24 can be converted to Au38(SCH2CH2Ph)24, which explains why the ~40 h long size-focusing product did not contain Au40(SCH2CH2Ph)24. Nevertheless, Au40(SCH2CH2Ph)24 is quite stable (though somewhat less than Au38(SCH2CH2Ph)24), and future work may reveal its structure. A comparison with the structure of Au40(SCH2CH2Ph)24 would be interesting.

The availability of atomically precise Au38(SCH2CH2Ph)24 nanoclusters provided new starting materials for the synthesis of different-sized nanoclusters via ligand exchange process [99]. Recently, the molecularly pure Au36(SPh-t-Bu)24 was synthesized by performing thiol-to-thiol ligand exchange with 4-tert-butylbenzenethiolate (denoted as SPh-t-Bu) using Au38(SCH2CH2Ph)24 as starting clusters. The crystal structure of Au36(SPh-t-Bu)24 was successfully determined by single-crystal X-ray crystallography [100]. Surprisingly, the structure of Au36(SPh-t-Bu)24 is significantly different from that of Au38(SCH2CH2Ph)24. The Au36(SR)24 cluster contains a truncated FCC tetrahedral Au28 kernel. The exposed (111) and (100) facets in Au28 kernel are capped by a new type of thiolate binding mode, that is, 12 of the 24 ligands bind to the underlying Au atoms on the (100) facets in a simple bridging mode, and the remaining 12 thiolates forming the known dimeric staple motifs on the (111) facets [100]. First-principle DFT calculations reveal a large HOMO-LUMO energy gap (approximately 1.7 eV, c.f. 0.9 eV for its parent cluster Au38(SCH2CH2Ph)24), which is in good agreement with the experimental result from the optical absorption spectroscopy. The extremely high stability of the nanocluster comes from the geometric structure and organization of the electronic states into superatom shells [100].

A disproportionation mechanism was further identified in the transformation of rod-like biicosahedral Au38(SCH2CH2Ph)24 to tetrahedral Au36(SPh-t-Bu)24 nanoclusters [99]. Figure 8 shows the detailed size-conversion pathway (roughly four stages) from the analysis of time-dependent mass spectrometry and optical spectroscopy. In stage I, the ligand exchange of Au38(SCH2CH2Ph)24 with bulkier HSPh-t-Bu occurred. A maximum of ~12 HSPh-t-Bu ligands were exchanged on the surface of Au38 cluster. In stage II, the ligand exchange reaction continued, but meanwhile it started to induce structural distortion to the original Au38(SR)24 cluster. In the optical absorption spectroscopy, Au38(SPh-t-Bu)m(SCH2CH2Ph)24–m (~12<m<~21) clusters showed some new absorption bands. In stage III, a disproportionation reaction from Au38(SR)24 to Au36(SR)24 and Au40(SR)26 was observed. In this process, one Au38(SR)24 cluster released two Au atoms and eventually generated Au36(SR)24. Meanwhile, another Au38(SR)24 cluster captured the two released Au atoms together with two free HSPh-t-Bu ligands to form Au40(SR)26. In the last stage, a size-focusing process accompanied by the ligand exchange rendered the pure Au36(SPh-t-Bu)24 clusters [99]. The conversion from rod-like biicosahedral Au38(SCH2CH2Ph)24 to tetrahedral Au36(SPh-t-Bu)24 nanoclusters provides a good example that the bulkiness of ligand would significantly affect the size and structure of thiolate-protected Au nanoclusters.

Fig. 8 
          Schematic diagram of reaction pathway for conversion of Au38(SC2H4Ph)24 to Au36(SPh-t-Bu)24. Stage I, ligand exchange; II, structure distortion; III, disproportionation; IV, size focusing. Adapted with permission from ref. [99].
Fig. 8

Schematic diagram of reaction pathway for conversion of Au38(SC2H4Ph)24 to Au36(SPh-t-Bu)24. Stage I, ligand exchange; II, structure distortion; III, disproportionation; IV, size focusing. Adapted with permission from ref. [99].

