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关于中性巢状杂硫金属[MOS3Py5Cu3X](M = Mo,W;X = F,Cl,Br,I)簇的非线性光学性质的密度泛函理论研究。

DFT studies on nonlinear optical properties of neutral nest-shaped heterothiometallic [MOS3Py5Cu3X] (M=Mo, W; X=F, Cl, Br, I) clusters.

作者信息

Tang Guo-dong, Jiang Zheng-jing, Li Rong-qing, Zhang Jin-fang, Zhang Yu, Zhang Chi

机构信息

Department of Chemistry, Jiangsu Province Key Laboratory for Chemistry of Low-dimensional Materials, Huaiyin Teachers College, Huai'an 223001, Jiangsu Province, PR China.

出版信息

Spectrochim Acta A Mol Biomol Spectrosc. 2009 Sep 15;74(1):228-32. doi: 10.1016/j.saa.2009.06.035. Epub 2009 Jun 21.

DOI:10.1016/j.saa.2009.06.035
PMID:19646920
Abstract

Theoretical calculations were carried out on some neutral nest-shaped heterothiometallic cluster compounds [MOS(3)Py(5)Cu(3)X] (M=Mo, W; X=F, Cl, Br, I) with the high first static hyperpolarizabilities beta values. The geometries of these cluster compounds were optimized by the restricted DFT method at B3LYP level with LanL2DZ base set without any constrains. In order to understand the relationship between the first static hyperpolarizabilities and the compositions of these clusters, the frontier orbital compositions and energy gaps between the HOMO and LUMO orbitals were calculated and analysed. In these clusters the HOMO orbitals are mainly composed of halogen atoms and the first static hyperpolarizability increases from F to I atom. The LUMO orbitals of clusters [MoOS(3)Py(5)Cu(3)X] are comprised of Mo, O and S atoms while the LUMO orbitals of clusters [WOS(3)Py(5)Cu(3)X] composed of W atom and pyridine ring. The energy gaps between the HOMO and LUMO orbitals of the clusters [MoOS(3)Py(5)Cu(3)X] are smaller than those of the clusters [WOS(3)Py(5)Cu(3)X]. As a result the first static hyperpolarizability values of the clusters [MoOS(3)Py(5)Cu(3)X] are higher than those of the clusters [WOS(3)Py(5)Cu(3)X].

摘要

对一些具有高第一静态超极化率β值的中性巢状异硫属金属簇化合物[MOS(3)Py(5)Cu(3)X](M = Mo、W;X = F、Cl、Br、I)进行了理论计算。这些簇化合物的几何结构通过受限密度泛函理论方法在B3LYP水平下使用LanL2DZ基组进行优化,无任何限制。为了理解第一静态超极化率与这些簇的组成之间的关系,计算并分析了前线轨道组成以及最高占据分子轨道(HOMO)和最低未占据分子轨道(LUMO)之间的能隙。在这些簇中,HOMO轨道主要由卤素原子组成,并且第一静态超极化率从F原子到I原子逐渐增加。簇[MoOS(3)Py(5)Cu(3)X]的LUMO轨道由Mo、O和S原子组成,而簇[WOS(3)Py(5)Cu(3)X]的LUMO轨道由W原子和吡啶环组成。簇[MoOS(3)Py(5)Cu(3)X]的HOMO和LUMO轨道之间的能隙小于簇[WOS(3)Py(5)Cu(3)X]的能隙。结果,簇[MoOS(3)Py(5)Cu(3)X]的第一静态超极化率值高于簇[WOS(3)Py(5)Cu(3)X]的第一静态超极化率值。

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