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W(110)表面氧吸附的从头算相图。

Ab initio phase diagram of oxygen adsorption on W(110).

作者信息

Stöhr M, Podloucky R, Müller S

机构信息

Institute for Physical Chemistry, University of Vienna, Sensengasse 8/7, A-1090 Vienna, Austria.

出版信息

J Phys Condens Matter. 2009 Apr 1;21(13):134017. doi: 10.1088/0953-8984/21/13/134017. Epub 2009 Mar 12.

Abstract

The phase diagram of oxygen adsorption on the W(110) surface is derived without any empirical parameters by a combination of density functional theory (DFT) calculations, the cluster expansion (CE) technique and Monte Carlo (MC) applications. Coverages up to 1 monolayer are considered corresponding to the range of oxygen concentrations, 0≤x(O)≤1. DFT results for single-site adsorption and in particular for full coverage reveal that adsorption at threefold hollow (H3) sites is by far the most stable one. Therefore, the CE is done for an atomic layer with the two H3 sublattices of the W(110) surface. Based on 60 DFT calculations with fully relaxed atomic geometries of lateral unit cells containing 12 atoms, and a ground state search for 80 394 structures, four ground state structures are found with the lateral unit cells (2 × 5) for x(O) = 0.20, (2 × 2) (a) for x(O) = 0.25, (2 × 1) for x(O) = 0.50 and (2 × 2) (b) for x(O) = 0.75. In agreement with experiments the most stable structures are (2 × 1) and (2 × 2) (b), which correspond to higher coverages. The thermodynamical stability of the two ground states at lower coverages is very weak. Detailed analysis of the relaxation of the (2 × 1) structure reveals sizeable lateral stresses acting on the surface tungsten atoms. On the basis of the effective cluster interactions MC simulations are performed in order to derive the critical temperatures by which the phase diagram is finally constructed.

摘要

通过结合密度泛函理论(DFT)计算、团簇展开(CE)技术和蒙特卡罗(MC)应用,在没有任何经验参数的情况下得出了氧在W(110)表面的吸附相图。考虑了高达1个单层的覆盖度,对应于氧浓度范围0≤x(O)≤1。单原子吸附的DFT结果,特别是全覆盖的结果表明,在三重中空(H3)位点的吸附是迄今为止最稳定的。因此,对具有W(110)表面两个H3子晶格的原子层进行了团簇展开。基于对包含12个原子的横向晶胞进行完全弛豫原子几何结构的60次DFT计算,以及对80394个结构的基态搜索,发现了四个基态结构,对于x(O)=0.20,横向晶胞为(2×5);对于x(O)=0.25,横向晶胞为(2×2)(a);对于x(O)=0.50,横向晶胞为(2×1);对于x(O)=0.75,横向晶胞为(2×2)(b)。与实验一致,最稳定的结构是(2×1)和(2×2)(b),它们对应于更高的覆盖度。较低覆盖度下两个基态的热力学稳定性非常弱。对(2×1)结构弛豫的详细分析揭示了作用在表面钨原子上的相当大的横向应力。基于有效的团簇相互作用进行了MC模拟,以便得出最终构建相图的临界温度。

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