Conclusions

This review summarized the research on one of the representative Au nanoclusters – Au38(SR)24, including its identification, size-focusing synthesis, structure determination, intrinsic chirality, and two size-adjacent nanoclusters. There is still tremendous science in Au38(SR)24 nanoclusters to be discovered in future research. As the properties of Au38(SR)24 continue to be fleshed out, the results summarized in this review will be useful for further analyses and applications.

Future research on the Au38(SR)24 cluster will focus on the application in catalysis, optics, photovoltaics, and biomedicine, etc. In catalysis, Au38(SR)24 clusters, including the doped ones or surface-functionalized clusters, hold great promise in asymmetric catalysis. Well-defined Au38(SR)24 nanocluster catalysts will lead to fundamental understanding of the origin of nanogold catalysis, especially how the intrinsic chiral surface and quantum confinement in nanoclusters affects their catalytic properties. The semiconducting electronic properties and wide absorption spectrum spanning the UV-vis-NIR range also render them great potentials in optics and photovoltaics applications. The systematic and comprehensive studies on nanocluster materials will stimulate broad scientific and technological interests.


Corresponding author: Huifeng Qian, Department of Chemical and Biomolecular Engineering, Rice University, 6100 Main Street, Houston, TX 77005-1892, USA, e-mail: ;


A collection of invited, peer-reviewed articles by the winners of the 2013 IUPAC Prize for Young Chemists.


I acknowledge IUPAC for providing this opportunity to present this work and the support from J. Evans Attwell-Welch Postdoctoral Fellowship Program at the Richard E. Smalley Institute at Rice University. I deeply appreciate my PhD. advisor Prof. Rongchao Jin for his guidance, understanding, and encouragement during my graduate studies. I also thank Chenjie Zeng for valuable discussions.

References

[1] H. Qian, M. Zhu, Z. Wu, R. Jin. Acc. Chem. Res. 45, 1470 (2012).10.1021/ar200331zSearch in Google Scholar PubMed

[2] P. D. Jadzinsky, G. Calero, C. J. Ackerson, D. A. Bushnell, R. D. Kornberg. Science 318, 430 (2007).10.1126/science.1148624Search in Google Scholar PubMed

[3] T. Tsukuda. Bull. Chem. Soc. Jpn. 85, 151 (2012).10.1246/bcsj.20110227Search in Google Scholar

[4] J. F. Parker, C. A. Fields-Zinna, R. W. Murray. Acc. Chem. Res. 43, 1289 (2010).10.1021/ar100048cSearch in Google Scholar PubMed

[5] R. B. Wyrwas, M. M. Alvarez, J. T. Khoury, R. C. Price, T. G. Schaaff, R. L. Whetten. Eur. Phys. J. D 43, 91 (2007).10.1140/epjd/e2007-00117-6Search in Google Scholar

[6] Y. Niihori, M. Matsuzaki, T. Pradeep, Y. Negishi. J. Am. Chem. Soc. 135, 4946 (2013).10.1021/ja4009369Search in Google Scholar PubMed

[7] T. Udayabhaskararao, T. Pradeep. J. Phys. Chem. Lett. 4, 1553 (2013).10.1021/jz400332gSearch in Google Scholar PubMed

[8] H. Häkkinen. Nat. Chem. 4, 443 (2012).10.1038/nchem.1352Search in Google Scholar PubMed

[9] D.-e. Jiang. Nanoscale 5, 7149 (2013).10.1039/c3nr34192eSearch in Google Scholar PubMed

[10] R. S. McCoy, S. Choi, G. Collins, B. J. Ackerson, C. J. Ackerson. ACS Nano 7, 2610 (2013).10.1021/nn306015cSearch in Google Scholar PubMed

[11] C. M. Aikens. J. Phys. Chem. Lett. 2, 99 (2011).10.1021/jz101499gSearch in Google Scholar PubMed

