星团(航天器)
离解(化学)
光解
化学计量学
化学
铈
质谱
氧化铈
激光汽化
密度泛函理论
氧气
氧化物
氧化态
质谱法
金属
分析化学(期刊)
无机化学
结晶学
光化学
物理化学
激光器
计算化学
物理
色谱法
有机化学
计算机科学
光学
程序设计语言
作者
Scott T. Akin,Shaun G. Ard,Bryson E. Dye,Henry F. Schaefer,Michael A. Duncan
标识
DOI:10.1021/acs.jpca.6b02052
摘要
Cerium oxide cluster cations, CexOy(+), are produced via laser vaporization in a pulsed nozzle source and detected with time-of-flight mass spectrometry. The mass spectrum displays a strongly preferred oxide stoichiometry for each cluster with a specific number of metal atoms x, with x ≤ y. Specifically, the most prominent clusters correspond to the formula CeO(CeO2)n(+). The cluster cations are mass selected and photodissociated with a Nd:YAG laser at either 532 or 355 nm. The prominent clusters dissociate to produce smaller species also having a similar CeO(CeO2)n(+) formula, always with apparent leaving groups of (CeO2). The production of CeO(CeO2)n(+) from the dissociation of many cluster sizes establishes the relative stability of these clusters. Furthermore, the consistent loss of neutral CeO2 shows that the smallest neutral clusters adopt the same oxidation state (IV) as the most common form of bulk cerium oxide. Clusters with higher oxygen content than the CeO(CeO2)n(+) masses are present with much lower abundance. These species dissociate by the loss of O2, leaving surviving clusters with the CeO(CeO2)n(+) formula. Density functional theory calculations on these clusters suggest structures composed of stable CeO(CeO2)n(+) cores with excess oxygen bound to the surface as a superoxide unit (O2(-)).
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