Williams Darryl S., Korolev Andrey V.
Contribution from Department of Chemistry, 145, Wayne State University, Detroit, Michigan 48202.
Inorg Chem. 1998 Jul 27;37(15):3809-3819. doi: 10.1021/ic9800740.
Electronic absorption and emission spectra are reported for luminescent d(0) monoimido group 5 compounds M(NR)Cl(3)L(2) (M = Nb, Ta; R = alkyl, aryl; L = dme, Cl(-), py). These compounds display weak (epsilon < 200 M(-)(1) cm(-)(1)), well-resolved lowest-energy transitions in the high-energy visible and near-UV regions (20 000 < E(abs) < 29 000 cm(-)(1)). The energy of this absorption band depends strongly on the nature of the imido substituent, with a significant decrease observed when aryl groups are present. Excitation into this transition results in long-lived luminescent excited states. Long emission lifetimes (50 ns to 17 &mgr;s) and high quantum yields (0.001-0.24) are observed, decreasing primarily as a function of the alkyl substituent, being lowest in the aryl imidos. Good overlap is observed with absorption, excitation, and emission mirror spectra, indicating absorption into and emission from the same excited state. The data are consistent with absorption into and emission from a (3)(nb, pi) state, or d(xy)() <-- Ta-N pi. Semiempirical molecular orbital calculations are presented which suggest that the imido compounds may be considered as having highly mixed but localized Ta=N pi-bonding. A significant difference is noted in Ta(NPh)Cl(5)(-), in which there is appreciable aryl character in Ta=N pi-type orbitals. This accounts for the difference in electronic properties of the aryl imidos compared to the alkyl imidos. An analysis of radiative and nonradiative excited-state deactivation pathways is presented. Significantly, an energy gap law correlation is observed for nonradiative decay in the imido compounds as a group, but a corresponding correlation of radiative rates with emission energy is not observed when aryl and alkyl imidos are compared, evidence of electronic perturbation by the aryl substituent.
报道了发光的d(0)单亚胺基第5族化合物M(NR)Cl(3)L(2)(M = Nb、Ta;R = 烷基、芳基;L = dme、Cl(-)、py)的电子吸收光谱和发射光谱。这些化合物在高能可见光和近紫外区域(20000 < E(abs) < 29000 cm(-1))显示出弱的(ε < 200 M(-1) cm(-1))、分辨率良好的最低能量跃迁。该吸收带的能量强烈依赖于亚胺取代基的性质,当存在芳基时观察到显著降低。激发进入该跃迁会产生长寿命的发光激发态。观察到长的发射寿命(50 ns至17 μs)和高量子产率(0.001 - 0.24),主要随烷基取代基而降低,在芳基亚胺中最低。吸收、激发和发射镜像光谱之间观察到良好的重叠,表明吸收和发射来自同一激发态。数据与吸收进入和发射自(3)(nb, π)态或d(xy)() <-- Ta - N π一致。给出了半经验分子轨道计算,表明亚胺化合物可被视为具有高度混合但局域化的Ta = N π键。在Ta(NPh)Cl(5)(-)中注意到一个显著差异,其中Ta = N π型轨道中有明显的芳基特征。这解释了芳基亚胺与烷基亚胺相比电子性质的差异。给出了辐射和非辐射激发态失活途径的分析。值得注意的是,作为一组,在亚胺化合物中观察到非辐射衰变的能隙定律相关性,但当比较芳基亚胺和烷基亚胺时,未观察到辐射速率与发射能量的相应相关性,这是芳基取代基引起电子扰动的证据。