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首页> 外文期刊>Physical chemistry chemical physics: PCCP >Theoretical analysis of NMR shieldings of group-11 metal halides on MX (M = Cu, Ag, Au; X = H, F, Cl, Br, I) molecular systems, and the appearance of quasi instabilities on AuF
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Theoretical analysis of NMR shieldings of group-11 metal halides on MX (M = Cu, Ag, Au; X = H, F, Cl, Br, I) molecular systems, and the appearance of quasi instabilities on AuF

机译:MX(M = Cu,Ag,Au; X = H,F,Cl,Br,I)分子系统上第11组金属卤​​化物的NMR屏蔽的理论分析以及在AuF上出现的拟不稳定性

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Accurate calculations of nuclear magnetic shieldings of group-11 metal halides, sigma(M; MX) (M = Cu, Ag, Au; X = H, F, Cl, Br, I), were performed with relativistic and nonrelativistic theoretical schemes in order to learn more about the importance of the involved electronic mechanisms that underlie such shieldings. We applied state of the art schemes: polarization propagators at a random phase level of approach (PP-RPA); spin-free Hamiltonian (SF); linear response elimination of small component (LRESC) and density functional theory (DFT) with two different functionals: B3LYP and PBE0. The results from DFT calculations are not close to those from the relativistic polarization propagator calculations at the RPA level of approach (RelPP-RPA), in line with previous results. The spin-orbit (SO) contribution to a shielding constant is important only for MF molecules (M = Cu, Ag, Au). Different electronic mechanisms are considered within the LRESC method, bunched into two groups: core-and ligand-dependent. For the analysed shieldings the core-dependent electronic mechanisms are the most important ones; the ligand-dependent being only important for MF molecules. An out of range value for s(Au) is found in AuF. It was previously reported in the literature, either originated in the large fluorine electronegativity together with large spin-orbit coupling contributions; or, due to Fermi-contact contributions. We argue here that such an unexpected large value is an artifact originated in the appearance of quasi instabilities, and show how to handle this apparent problem.
机译:使用相对论和非相对论的理论方案对11组金属卤​​化物的核磁屏蔽σ(M; MX)(M = Cu,Ag,Au; X = H,F,Cl,Br,I)进行精确计算。为了更多地了解构成这种屏蔽的电子机制的重要性。我们采用了最先进的方案:在随机相位阶段进场的极化传播器(PP-RPA);无自旋哈密顿量(SF);小组件线性响应消除(LRESC)和具有两个不同功能的密度泛函理论(DFT):B3LYP和PBE0。 DFT计算的结果与RPA进近水平(RelPP-RPA)的相对论极化传播器计算的结果不相近,与先前的结果一致。自旋轨道(SO)对屏蔽常数的贡献仅对于MF分子(M = Cu,Ag,Au)很重要。 LRESC方法中考虑了不同的电子机制,分为两类:核心依赖性和配体依赖性。对于分析的屏蔽,依赖于芯的电子机制是最重要的。配体依赖性仅对MF分子重要。在AuF中发现s(Au)的值超出范围。先前曾在文献中报道过,要么起源于大的氟电负性,要么伴随着巨大的自旋-轨道耦合作用。或者,由于费米接触的贡献。我们在这里辩称,这样一个意想不到的大值是一种由准不稳定现象引起的假象,并说明了如何处理这个明显的问题。

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