Quynh
Nguyen
a,
Attilio
Zilli
b,
Michele
Celebrano
b and
Andrea
Baldi
*a
aVrije Universiteit Amsterdam, Department for Physics and Astronomy, De Boelelaan 1100, 1081HV Amsterdam, The Netherlands. E-mail: a.baldi@vu.nl
bPolitecnico di Milano, Department of Physics, Piazza Leonardo da Vinci, 32, 20133 Milano, Italy
First published on 13th March 2025
Plasmonic materials, such as gold nanoparticles (AuNPs), exhibit significant extinction and near-field enhancement across the visible and near-infrared spectrum, attributable to localized surface plasmon resonances (LSPRs). Epsilon-near-zero (ENZ) materials, such as aluminium doped zinc oxide (AZO) are known in non-linear optics for their ability to generate and manipulate light-matter interactions through processes like higher harmonic generation. Combining doped ZnO with plasmonic materials therefore holds promise for enhancing non-linear efficiencies and tuning their operational wavelengths. To date, however, only top-down structures based on plasmonically decorated thin ENZ films have been realized, and no colloidal and scalable route to obtain these hybrid materials has been reported yet. Here, we introduce a novel colloidal synthesis approach for fabricating Au@AZO core@shell nanoparticles with tunable core size, shell thickness, and dopant concentration, allowing for the spectral alignment of the LSPRs of the AuNPs with the non-linear optical properties of the AZO shells. Our method involves the colloidal synthesis of gold cores followed by an ascorbic acid-assisted process to deposit polycristalline ZnO and AZO shells, resulting in core diameters ranging from 25 to 69 nm, shell thicknesses from 16 to 47 nm, and aluminium doping levels between 0 and 4 at%. Our procedure widens the range of hybrid plasmonic nanostructures that can be colloidally synthesised, opening new possibilities for the large scale fabrication of high-performance nanomaterials for integration in photonic, photocatalytic, and sensing applications.
The near-field enhancement of LSPRs has been utilized to amplify intrinsically weak non-linear responses, such as second- (SHG) and third-harmonic generation (THG). Yet, these performances were achieved by highly engineered nanostructures, which require a demanding fabrication, the use of extremely short pulses, and are not readily scalable.9–15
To date, the integration of plasmonics with non-linear optics (NLO) has primarily focused on lithographically fabricated two-dimensional structures.16–18 However, several applications such as biomedical labelling and imaging demand scalable syntheses of large quantities of colloidal NPs. A viable approach is to synthesise plasmonic NPs coated by a NLO thin shell, where the second or third harmonics of the shell are, both spatially and spectrally, overlapping with the LSPR of the core to further enhance the intrinsically weak non-linear optical signals.
Zinc oxide (ZnO) is chemically and mechanically stable.19–26 Additionally, while the toxicity of ZnO has been well studied and documented, specific surface modifications and application methods have been developed to mitigate these effects, making them suitable for bio-imaging under controlled conditions.27–29 Additionally, ZnO displays NLO properties that can be modulated by chemical doping.10,30,31 In particular, aluminium doped zinc oxide (AZO) exhibits a vanishing real part of the permittivity in the near-infrared (near-IR) range, classifying it as an epsilon-near-zero (ENZ) material. The level of aluminium doping controls the wavelength at which the permittivity crosses zero, providing an additional dimension of tunability.32 ENZ materials have been recently suggested as promising materials for NLO, thanks to their sizeable nonlinear susceptibility that combines with the strong field enhancements at specific wavelength, typically set in the NIR region of the spectrum. This phenomenon, known as ENZ condition, occurs in transparent conducting oxides when the real part of the electric permittivity approaches zero yielding a metal-like behavior.33,34
An ideal system to combine plasmonic near-field enhancement with ENZ materials could therefore be composed of a gold core coated with an aluminium-doped ZnO shell, where the size and shape of the core, and the thickness and dopant level of the shell are tuneable at will.