[12] Y. Yu, Q. Yao, Z. Luo, X. Yuan, J. Y. Lee, J. Xie. Nanoscale 5, 4606 (2013).10.1039/c3nr00464cSearch in Google Scholar PubMed

[13] H. Yang, Y. Wang, J. Lei, L. Shi, X. Wu, V. Makinen, S. Lin, Z. Tang, J. He, H. Hakkinen, L. Zheng, N. Zheng. J. Am. Chem. Soc. 135, 9568 (2013).10.1021/ja402249sSearch in Google Scholar PubMed

[14] G. Schmid. Chem. Soc. Rev. 37, 1909 (2008).10.1039/b713631pSearch in Google Scholar PubMed

[15] S. H. Yau, O. Varnavski, T. Goodson. Acc. Chem. Res. 46, 1506 (2013).10.1021/ar300280wSearch in Google Scholar PubMed

[16] K. M. Harkness, A. Balinski, J. A. McLean, D. E. Cliffel. Angew. Chem., Int. Ed. 50, 10554 (2011).10.1002/anie.201102882Search in Google Scholar PubMed PubMed Central

[17] S. Antonello, M. Hesari, F. Polo, F. Maran. Nanoscale 4, 5333 (2013).10.1039/c2nr31066jSearch in Google Scholar PubMed

[18] H. Qian, Y. Zhu, R. Jin. Proc. Natl. Acad. Sci. USA 109, 696 (2012).10.1073/pnas.1115307109Search in Google Scholar PubMed PubMed Central

[19] T. D. Green, K. L. Knappenberger. Nanoscale 4, 4111 (2013).10.1039/c2nr31080eSearch in Google Scholar PubMed

[20] A. Desireddy, S. Kumar, J. Guo, M. D. Bolan, W. P. Griffith, T. P. Bigioni. Nanoscale 5, 2036 (2013).10.1039/c3nr33705gSearch in Google Scholar PubMed

[21] J. Liu, M. Yu, C. Zhou, S. Yang, X. Ning, J. Zheng. J. Am. Chem. Soc. 135, 4978 (2013).10.1021/ja401612xSearch in Google Scholar PubMed PubMed Central

[22] R. Jin, Y. Zhu, H. Qian. Chem. – Eur. J. 17, 6584 (2011).10.1002/chem.201002390Search in Google Scholar PubMed

[23] R. P. Carney, J. Y. Kim, H. F. Qian, R. C. Jin, H. Mehenni, F. Stellacci, O. M. Bakr. Nat. Commun. 2, 335 (2011).10.1038/ncomms1338Search in Google Scholar PubMed PubMed Central

[24] Y. Li, O. Zaluzhna, B. Xu, Y. Gao, J. M. Modest, Y. J. Tong. J. Am. Chem. Soc. 133, 2092 (2011).10.1021/ja1105078Search in Google Scholar PubMed

[25] Z. W. Wang, O. Toikkanen, B. M. Quinn, R. E. Palmer. Small 7, 1542 (2011).10.1002/smll.201002168Search in Google Scholar PubMed

[26] T. G. Schaaff, M. N. Shafigullin, J. T. Khoury, I. Vezmar, R. L. Whetten, W. G. Cullen, P. N. First, C. Gutierrez-Wing, J. Ascensio, M. J. Jose-Yacaman. J. Phys. Chem. B 101, 7885 (1997).10.1021/jp971438xSearch in Google Scholar

[27] S. W. Chen, R. S. Ingram, M. J. Hostetler, J. J. Pietron, R. W. Murray, T. G. Schaaff, J. T. Khoury, M. M. Alvarez, R. L. Whetten. Science 280, 2098 (1998).10.1126/science.280.5372.2098Search in Google Scholar PubMed

[28] Y. Negishi, K. Nobusada, T. Tsukuda. J. Am. Chem. Soc. 127, 5261 (2005).10.1021/ja042218hSearch in Google Scholar PubMed

[29] M. Zhu, C. M. Aikens, M. P. Hendrich, R. Gupta, H. Qian, G. C. Schatz, R. Jin. J. Am. Chem. Soc. 131, 2490 (2009).10.1021/ja809157fSearch in Google Scholar PubMed

