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[Re6S8X6](4-)(X = Cl、Br、I)中的电子跃迁:含时密度泛函理论和固态计算的结果

Electronic transitions in [Re6S8X6](4-) (X = Cl, Br, I): results from time-dependent density functional theory and solid-state calculations.

作者信息

Roy Lindsay E, Hughbanks Timothy

机构信息

Department of Chemistry, Texas A&M University, P.O. Box 30012 College Station, Texas 77842-3012, USA.

出版信息

Inorg Chem. 2006 Oct 2;45(20):8273-82. doi: 10.1021/ic061061m.

Abstract

Relativistic time-dependent density functional theory (TDDFT) calculations were performed on the excited states of the Re6S8X6 (X = Cl, Br, I) series. For all members of the series, the lowest excited states in the spectra do not correspond to a ligand-to-metal (or ligand-to-cluster) excitation but rather a cluster-cluster transition from the HOMO e(g) to antibonding t(1u) orbitals with only a modest admixture of Re-X sigma* character. These results lead to a re-evaluation of the role of the axial ligand in these compounds. The calculated excitation energies reproduce the experimental absorption and emission spectra. This work also confirms previous TDDFT calculations on the emission energies. Results for discrete cluster ions are compared with those obtained from calculations in the solid state in Cs4[Re6S8X6].CsX (X = Cl, Br) and Cs4[Re6S8I6].2CsI. Significant differences are seen in the relatively higher energies of the antibonding t(1u) orbital in the solid-state case, and an inversion in the orbital character of the two allowed absorptions is calculated. The e(g) (HOMO)-to-a(2g) (LUMO) orbital energy differences corresponding to the emission transition are quite comparable for the solid state and discrete cluster calculations, and both overestimate the observed emission energy by the same margin.

摘要

采用相对论含时密度泛函理论(TDDFT)对Re6S8X6(X = Cl、Br、I)系列的激发态进行了计算。对于该系列的所有成员,光谱中最低的激发态并非对应于配体到金属(或配体到簇)的激发,而是从HOMO e(g)轨道到反键t(1u)轨道的簇-簇跃迁,其中仅适度混合了Re-X σ*特征。这些结果导致对这些化合物中轴向配体的作用进行重新评估。计算得到的激发能重现了实验吸收光谱和发射光谱。这项工作还证实了先前关于发射能的TDDFT计算。将离散簇离子的结果与在Cs4[Re6S8X6].CsX(X = Cl、Br)和Cs4[Re6S8I6].2CsI固态计算中获得的结果进行了比较。在固态情况下,反键t(1u)轨道的能量相对较高,存在显著差异,并且计算出两个允许吸收的轨道特征发生了反转。对于固态和离散簇计算,对应于发射跃迁的e(g)(HOMO)到a(2g)(LUMO)轨道能量差相当可比,并且两者都以相同幅度高估了观测到的发射能。

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