It is possible to synthesise Au@ZnO core@shell NPs by combining the colloidal synthesis of the metallic cores to an ascorbic acid-assisted step for the formation of an oxide shell, in which ascorbic acid (AA) forms a CTAB–[AA–Zn(OH)4]2− complexing agent to facilitate the deposition of Zn2+ ions onto the Au cores. However, previous studies largely overlooked possibilities of tailoring the structural parameters of the NPs35–40 or led to the formation of a hydrated zinc hydroxide (Zn(OH)2) shell in the absence of an annealing final step.41 Additionally, no colloidal synthesis of Au@AZO core@shell NPs has been reported, likely due to the high sensitivity of the AZO syntheses to the reactant concentrations, the pH level of the solution, the ratio of surfactant to ascorbic acid, and the temperature of the reaction.42,43
In this work, we demonstrate the colloidal synthesis of Au@ZnO and Au@AZO core@shell NPs with controlled shell thickness, core size and shape, and aluminium dopant concentration. As a first step to demonstrate tunability of the synthetic process, we establish a procedure to vary the shell thickness of Au@ZnO NPs by varying the initial concentration of Au cores while keeping the concentration of the other reactants constant. We then demonstrate that ZnO shells can easily be grown on spherical Au cores of different diameters as well as on gold nanorods. Finally, we develop a novel procedure to obtain Au@AZO NPs by adding an aluminium doping step before calcination. We corroborate the synthetic results with UV-Vis spectroscopy, scanning electron microscopy (SEM), energy-dispersive X-ray spectroscopy (EDX), inductively coupled plasma mass spectrometry (ICP-MS), and Mie theory calculations of the extinction cross-section spectra of the core@shell NPs.44
The result of a typical Au@ZnO synthesis is shown in Fig. 1, for Au cores of 43 ± 3 nm in diameter and a ZnO shell thickness of 47 ± 4 nm. Fig. 1(a) shows the extinction spectrum of the reaction solution, containing AuNPs, L-ascorbic acid (AA), cetyltrimethylammonium bromide (CTAB), hexamethylenetetramine (HMTA), and zinc nitrate (Zn(NO3)2), prior to hydrothermal synthesis. At this stage, light extinction is solely attributed to the LSPR of the AuNPs with a peak at 534 nm. Fig. 1(b) shows the extinction spectrum of the as-synthesised Au@Zn(OH)2 dispersion after the hydrothermal reaction. The formation of a hydrated Zn(OH)2 shell with an average thickness of 59 ± 5 nm induces a ∼15 nm redshift in the LSPR wavelength to 549 nm, due to the slight increase in the refractive index of the gold surrounding from water to Zn(OH)2.45 The NP dimensions and core@shell structure are confirmed by SEM.
To convert the hydrated Zn(OH)2 shell into crystalline ZnO, we centrifuge the Au@Zn(OH)2 NPs, redisperse them in water, dry them in air at 150 °C for 30 min, and calcinate them at 500 °C in air for 2 h. The obtained powder is then let to cool down and redispersed in water. Fig. 1(c) shows the extinction spectrum of a suspension of Au@ZnO core@shell NPs, highlighting a further ∼86 nm red-shift of the LSPR to 635 nm, due to the higher refractive index of ZnO compared to Zn(OH)2. The spectrum also shows the emergence of a peak at 375 nm, corresponding to the band gap energy of ZnO (E ≈ 3.37 eV) and indicating the presence of crystalline wurtzite phase ZnO, as confirmed via X-ray diffraction (XRD) measurement (see SI 1.1, ESI†). The SEM images demonstrate a uniform particle shape and narrow size distribution, as also indicated by the narrow LSPR peaks observed in the UV-Vis extinction spectra. The inset of backscattered electron SEM image in Fig. 1(c) (middle row) shows the presence of a Au core in all the Au@ZnO NPs.