[30] C. Gautier, T. Burgi. ChemPhysChem 10, 483 (2009).10.1002/cphc.200800709Search in Google Scholar PubMed

[31] P. R. Nimmala, A. Dass. J. Am. Chem. Soc. 133, 9175 (2011).10.1021/ja201685fSearch in Google Scholar PubMed

[32] R. Jin. Nanoscale 2, 343 (2010).10.1039/B9NR00160CSearch in Google Scholar

[33] Z. Tang, D. A. Robinson, N. Bokossa, B. Xu, S. Wang, G. Wang. J. Am. Chem. Soc. 133, 1603 (2011).10.1021/ja109925gSearch in Google Scholar PubMed

[34] R. Philip, P. Chantharasupawong, H. Qian, R. Jin, J. Thomas. Nano Lett. 12, 4661 (2012).10.1021/nl301988vSearch in Google Scholar PubMed

[35] Y. Lu, W. Chen. Chem. Soc. Rev. 41, 3594 (2012).10.1039/c2cs15325dSearch in Google Scholar PubMed

[36] A. Tlahuice-Flores, R. L. Whetten, M. Jose-Yacaman. J. Phys. Chem. C 117 20867 (2013).10.1021/jp407150tSearch in Google Scholar

[37] M. Zhu, C. M. Aikens, F. J. Hollander, G. C. Schatz, R. Jin. J. Am. Chem. Soc. 130, 5883 (2008).10.1021/ja801173rSearch in Google Scholar PubMed

[38] R. Jin, H. Qian, Y. Zhu, A. Das. J. Nanosci. Lett. 1, 72 (2011).Search in Google Scholar

[39] Y. Negishi, H. Tsunoyama, M. Suzuki, N. Kawamura, M. M. Matsushita, K. Maruyama, T. Sugawara, T. Yokoyama, T. Tsukuda. J. Am. Chem. Soc. 128, 12034 (2006).10.1021/ja062815zSearch in Google Scholar PubMed

[40] C. Noguez, I. L. Garzon. Chem. Soc. Rev. 38, 757 (2009).10.1039/b800404hSearch in Google Scholar PubMed

[41] I. Dolamic, S. Knoppe, A. Dass, T. Burgi. Nat. Commun. 3, 798 (2012).10.1038/ncomms1802Search in Google Scholar PubMed PubMed Central

[42] H. Yao. J. Phys. Chem. Lett. 3, 1701 (2012).10.1021/jz300396uSearch in Google Scholar PubMed

[43] G. Li, R. Jin. Acc. Chem. Res. 46, 1749 (2013).10.1021/ar300213zSearch in Google Scholar PubMed

[44] T. Tsukuda, H. Tsunoyama, H. Sakurai. Chem. Asian J. 6, 736 (2011).10.1002/asia.201000611Search in Google Scholar PubMed

[45] M. Turner, V. B. Golovko, O. P. H. Vaughan, P. Abdulkin, A. Berenguer-Murcia, M. S. Tikhov, B. F. G. Johnson, R. M. Lambert. Nature 454, 981 (2008).10.1038/nature07194Search in Google Scholar PubMed

[46] M. Brust, M. Walker, D. Bethell, D. J. Schiffrin, R. Whyman. J. Chem. Soc., Chem. Commun. 801 (1994).10.1039/C39940000801Search in Google Scholar

[47] C. A. Mirkin, R. L. Letsinger, R. C. Mucic, J. J. Storhoff. Nature 382, 607 (1996).10.1038/382607a0Search in Google Scholar PubMed

[48] R. L. Whetten, J. T. Khoury, M. M. Alvarez, S. Murthy, I. Vezmar, Z. L. Wang, P. W. Stephens, C. L. Cleveland, W. D. Luedtke, U. Landman. Adv. Mater. 8, 428 (1996).10.1002/adma.19960080513Search in Google Scholar

