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通过与天线配体结合诱导的末端铜氮烯的形成及反应活性

Terminal Copper Nitrenoid Formation and Reactivity Induced by Absorption to an Antenna Ligand.

作者信息

de Kler Noël, Pereverzev Aleksandr Y, Roithová Jana

机构信息

Department of Spectroscopy and Catalysis, Institute for Molecules and Materials, Radboud University, Heyendaalseweg 135, 6525 AJ, Nijmegen, The Netherlands.

出版信息

Angew Chem Int Ed Engl. 2024 Apr 2;63(14):e202319270. doi: 10.1002/anie.202319270. Epub 2024 Feb 29.

Abstract

Copper nitrenoids are key intermediates in copper-catalyzed direct C-H amination reactions. Further development of this important reaction relies on knowing the properties and reactivity of the nitrenoid intermediates. This work utilizes antenna ligands to form copper nitrenoid complexes and monitor the consecutive C-H amination reactions under well-defined single-molecule conditions in the gas phase. The [Cu(L)(L)] precursors (L is a bidentate antenna ligand, and L is an organic azide) were stored in an ion trap at 3.5 K and irradiated by visible light, which resulted in denitrogenation of the complex. Further irradiation of the copper nitrenoid led to the consecutive C-H amination of the antenna ligand. The nitrenoid complexes, as well as the products of the C-H amination, were characterized by helium tagging IRPD spectroscopy, and the mechanism was described by DFT calculations. This research demonstrates that the antenna ligands can be used to promote the denitrogenation of metal azides in the gas phase and also channel the internal energy to promote further reactivity, which opens a new way to study the reactivity of highly reactive species under well-defined conditions.

摘要

铜氮宾是铜催化直接C-H胺化反应中的关键中间体。这一重要反应的进一步发展依赖于了解氮宾中间体的性质和反应活性。本工作利用天线配体形成铜氮宾配合物,并在气相中明确的单分子条件下监测连续的C-H胺化反应。[Cu(L)(L)]前体(L是双齿天线配体,L是有机叠氮化物)在3.5 K下存储于离子阱中,并用可见光照射,这导致配合物脱氮。对铜氮宾的进一步照射导致天线配体连续的C-H胺化。通过氦标记红外光解离光谱对氮宾配合物以及C-H胺化产物进行了表征,并通过密度泛函理论计算描述了反应机理。本研究表明,天线配体可用于促进气相中金属叠氮化物的脱氮,并引导内能以促进进一步的反应活性,这为在明确条件下研究高反应活性物种的反应活性开辟了一条新途径。

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