The shell thickness of the final Au@ZnO NPs can be controlled by varying the number of gold NPs in the initial reaction solution while keeping the concentration of the remaining reactants constant. The Au@ZnO NPs shown in Fig. 1(c), are obtained with an initial concentration of 3.1 × 1011 AuNPs per ml leading to a final diameter of the Au@ZnO core@shell NPs of 137 nm, corresponding to a ZnO shell thickness of 47 nm. In Fig. 2, we demonstrate the coating of the same 43 nm AuNPs with ZnO shell thicknesses of 21, 25, 30, and 34 nm, obtained from reaction solutions with initial AuNP concentration of 10.8 × 1010, 9.6 × 1010, 7.5 × 1010, and 5.6 × 1010 NPs per ml, respectively. The initial AuNP concentrations in the reaction solution are estimated via Beer–Lambert law from the OD of the solutions, using Mie theory to calculate the extinction cross section of a 43 nm AuNP (see calculations in SI 1.2, ESI†).46
Precise knowledge of the AuNPs concentration allows us to estimate the yield of the ZnO synthesis reaction.
We estimated the theoretical maximum yield of ZnO shell synthesis around a AuNP core. Assuming complete conversion of the zinc nitrate precursor to zinc oxide, the calculations indicate a maximum yield of ∼7.3 mg of Au@ZnO NPs.
These calculations were based on the initial amount of zinc nitrate used, and the properties of the AuNPs, including their OD and radius. The detailed derivations and the full set of assumptions made in these calculations are given in SI 1.3 (ESI†).
Fig. 3(a) shows the extinction spectra of the particles shown in Fig. 2, after the hydrothermal treatment but before the final annealing step, i.e. corresponding to Au@Zn(OH)2 core@shell NPs. As expected, suspensions with a larger initial concentration of AuNPs have higher overall extinction across the visible and a slightly blue-shifted LSPR, indicating a thinner Zn(OH)2 shell (Fig. 3(b)). Fig. 3(c) shows the total volume of ZnO in the final Au@ZnO core@shell NP suspensions of Fig. 2, calculated from the initial AuNP concentration, cAuNPs, the radius of the gold cores, rAu, and the radius of the final Au@ZnO core@shell NPs, rAu@ZnO, according to:
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The horizontal dashed line in Fig. 3(c) represents the maximum obtainable ZnO volume per ml, calculated from the total amount of zinc nitrate added to the hydrothermal reaction, indicating a nearly quantitative conversion of the initial Zn(NO3)2 into ZnO shells around the Au cores.
Our synthetic procedure can be used to synthesise ZnO shells around Au particles of different diameters and shapes. In Fig. 4(a)–(c) we show SEM images of Au@ZnO core@shell NPs with spherical core diameters of 25, 43 and 69 nm. Fig. 4(d) shows the encapsulation of non-spherical gold nanorods with average width and length of 54 × 118 nm. Coating different Au NPs with ZnO shells allows us to tune their optical response across the visible (Fig. SI.2, ESI†).
As a final step in the development of our synthesis, we altered the shell composition by intercalating Al3+ ions into the ZnO lattice, using a novel approach. Zeto et al. have successfully embedded copper and rare earth metals (Ce, Er, Nd, Tm, and Yb) into the ZnO shells of Au@doped-ZnO core@shell nanostructures.38 However, the synthesis of Au@AZO core@shell NPs remains largely unexplored. Previous studies on ZnO NPs and thin films showed that aluminium doping significantly affects the morphology of the final AZO crystallites.42,47,48
As a first approach to obtain Au@AZO core@shell NPs, we followed previous experimental procedures for the synthesis of AZO49,50 and added a stoichiometric quantity of Al(NO3)3 to the initial hydrothermal reaction mixture containing Zn(NO3)2 (procedure 1 in Scheme 1). However, such an approach proved to be unsuccessful in leading to well-controlled core@shell NPs, resulting in large quantities of AZO agglomerates decorated with the AuNPs (Fig. SI.3, ESI†). Our working hypothesis to explain the difficulty in incorporating Al3+ ions in the ZnO shell structure is that the acidity of the aluminium nitrate solution (pH ∼ 3) prevents the precipitation of Zn(OH)2, which is unstable below pH 6.51,52 In fact, the significance of the structural damage to the final AZO shell increases for higher Al3+ dopant concentration.
To mitigate the impact of pH on the overall hydrothermal synthesis, we also tried a different approach whereby the Al3+ dopant solution was neutralized to a pH of 6.5 using ammonium hydroxide (NH4OH) before addition to the reaction mixture prior to hydrothermal heating. Despite the formation of Au@AZO core@shell NPs, we noticed a significant decrease in particle size and shell homogeneity with increasing concentrations of the dopant (Fig. SI.4, ESI†).