[49] M. J. Hostetler, C.-J. Zhong, B. K. H. Yen, J. Anderegg, S. M. Gross, N. D. Evans, M. Porter, R. W. Murray. J. Am. Chem. Soc. 120, 9396 (1998).10.1021/ja981454nSearch in Google Scholar

[50] H. Häkkinen, R. N. Barnett, U. Landman. Phys. Rev. Lett. 82, 3264 (1999).10.1103/PhysRevLett.82.3264Search in Google Scholar

[51] R. L. Donkers, D. Lee, R. W. Murray. Langmuir 20, 1945 (2004).10.1021/la035706wSearch in Google Scholar

[52] V. L. Jimenez, D. G. Georganopoulou, R. J. White, A. S. Harper, A. J. Mills, D. Lee, R. W. Murray. Langmuir 20, 6864 (2004).10.1021/la049274gSearch in Google Scholar PubMed

[53] D. Lee, R. L. Donkers, G. L. Wang, A. S. Harper, R. W. Murray. J. Am. Chem. Soc. 126, 6193 (2004).10.1021/ja049605bSearch in Google Scholar PubMed

[54] G. Wang, T. Huang, R. W. Murray, L. Menard, R. G. Nuzzo. J. Am. Chem. Soc. 127, 812 (2004).10.1021/ja0452471Search in Google Scholar PubMed

[55] R. L. Donkers, D. Lee, R. W. Murray. Langmuir 24, 5976 (2008).10.1021/la801163tSearch in Google Scholar

[56] J. B. Tracy, M. C. Crowe, J. F. Parker, O. Hampe, C. A. Fields-Zinna, A. Dass, R. W. Murray. J. Am. Chem. Soc. 129, 16209 (2007).10.1021/ja076621aSearch in Google Scholar PubMed

[57] A. Dass, A. Stevenson, G. R. Dubay, J. B. Tracy, R. W. Murray. J. Am. Chem. Soc. 130, 5940 (2008).10.1021/ja710323tSearch in Google Scholar PubMed

[58] M. W. Heaven, A. Dass, P. S. White, K. M. Holt, R. W. Murray. J. Am. Chem. Soc. 130, 3754 (2008).10.1021/ja800561bSearch in Google Scholar PubMed

[59] H. Tsunoyama, P. Nickut, Y. Negishi, K. Al-Shamery, Y. Matsumoto, T. Tsukuda. J. Phys. Chem. C 111, 4153 (2007).10.1021/jp067025qSearch in Google Scholar

[60] N. K. Chaki, Y. Negishi, H. Tsunoyama, Y. Shichibu, T. Tsukuda. J. Am. Chem. Soc. 130, 8608 (2008).10.1021/ja8005379Search in Google Scholar PubMed

[61] O. Toikkanen, V. Ruiz, G. Ronholm, N. Kalkkinen, P. Liljeroth, B. M. Quinn. J. Am. Chem. Soc. 130, 11049 (2008).10.1021/ja802317tSearch in Google Scholar PubMed

[62] H. Qian, M. Zhu, U. N. Andersen, R. Jin. J. Phys. Chem. A 113, 428184 (2009).10.1021/jp810893wSearch in Google Scholar PubMed PubMed Central

[63] H. Qian, Y. Zhu, R. Jin. ACS Nano 3, 3795 (2009).10.1021/nn901137hSearch in Google Scholar PubMed

[64] R. Jin, H. Qian, Z. Wu, Y. Zhu, M. Zhu, A. Mohanty, N. Garg. J. Phys. Chem. Lett. 1, 2903 (2010).10.1021/jz100944kSearch in Google Scholar

[65] T. G. Schaaff, R. L. Whetten. J. Phys. Chem. B 103, 9394 (1999).10.1021/jp993229dSearch in Google Scholar

[66] S. Knoppe, R. Azoulay, A. Dass, T. Burgi. J. Am. Chem. Soc. 134, 20302 (2012).10.1021/ja310330mSearch in Google Scholar PubMed

