Simulations of x-ray absorption spectra for CO desorbing from Ru(0001) with transition-potential and time-dependent density functional theory approaches.

Pub Date : 2022-01-13 eCollection Date: 2022-01-01 DOI:10.1063/4.0000135
Gabriel L S Rodrigues, Elias Diesen, Johannes Voss, Patrick Norman, Lars G M Pettersson
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Abstract

The desorption of a carbon monoxide molecule from a Ru(0001) surface was studied by means of X-ray Absorption Spectra (XAS) computed with Transition Potential (TP-DFT) and Time Dependent (TD-DFT) DFT methods. By unraveling the evolution of the CO electronic structure upon desorption, we observed that at 2.3 Å from the surface, the CO molecule has already predominantly gas-phase character. While C 1s XAS is quite insensitive to changes in the C-O bond length, the O 1s excitation is very sensitive with the π* coming down in energy upon CO bond stretching, which competes with the increase in orbital energy due to the repulsive interaction with the metallic surface. We show in a systematic way that the TP-DFT method can describe the XAS rather well at the endpoints (chemisorbed and gas phase) but is affected by artificial charge transfer and/or incorrect spin treatment in the transition region in cases like CO, where there are low-lying π* orbitals and large exchange interactions between the core 1s and valence-acceptor π* orbitals. As an alternative, we demonstrate by comparing with experimental data that a linear response approach using TD-DFT employing common exchange-correlation functionals and finite-size clusters can yield a good description of the spectral evolution of the 1s → π* transition with correct spin and gas-to-chemisorbed chemical shifts in good agreement with experiment.

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用过渡电位和随时间变化的密度泛函理论方法模拟从 Ru(0001) 解吸 CO 的 X 射线吸收光谱。
我们利用过渡势(TP-DFT)和时变(TD-DFT)DFT 方法计算的 X 射线吸收光谱(XAS)研究了一氧化碳分子从 Ru(0001)表面解吸的过程。通过揭示解吸过程中 CO 电子结构的演变,我们观察到在距离表面 2.3 Å 处,CO 分子已经主要具有气相特性。虽然 C 1s XAS 对 C-O 键长度的变化非常不敏感,但 O 1s 激发却非常敏感,在 CO 键伸展时,π* 的能量会下降,这与与金属表面的排斥作用导致的轨道能量增加形成了竞争。我们用系统的方法表明,TP-DFT 方法可以很好地描述端点(化学吸附和气相)的 XAS,但在 CO 等情况下,会受到过渡区人为电荷转移和/或不正确自旋处理的影响,因为在过渡区存在低洼的 π* 轨道以及核心 1s 与价受 π* 轨道之间的大量交换相互作用。作为一种替代方法,我们通过与实验数据的比较证明,利用普通交换相关函数和有限尺寸簇的 TD-DFT 线性响应方法可以很好地描述 1s → π* 转变的光谱演变,其正确的自旋和气体-化合层化学位移与实验结果非常一致。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
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