负载ag的A、X、Y型沸石在大气中热处理的光致发光

Yushi Suzuki, T. Miyanaga, K. Yamauchi, Naohiro Mori, Reki Nakamura
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引用次数: 3

摘要

利用原位x射线吸收精细结构(XAFS)研究了银团簇或银离子与光致发光(PL)性能之间的关系。Ag团簇是在Ag型沸石a、X、Y在大气中加热的空腔中生成的。沸石腔内的银团簇经大气加热冷却至室温后发生破坏。本研究结果表明,Ag团簇坍塌在强PL条带的产生中起着重要作用,Ag团簇可能不是PL的直接种类。结果还表明,Ag团簇形成和破坏引起的Ag离子的局部位置与未加热的种类略有不同。
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Photoluminescence of Ag-loaded A, X, and Y type zeolites heat-treated in atmosphere
We use in-situ X-ray absorption fine structure (XAFS) to examine the relation between Ag clusters or Ag ions and properties of photoluminescence (PL). The Ag clusters are generated in the cavity of Ag-type zeolite-A, X, and Y heating in atmosphere. The Ag clusters in the zeolite cavity break down when cooled to room temperature after heating in atmosphere. Results of this study suggest that collapsing Ag cluster plays an important role in the generation of strong PL bands and that Ag clusters might not be a direct species of PL. Results also show that the local sites of Ag ions differ slightly from the unheated species induced by the formation and destruction of Ag clusters.
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