[67] S. Knoppe, A. C. Dharmaratne, E. Schreiner, A. Dass, T. Burgi. J. Am. Chem. Soc. 132, 16783 (2010).10.1021/ja104641xSearch in Google Scholar PubMed

[68] H. Qian, C. Liu, R. Jin. Sci. China Chem. 55, 2359 (2012).10.1007/s11426-012-4669-8Search in Google Scholar

[69] D. Stellwagen, A. Weber, G. L. Bovenkamp, R. Jin, J. H. Bitter, C. S. S. R. Kumar. RSC Adv. 2, 2276 (2012).10.1039/c2ra00747aSearch in Google Scholar

[70] S. Gaur, J. T. Miller, D. Stellwagen, A. Sanampudi, C. S. S. R. Kumar, J. J. Spivey. Phys. Chem. Chem. Phys. 14, 1627 (2012).10.1039/C1CP22438GSearch in Google Scholar PubMed

[71] C. Zeng, T. Li, A. Das, N. L. Rosi, R. Jin. J. Am. Chem. Soc. 135, 10011 (2013).10.1021/ja404058qSearch in Google Scholar PubMed

[72] H. Qian, R. Jin. Chem. Commun. 47, 11462 (2011).10.1039/c1cc15099eSearch in Google Scholar PubMed

[73] H. Qian, R. Jin. Nano Lett. 9, 4083 (2009).10.1021/nl902300ySearch in Google Scholar PubMed

[74] H. Qian, R. Jin. Chem. Mater. 23, 2209 (2011).10.1021/cm200143sSearch in Google Scholar

[75] H. Yang, Y. Wang, H. Huang, L. Gell, L. Lehtovaara, S. Malola, H. Hakkinen, N. Zheng. Nat. Commun. 4, 2422 (2013).10.1038/ncomms3422Search in Google Scholar PubMed

[76] A. Desireddy, B. E. Conn, J. Guo, B. Yoon, R. N. Barnett, B. M. Monahan, K. Kirschbaum, W. P. Griffith, R. L. Whetten, U. Landman, T. P. Bigioni. Nature 501, 399–402 (2013).10.1038/nature12523Search in Google Scholar PubMed

[77] Y. Zhu, H. Qian, R. Jin. J. Mater. Chem. 21, 6793 (2011).10.1039/c1jm10082cSearch in Google Scholar

[78] G. Li, H. Qian, R. Jin. Nanoscale 4, 6714 (2013).10.1039/c2nr32171hSearch in Google Scholar PubMed

[79] Y. Liu, H. Tsunoyama, T. Akita, S. Xie, T. Tsukuda. ACS Catal. 1, 2 (2011).10.1021/cs100043jSearch in Google Scholar

[80] D. R. Kauffman, D. Alfonso, C. Matranga, H. Qian, R. Jin. J. Am. Chem. Soc. 134 10237 (2012).10.1021/ja303259qSearch in Google Scholar PubMed

[81] H. Qian, W. T. Eckenhoff, Y. Zhu, T. Pintauer, R. Jin. J. Am. Chem. Soc. 132, 8280 (2010).10.1021/ja103592zSearch in Google Scholar PubMed

[82] I. L. Garzon, C. Rovira, K. Michaelian, M. R. Beltran, P. Ordejon, J. Junquera, D. Sanchez-Portal, E. Artacho, J. M. Soler. Phys. Rev. Lett. 85, 5250 (2000).10.1103/PhysRevLett.85.5250Search in Google Scholar PubMed

[83] I. L. Garzon, J. A. Reyes-Nava, J. I. Rodriguez-Hernandez, I. Sigal, M. R. Beltran, K. Michaelian. Phys. Rev. B 66, 073403 (2002).10.1103/PhysRevB.66.073403Search in Google Scholar

[84] D. Jiang, M. L. Tiago, W. Luo, S. Dai. J. Am. Chem. Soc. 130, 2777 (2008).10.1021/ja710991nSearch in Google Scholar PubMed

