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超快 X 射线溶液散射揭示了三核十二羰基合钌(Ru3(CO)12)在紫外光和可见光激发后的光解过程中不同的反应途径。

Ultrafast X-ray solution scattering reveals different reaction pathways in the photolysis of triruthenium dodecacarbonyl (Ru3(CO)12) after ultraviolet and visible excitation.

机构信息

Société civile Synchrotron SOLEIL, L'Orme des Merisiers, Saint-Aubin-BP 48, 91192 GIF-sur-Yvette Cedex, France.

出版信息

J Am Chem Soc. 2010 Mar 3;132(8):2600-7. doi: 10.1021/ja9097548.

Abstract

Ultrafast (ps) time-resolved X-ray scattering was used to study the structural dynamics of Ru(3)(CO)(12) in cyclohexane after photolysis at 260 nm. Two intermediates form after 100 ps at the onset of the reaction: Ru(3)(CO)(10) for the CO loss channel and Ru(3)(CO)(11)(mu-CO) for the metal-metal cleavage channel. In our previous study at 390 nm, by contrast, three intermediates were observed simultaneously at the onset of the reaction that all relax back to Ru(3)(CO)(12) with different lifetimes. The major difference between photolysis at 260 and 390 nm is that in the first case Ru(3)(CO)(10)(mu-CO) is formed by bimolecular recombination of Ru(3)(CO)(10) with a free CO in 50 ns, whereas in the second case it forms directly from Ru(3)(CO)(12) at the onset of the reaction. The differences between the photofragmentation pathways are related to the absorption bands available at the two wavelengths. The extrema in the difference radial distribution functions (RDFs) are unambiguously assigned by decomposing the total signal into contributions from the solutes, the solvent and the solute-solvent cross-terms, and also contributions from each candidate species. The difference RDFs reveal the depletion of Ru-Ru bonds (2.88 A) in the initial Ru(3)(CO)(12) molecule and formation of Ru(3)(CO)(10) as the major photoproduct. The high-resolution X-ray (88 keV) scattering pattern of pure liquid C(6)H(12) indicates that the solvent dynamics at early time delays is due to broadening of the intermolecular interatomic correlations at constant volume, whereas during thermal expansion at longer time delays, it results from shifts in these correlations.

摘要

超快(ps)时间分辨 X 射线散射被用来研究 Ru(3)(CO)(12) 在 260nm 光解后在环己烷中的结构动力学。反应开始后 100ps 时形成了两个中间体:CO 损失通道的 Ru(3)(CO)(10)和金属-金属断裂通道的 Ru(3)(CO)(11)(mu-CO)。相比之下,在我们之前在 390nm 的研究中,反应开始时同时观察到三个中间体,它们都以不同的寿命松弛回 Ru(3)(CO)(12)。260nm 和 390nm 光解的主要区别在于,在前一种情况下,Ru(3)(CO)(10)(mu-CO)是通过 Ru(3)(CO)(10)与自由 CO 在 50ns 内的双分子重排形成的,而在后一种情况下,它直接从 Ru(3)(CO)(12)形成。光解途径的差异与两个波长下可用的吸收带有关。通过将总信号分解为溶质、溶剂和溶质-溶剂交叉项以及每个候选物种的贡献,可以明确地将差分径向分布函数(RDF)的极值分配。差分 RDF 揭示了初始 Ru(3)(CO)(12)分子中 Ru-Ru 键(2.88A)的耗尽和 Ru(3)(CO)(10)的形成作为主要光产物。纯液态 C(6)H(12)的高分辨率 X 射线(88keV)散射图案表明,早期时间延迟的溶剂动力学是由于体积恒定的分子间原子间相关性的展宽,而在较长时间延迟的热膨胀过程中,它是由于这些相关性的位移所致。

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