Bagus Paul S, Nelin Connie J, Brundle C R, Crist B Vincent, Lahiri N, Rosso Kevin M
Department of Chemistry, University of North Texas, Denton, Texas 76203-5017, USA.
Consultant, Austin, Texas 78730, USA.
J Chem Phys. 2021 Mar 7;154(9):094709. doi: 10.1063/5.0039765.
The Al K alpha, 1486.6 eV, based x-ray photoelectron spectroscopy (XPS) of Fe 2p and Fe 3p for Fe(III) in FeO and Fe(II) in FeO is compared with theoretical predictions based on ab initio wavefunctions that accurately treat the final, core-hole, multiplets. The principal objectives of this comparison are to understand the multiplet structure and to evaluate the use of both the 2p and 3p spectra in determining oxidation states. In order to properly interpret the features of these spectra and to use the XPS to provide atomistic insights as well as atomic composition, it is necessary to understand the origin of the multiplet energies and intensities. The theoretical treatment takes into account the ligand field and spin-orbit splittings, the covalent mixing of ligand and Fe 3d orbitals, and the angular momentum coupling of the open shell electrons. These effects lead to the distribution of XPS intensity into a large number of final, ionic, states that are only partly resolved with energies spread over a wide range of binding energies. For this reason, it is necessary to record the Fe 2p and 3p XPS spectra over a wide energy range, which includes all the multiplets in the theoretical treatment as well as additional shake satellites. We also evaluate the effects of differing assumptions concerning the extrinsic background subtraction, to make sure our experimental spectrum may be fairly compared to the theory. We conclude that the Fe 3p XPS provides an additional means for distinguishing Fe(III) and Fe(II) oxidation states beyond just using the Fe 2p spectrum. In particular, with the use of the Fe 3p XPS, the depth of the material probed is about 1.5 times greater than for the Fe 2p XPS. In addition, a new type of atomic many-body effect that involves excitations into orbitals that have Fe f,ℓ = 3, symmetry has been shown to be important for the Fe 3p XPS.
对FeO中Fe(III)的Fe 2p和Fe 3p以及FeO中Fe(II)的基于Al Kα(1486.6 eV)的X射线光电子能谱(XPS)与基于从头算波函数的理论预测进行了比较,该波函数能精确处理终态、芯孔、多重态。这种比较的主要目的是了解多重态结构,并评估2p和3p光谱在确定氧化态方面的用途。为了正确解释这些光谱的特征,并利用XPS提供原子层面的见解以及原子组成,有必要了解多重态能量和强度的来源。理论处理考虑了配体场和自旋轨道分裂、配体与Fe 3d轨道的共价混合以及开壳层电子的角动量耦合。这些效应导致XPS强度分布到大量终态离子态中,这些态仅部分被分辨,能量分布在很宽的结合能范围内。因此,有必要在很宽的能量范围内记录Fe 2p和3p XPS光谱,该范围包括理论处理中的所有多重态以及额外的摇振卫星峰。我们还评估了关于外部背景扣除的不同假设的影响,以确保我们的实验光谱可以与理论进行公平比较。我们得出结论,Fe 3p XPS提供了一种除仅使用Fe 2p光谱之外区分Fe(III)和Fe(II)氧化态的额外方法。特别是,使用Fe 3p XPS时,探测到的材料深度约为Fe 2p XPS的1.5倍。此外,一种涉及激发到具有Fe f,ℓ = 3对称性轨道的新型原子多体效应已被证明对Fe 3p XPS很重要。