[85] D. Jiang, W. Luo, M. L. Tiago, S. Dai. J. Phys. Chem. C 112, 13905 (2008).10.1021/jp802766wSearch in Google Scholar

[86] Y. Pei, Y. Gao, X. C. Zeng. J. Am. Chem. Soc. 130, 7830 (2008).10.1021/ja802975bSearch in Google Scholar PubMed

[87] O. Lopez-Acevedo, H. Tsunoyama, T. Tsukuda, H. Häkkinen, C. M. Aikens. J. Am. Chem. Soc. 132, 8210 (2010).10.1021/ja102934qSearch in Google Scholar PubMed

[88] D.-e. Jiang. Acta Phys. -Chim. Sin. 26, 999 (2010).10.3866/PKU.WHXB20100414Search in Google Scholar

[89] L. Cheng, C. Ren, X. Zhang, J. Yang. Nanoscale 5, 1475 (2013).10.1039/c2nr32888gSearch in Google Scholar PubMed

[90] M. A. MacDonald, P. Zhang, N. Chen, H. Qian, R. Jin. J. Phys. Chem. C 115, 65 (2011).10.1021/jp1102884Search in Google Scholar

[91] H. Qian, E. Barry, Y. Zhu, R. Jin. Acta Phys. -Chim. Sin. 27, 513 (2011).10.3866/PKU.WHXB20112907Search in Google Scholar

[92] Y. Negishi, K. Igarashi, K. Munakata, W. Ohgake, K. Nobusada. Chem. Commun. 48, 660 (2012).10.1039/C1CC15765ESearch in Google Scholar

[93] W. Kurashige, S. Yamazoe, K. Kanehira, T. Tsukuda, Y. Negishi. J. Phys. Chem. Lett. 4, 3181 (2013).10.1021/jz401770ySearch in Google Scholar

[94] H. Qian, M. Zhu, C. Gayathri, R. R. Gil, R. Jin. ACS Nano 5, 8935 (2011).10.1021/nn203113jSearch in Google Scholar PubMed

[95] M. S. Devadas, S. Bairu, H. Qian, E. Sinn, R. Jin, G. Ramakrishna. J. Phys. Chem. Lett. 2, 2752 (2011).10.1021/jz2012897Search in Google Scholar

[96] S. Knoppe, I. Dolamic, T. Burgi. J. Am. Chem. Soc. 134, 13114 (2012).10.1021/ja3053865Search in Google Scholar PubMed

[97] S. Knoppe, S. Michalet, T. Burgi. J. Phys. Chem. C 117, 15354 (2013).10.1021/jp4040908Search in Google Scholar

[98] H. Qian, Y. Zhu, R. Jin. J. Am. Chem. Soc. 132, 4583 (2010).10.1021/ja1006383Search in Google Scholar PubMed

[99] C. Zeng, C. Liu, Y. Pei, R. Jin. ACS Nano 7, 6138 (2013).10.1021/nn401971gSearch in Google Scholar PubMed

[100] C. Zeng, H. Qian, T. Li, G. Li, N. L. Rosi, B. Yoon, R. N. Barnett, R. L. Whetten, U. Landman, R. Jin. Angew. Chem., Int. Ed. 51, 13114 (2013).10.1002/anie.201207098Search in Google Scholar PubMed

[101] S. Knoppe, J. Boudon, I. Dolamic, A. Dass, T. Burgi. Anal. Chem. 83, 5056 (2011).10.1021/ac200789vSearch in Google Scholar PubMed

[102] S. Knoppe, I. Dolamic, A. Dass, T. Bürgi. Angew. Chem., Int. Ed. 51, 7589 (2012).10.1002/anie.201202369Search in Google Scholar PubMed

[103] S. Malola, L. Lehtovaara, S. Knoppe, K.-J. Hu, R. E. Palmer, T. Burgi, H. Häkkinen. J. Am. Chem. Soc. 134, 19560 (2012).10.1021/ja309619nSearch in Google Scholar PubMed

Published Online: 2014-01-17
Published in Print: 2014-01-22

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