等离子体-气体凝聚团簇源产生的Ag-Nb合金团簇中的成分分配

K. Wakoh , T. Hihata , D.L. Peng , K. Sumiyama
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引用次数: 17

摘要

作为我们迈向合金团簇形成的第一步,我们已经通过面向目标型等离子体-气体冷凝团簇源生产了Ag-Nb团簇。在衬底上沉积了Ag-Nb簇,并用透射电子显微镜对其进行了纳米束能量色散x射线分析。我们获得了直径在5 ~ 10nm之间的Ag-Nb合金团簇。它们的化学成分分布广泛,分为富银和富铌两种,符合非混相型平衡相图。结果表明,合金团簇的形成是由合金相稳定性驱动的。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
Compositional partition in Ag-Nb alloy clusters produced by a plasma-gas-condensation cluster source

We have produced Ag-Nb clusters by a facing-target type plasma-gas-condensation cluster source as our first step toward alloy cluster formation. The Ag-Nb clusters have been deposited on substrates and examined by a transmission electron microscope with a nano-beam energy dispersive X-ray analysis. We have obtained Ag-Nb alloy clusters with the sizes range between 5 and 10 nm in diameter. Their chemical compositions are broadly dispersed and partitioned into Ag-rich and Nb-rich ones, being consistent with the immiscible type equilibrium phase diagram. This result suggests that alloy cluster formation is driven by the alloy phase stability.

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