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The Protonation States of Oxo-Bridged MnIV-Dimers Resolved by Experimental and Computational Mn K Pre-Edge X-Ray Absorption Spectroscopy

机译:通过实验和计算的Mn K前缘X射线吸收光谱解析的氧桥联MnIV二聚体的质子化态

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摘要

In nature, the protonation of oxo bridges is a commonly encountered mechanism for fine-tuning chemical properties and reaction pathways. Often, however, the protonation states are difficult to establish experimentally. This is of particular importance in the oxygen evolving complex of Photosystem II, where identification of the bridging oxo protonation states is one of the essential requirements toward unraveling the mechanism. In order to establish a combined experimental and theoretical protocol for the determination of protonation states, we have systematically investigated a series of Mn model complexes by Mn K pre-edge X-ray absorption spectroscopy. An ideal test case for selective bis-μ-oxo-bridge protonation in a Mn-dimer is represented by the system [MnIV2(salpn)2(μ-OH(n))2](n+). Although the three species [MnIV2(salpn)2(μ-O)2], [MnIV2(salpn)2(μ-O)(μ-OH)]+ and [MnIV2(salpn)2(μ-OH)2]2+ differ only in the protonation of the oxo bridges, they exhibit distinct differences in the pre-edge region while maintaining the same edge energy. The experimental spectra are correlated in detail to theoretical ly calculated spectra. A time-dependent density functional theory approach for calculating the pre-edge spectra of molecules with multiple metal centers is presented, using both high-spin (HS) and broken-symmetry (BS) electronic structure solutions. The most intense pre-edge transitions correspond to an excitation of the Mn-1s core electrons into the unoccupied orbitals of local eg character (dz2 and dxy based in the chosen coordinate system). The lowest by energy experimental feature is dominated by excitations of 1s-α electrons and the second observed feature is primarily attributed to 1s-β electron excitations. The observed energetic separation is due to spin polarization effects in spin-unrestricted density functional theory and models final state multiplet effects. The effects of spin polarization on the calculated Mn K pre-edge spectra, in both the HS and BS solutions, are discussed in terms of the strength of the antiferromagnetic coupling and associated changes in the covalency of Mn-O bonds. The information presented in this paper is complemented with the X-ray emission spectra of the same compounds published in an accompanying paper. Taken together, the two studies provide the foundation for a better understanding of the X-ray spectroscopic data of the oxygen evolving complex (OEC) in Photosystem II.
机译:在自然界中,氧代桥的质子化是微调化学性质和反应途径的常见机制。但是,通常很难通过实验确定质子化状态。这在光系统II的放氧复合物中尤为重要,在该系统中,确定桥联的羰基质子化状态是阐明该机理的基本要求之一。为了建立确定质子化状态的组合实验和理论方案,我们通过Mn K前缘X射线吸收光谱系统地研究了一系列Mn模型配合物。 [Mn IV 2(salpn)2(μ-OH(n))2]系统表示Mn-二聚体中选择性双-μ-氧代桥质子化的理想测试用例sup>(n +)。尽管这三个物种[Mn IV 2(salpn)2(μ-O)2],[Mn IV 2(salpn)2(μ-O)(μ- OH)] + 和[Mn IV 2(salpn)2(μ-OH)2] 2 + 的区别仅在于氧代桥,它们在前边缘区域表现出明显的差异,同时保持相同的边缘能量。将实验光谱与理论计算的光谱进行详细的关联。提出了一种基于时间的密度泛函理论方法,该方法使用高自旋(HS)和断裂对称(BS)电子结构解决方案来计算具有多个金属中心的分子的前缘光谱。最强烈的前边缘跃迁对应于Mn-1s核心电子激发到局部未占据的轨道,例如字符(在所选坐标系中基于dz 2 和dxy)。最低的能量实验特征是1s-α电子的激发,观察到的第二个特征主要是1s-β电子的激发。观察到的能量分离是由于自旋无限制密度泛函理论中的自旋极化效应所致,并且对最终状态多重峰效应进行了建模。在反铁磁耦合强度以及相关的Mn-O键共价变化方面,讨论了在HS和BS溶液中自旋极化对计算得出的Mn K前缘光谱的影响。本文提供的信息与随附论文中发布的相同化合物的X射线发射光谱相辅相成。两者合计,这两项研究为更好地了解Photosystem II中的析氧复合物(OEC)的X射线光谱数据提供了基础。

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