The synthesis of dopant-controlled Au@AZO NPs was achieved by first synthesizing Au@Zn(OH)2 core@shell NPs in the absence of any Al3+ doping, centrifuging the product and redispersing it in a pH-neutral aqueous solution of aluminium nitrate (Al(NO3)3).
The Au@Zn(OH)2 core@shell NPs are left in the Al3+ solution for 30 minutes before drop casting on a silicon substrate and annealing. This process is illustrated in procedure 2 in Scheme 1. Using a non-neutralized aluminium nitrate solution results in compromised NP morphology and uniformity (Fig. SI.5, ESI†).
Fig. 5 shows SEM images of Au@AZO NPs obtained by redispersing the Au@Zn(OH)2 core@shell NPs in pH-neutralized solutions of 0 mM, 0.055 mM, 0.11 mM, and 0.23 mM Al(NO3)3, corresponding to nominal Al-doping of 0, 1, 2, and 4 at%, respectively. A uniform core@shell structure of the Au@AZO NPs is visible up until a nominal doping percentage of 2 at%, with 4 at% doping leading to some loss of homogeneity of the AZO shell To confirm the incorporation of Al3+ ions into the semiconducting shell we performed energy dispersive X-ray spectroscopy (EDX) using a line-scan across a Au@ZnO particle and a 2 at% doped Au@AZO particle (Fig. 6(a) and (b)). The blue lines corresponding to the aluminium Kα1 transition, clearly show the presence of aluminium within the doped particle. To measure the dopant percentage in the AZO shells we performed inductively coupled mass-spectrometry (ICP-MS) on washed Au@AZO NPs, as illustrated in Fig. 6(c).
The aluminium content measured in the blank was subtracted from the one detected in each NP sample to correct for baseline contamination. The aluminium percentage in each sample was then determined from the ratio of the corrected aluminium signal to the zinc signal. When aiming for a nominal doping of 0, 1, 2, and 4 at% of aluminium, ICP-MS measurements show that our samples contain 0.4, 0.9, 2.2 and 3.4 at%, respectively. The ICP-MS data demonstrates a quantitative incorporation of Al3+ into the ZnO shell, which we further confirm using extinction spectroscopy.
Doping zinc oxide with aluminium causes a decrease in refractive index of the surrounding medium of the Au cores,53 resulting in a blue-shift of the LSPR. The extinction spectra measured on Au@AZO NPs suspensions confirm this trend (Fig. 7(a)) as the LSPR shifts from 617 nm for Au@ZnO to as low as 575 nm for a Au@AZO core@shell NP with a nominal shell doping of 4 at%. In literature, the successful doping of ZnO with Al3+ in thin AZO films is typically monitored by the lowering of the AZO bandgap with increasing dopant concentration.54,55 However, the high scattering of the Au@AZO NPs causes a strong increase in extinction at shorter wavelengths. This high scattering background affects the shape and spectral position of the ZnO bandgap, preventing us from using it as an indicator of dopant concentration.
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Fig. 7 (a) Normalised extinction spectra of Au@AZO core@shell NP dispersions with nominal dopant percentage up to 4 at% Al. The Au@AZO NPs with 0, 1, and 2 at% doping have dimensions of 121 ± 8 nm (0 at% Al), 130 ± 9 nm (1 at% Al), and 127 ± 6 nm (2 at% Al), as obtained from an analysis of the SEM images in Fig. 5. Since the Au cores have an average diameter of 43 nm, these dimensions correspond to shell thicknesses of 39 nm (0 at% Al), 43.5 nm (1 at% Al), and 42 nm (2 at% Al), respectively. The inset shows a zoomed in view of the LSPR peak positions. (b) Calculated extinction cross sections of Au@AZO particles with 43 nm core-diameter, 40 nm shell thickness and dopant percentage of 0, 2 and 5 at% Al. (c) LSPR peak positions for the spectra shown in panels (a) and (b) as a function of aluminium dopant percentage.53,56,57 |
Using Mie theory and literature values for the refractive indices of doped ZnO, we calculated the extinction cross section of core@shell particles with 43 nm diameter cores and 40 nm thick shells with Al3+ dopant percentages of 0, 2 and 5 at% (Fig. 7(b)).46,53,56,57 The position of the LSPR shifts towards shorter wavelengths for particles with increased dopant concentration, qualitatively reproducing the trend observed in our experimental spectra (Fig. 7(c)).
