Yao Qiaomu, Berenov Andrey V, Bower Ryan, Zou Bin, Xiao Xiaofei, Alford Neil M, Oulton Rupert F M, Petrov Peter K
Department of Materials, Imperial College London, London SW7 2AZ, United Kingdom.
Department of Physics, Imperial College London, London SW7 2AZ, United Kingdom.
ACS Appl Nano Mater. 2023 Jun 20;6(13):11115-11123. doi: 10.1021/acsanm.3c00934. eCollection 2023 Jul 14.
Gold nanoparticle (AuNP) decoration is a commonly used method to enhance the optical responses in many applications such as photocatalysis, biosensing, solar cells, etc. The morphology and structure of AuNPs are essential factors determining the functionality of the sample. However, tailoring the growth mechanism of AuNPs on an identical surface is not straightforward. In this study, AuNPs were deposited on the surface of a perovskite thin film, strontium niobate (SNO), using pulsed laser deposition (PLD). AuNPs exhibited a dramatic variation in their growth mechanisms, depending on whether they were deposited on SNO thin films grown on magnesium oxide (SNO/MgO) or strontium titanate (SNO/STO) substrates. On SNO/MgO, the Au aggregates form large NPs with an average size of up to 3500 nm. These AuNPs are triangular with sharp edges and corners. The out-of-plane direction of growth is favored, and the surface coverage ratio by AuNPs is low. When deposited on SNO/STO, the average size of AuNPs is much smaller, i.e., ∼250 nm. This reduction in the average size is accompanied by an increase in the number density of NPs. AuNPs on SNO/STO have a round shape and high coverage ratio. Such an impact from the substrate selection on the AuNP structure is significant when the sandwiched SNO film is below 80 nm thickness and is weakened for 200 nm of SNO films. X-ray diffraction (XRD) and scanning electron microscopy (SEM) were used to characterize all samples. Strain analysis was used to explain the growth mechanism of AuNPs. The average height of AuNPs was measured by using atomic force microscopy (AFM). Ellipsometry in the visible-near-infrared (vis-NIR) region was used to characterize the optical response of all samples. AuNP-decorated SNO/MgO and SNO/STO thin films exhibit different optical properties, with only gold-decorated SNO/MgO samples showing a size-dependent epsilon-near-zero behavior of nanoparticles. These results provide an additional route to control the structure of AuNPs. They can be used for various plasmonic applications like the design and development of strain-engineered gold-nanoparticle-decorated devices for surface-enhanced Raman spectroscopy (SERS) and photocatalysis.
金纳米颗粒(AuNP)修饰是一种常用的方法,可增强许多应用(如光催化、生物传感、太阳能电池等)中的光学响应。AuNP的形态和结构是决定样品功能的关键因素。然而,在同一表面上定制AuNP的生长机制并非易事。在本研究中,使用脉冲激光沉积(PLD)将AuNP沉积在钙钛矿薄膜铌酸锶(SNO)的表面。AuNP的生长机制表现出显著差异,这取决于它们是沉积在生长于氧化镁(SNO/MgO)或钛酸锶(SNO/STO)衬底上的SNO薄膜上。在SNO/MgO上,金聚集体形成平均尺寸高达3500 nm的大颗粒。这些AuNP呈三角形,边缘和角尖锐。生长倾向于面外方向,AuNP的表面覆盖率较低。当沉积在SNO/STO上时,AuNP的平均尺寸要小得多,即约250 nm。平均尺寸的减小伴随着颗粒数密度的增加。SNO/STO上的AuNP呈圆形且覆盖率高。当夹在中间的SNO薄膜厚度低于80 nm时,衬底选择对AuNP结构的这种影响很显著,而对于200 nm的SNO薄膜,这种影响会减弱。使用X射线衍射(XRD)和扫描电子显微镜(SEM)对所有样品进行表征。应变分析用于解释AuNP的生长机制。使用原子力显微镜(AFM)测量AuNP的平均高度。在可见-近红外(vis-NIR)区域的椭偏测量用于表征所有样品的光学响应。AuNP修饰的SNO/MgO和SNO/STO薄膜表现出不同的光学性质,只有金修饰的SNO/MgO样品显示出纳米颗粒尺寸依赖的近零介电常数行为。这些结果提供了另一种控制AuNP结构的途径。它们可用于各种等离子体应用,如设计和开发用于表面增强拉曼光谱(SERS)和光催化的应变工程金纳米颗粒修饰器件。