Ag(110)和Cu(110)表面加氧层不同形成方式的原因

T. Schimizu , M. Tsukuda
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引用次数: 0

摘要

氧在Ag(110)和Cu(110)表面的吸附已经通过第一性原理的总能量和力计算在局部密度近似(LDA)内的重复板几何形状进行了研究。对于化学吸附结构,如果允许AgOAg添加行发生屈曲和衬底结构发生一定的变形,则STM图像推测的添加行模型证实为稳定结构之一。根据最陡下降法,添加排和表面第一层中吸附的氧原子和贵金属原子向最小总能量的构型松弛。通过对Ag(110)(n × 1)−O (n = 2,3)和Cu(110)(2 × 1)−O的优化几何模型的比较,得到了Ag(110)和Cu(110)表面添加行形成模式差异机理的重要线索。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
Origin of the different formation modes of the oxygen added row overlayer on Ag(110) and Cu(110) surfaces

Oxygen adsorption on Ag(110) and Cu(110) surfaces has been investigated by means of first-principles total-energy, and force calculations for repeated-slab geometries within the local density approximation (LDA). As for the chemisorption structure, the added row model speculated by the obserbed STM images is confirmed to be one of the stable structures, if bucking of the AgOAg added row and some distortions of the substrate structure are allowed. The adsorbed oxygen atom and noble metal atoms in the added row and in the surface first-layer are relaxed toward the configuration of the minimum total energy in terms of steepest descent method. Moreover comparing the optimized geometrics of the added row model of Ag(110)(n × 1)−O (n = 2, 3) and Cu(110)(2 × 1)−O, we obtain an important clue for the mechanism of the difference in the formation modes of the added row on Ag(110) and Cu(110) surfaces.

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