To prepare Au nanoclusters, 5 ml of 0.5 mM HAuCl4 are added to 5 ml of 0.2 M CTAB in a round-bottom flask in a water bath at 27 °C under stirring. Then, 0.6 ml of 0.01 M fresh ice-cold sodium borohydride are added rapidly to the reaction mixture. The stirring is then stopped, and the reaction mixture is left undisturbed for 3 h.
To prepare the 10 nm seed solution, 20 ml of 0.2 M CTAC, 15 ml of 0.1 AA and 50 μl of the previously obtained Au nanocluster solution are added in a separate flask under stirring and kept at 27 °C. Using two 10 ml pipettes, 20 ml of 0.5 mM HAuCl4 are added via one-shot injection. The reaction is left to continue for 15 min to obtain a 10 nm AuNP seed solution with the characteristic vibrant red colour. The AuNPs are centrifuged at 14500 rpm (7943 × g) for 60 min. The supernatant is removed, and the pellet is redispersed in 0.02 mM CTAC. This procedure is repeated twice. Finally, the optical density (OD) at the LSPR wavelength of the seed solution is adjusted to OD = 3.06, corresponding to an estimated concentration of 1.37 × 1013 NPs per ml.
To obtain AuNPs with a diameter of 43 nm, 80 ml of an aqueous solution of 0.1 M CTAC are added to 4.8 ml of 0.01 M AA together with 798 μl of the 10 nm AuNP seed solution in a round-bottom flask and kept at 27 °C. Subsequently, 80 ml of 0.5 mM HAuCl4 are added drop-wise while stirring with a syringe pump at a rate of 80 ml h−1. After the HAuCl4 addition, the solution is left to stir for another 15 minutes. The solution is then centrifuged at 5000 rpm for 15 minutes and the final product was redispersed in water and diluted to an OD of 13, as confirmed using extinction spectroscopy. For AuNPs with a diameter of 43 nm, an OD of 13 corresponds to a concentration of ∼6.31 × 1011 AuNPs per ml. To synthesise 25 nm, 69 nm and 79 nm AuNPs the same procedure is being following with 4000 μl, 40 μl and 27 μl of the 10 nm AuNP seed solution, respectively.
The product, consisting of Au@Zn(OH)2 NPs, is drop-casted onto a flat Si wafer and dried in air at 150 °C for 30 min until dry, before calcination at 500 °C for 2 h in a furnace with a heating ramping time of 30 min. The product is then left to cool to room temperature. The obtained powder consisting of Au@ZnO NPs with a shell thickness of 47 nm, is then collected by scraping it off the Si wafer with a plastic spatula and stored in an airtight container for further characterization.
Au@ZnO NPs with shell thicknesses of 21, 25, 30, and 34 nm are obtained by adding 3.23, 2.77, 2.08, and 1.64 ml of the 43 nm AuNP solution in the initial step, respectively.
Au@ZnO NPs with core diameters of 25, 43, and 69 nm are obtained by replacing the initial AuNPs solution in the hydrothermal step with AuNPs with different diameter in the same NP concentration.
Au@ZnO NPs with Au nanorods as a core are obtained by adding 3 ml of a 118 × 54 nm AuNRs solution with an OD = 30 at the longitudinal LSPR to the reaction mixture.
Future studies will focus on characterizing their non-linear optical properties and integrating them into real-world settings to test their performance under different environmental conditions and irradiation profiles.
Potential applications of such versatile hybrid material include high-speed optical modulators, advanced photonic circuits, ultra-sensitive biosensors, as well as non-linear bio labels, contributing towards more efficient, faster, and miniaturized technologies.
Footnote |
† Electronic supplementary information (ESI) available. See DOI: https://doi.org/10.1039/d4tc04644g |
This journal is © The Royal Society of Chemistry 2025 |