Gendron Frédéric, Pritchard Ben, Bolvin Hélène, Autschbach Jochen
Department of Chemistry, University at Buffalo, State University of New York , Buffalo, New York 14260-3000, United States.
Inorg Chem. 2014 Aug 18;53(16):8577-92. doi: 10.1021/ic501168a. Epub 2014 Jul 30.
Electronic structures and magnetic properties of actinyl ions AnO2(n+) (An = U, Np, and Pu) and the equatorially coordinated carbonate complexes UO2(CO3)3, NpO2(CO3)3, and PuO2(CO3)3 are investigated by ab initio quantum chemical calculations. The complex PuO2(NO3)3 is also included because of experimentally available g-factors and for comparison with a previous study of NpO2(NO3)3 (Chem.—Eur. J. 2014, 20, 7994-8011). The results are rationalized with the help of crystal-field (CF)-type models with parameters extracted from the ab initio calculations, and with the help of natural orbitals and natural spin orbitals contributing to the magnetic properties and the unpaired spin distribution, generated from the spin–orbit wave functions. These orbitals resemble textbooklike representations of the actinide 5f orbitals. Calculated paramagnetic susceptibilities are used to estimate dipolar 13C chemical shifts for the carbonate ligands. Their signs and order of magnitude are compared to paramagnetic effects observed experimentally in NMR spectra. The results indicate that the experimental spectra are also influenced by contact shifts.
锕酰离子AnO2(n+)(An = U、Np和Pu)以及赤道配位的碳酸酯配合物UO2(CO3)3、NpO2(CO3)3和PuO2(CO3)3的电子结构和磁性通过从头算量子化学计算进行研究。由于实验可得的g因子以及为了与之前对NpO2(NO3)3的研究(《化学—欧洲杂志》2014年,20卷,7994 - 8011页)进行比较,PuO2(NO3)3配合物也被纳入研究。借助从从头算计算中提取参数的晶体场(CF)型模型,以及借助对磁性和未成对自旋分布有贡献的自然轨道和自然自旋轨道(由自旋 - 轨道波函数生成),对结果进行了合理解释。这些轨道类似于锕系元素5f轨道的教科书式表示。计算得到的顺磁磁化率用于估计碳酸酯配体的偶极13C化学位移。将它们的符号和量级与核磁共振谱中实验观察到的顺磁效应进行比较。结果表明,实验光谱也受到接触位移的影响。