首页> 外文期刊>Vacuum: Technology Applications & Ion Physics: The International Journal & Abstracting Service for Vacuum Science & Technology >Crystallization trend in STO-seeded sputtered PZT thin films: Effects of seed layer thickness and post-annealing temperature
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Crystallization trend in STO-seeded sputtered PZT thin films: Effects of seed layer thickness and post-annealing temperature

机译:STO种子溅射PZT薄膜的结晶趋势:种子层厚度和退火后温度的影响

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摘要

Based on the results of X-ray diffractometry (XRD) and analytical scanning/transmission electron microscopy (S/TEM), the crystallization trend and local chemistry of sputtered PZT films on SrTiO_3 (STO) coated corning glass substrates have been scrutinized as functions of STO layer thickness (~20-150 nm) and post-annealing temperature (450 C-650 ℃). It is shown that as a seed layer, STO thin films promote perovskite PZT nucleation at the PZT/STO interface at a temperature of ~450 ℃. Irrespective of STO seed layer thickness, PZT films evolve as a bi-layered structure comprising of tetragonal perovskite and disordered fcc fluorite upon post-annealing. The perovskite crystals are found to be enriched with Pb and lean in Zr and oxygen than fluorite structures. During the post-crystallization growth, Zr atoms get preferentially segregated from perovskite structures and accumulate in top fluorite zone resulting in Zrenrichment in the latter. Thinner STO seed layers are observed to be more effective in realizing better perovskite growth while crystallographic orientation selection of perovskite is dependent on both seed layer thickness and post-annealing temperature. Transverse compositional homogeneity of the grown perovskite PZT and the level of Pb-diffusion from film to the seed layer and glass substrate are also observed to be seed layer thickness dependent.
机译:根据X射线衍射(XRD)和分析扫描/透射电子显微镜(S / TEM)的结果,对SrTiO_3(STO)涂层的康宁玻璃基板上溅射的PZT膜的结晶趋势和局部化学性质进行了详细的研究。 STO层厚度(约20-150 nm)和后退火温度(450 C-650℃)。结果表明,在约450℃的温度下,STO薄膜作为晶种层可促进PZT / STO界面处钙钛矿PZT形核。不论STO种子层的厚度如何,PZT薄膜在退火后均会演化为包含四方钙钛矿和无序fcc萤石的双层结构。发现钙钛矿晶体比萤石结构富含Pb,并且Zr和氧气贫乏。在后结晶生长期间,Zr原子优先从钙钛矿结构中分离出来,并聚集在顶部的萤石区中,从而导致Zr富集。观察到更薄的STO晶种层在实现更好的钙钛矿生长方面更有效,而钙钛矿的晶体学取向选择取决于晶种层厚度和退火后温度。还观察到生长的钙钛矿PZT的横向组成均匀性以及从薄膜到籽晶层和玻璃基板的Pb扩散水平与籽晶层厚度有关。

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