| Literature DB >> 35266609 |
Li Feng Lim1, Martyna Judd1, Petra Vasko2, Michael G Gardiner1, Dimitrios A Pantazis3, Nicholas Cox1, Jamie Hicks1.
Abstract
An isostructural series of heavy Group 14 E(I) radical anions (Ge, Sn, Pb), stabilized by a bulky xanthene-based diamido ligand are reported. The radical anions were synthesised by the one-electron reduction of their corresponding E(II) precursor complexes with sodium naphthalenide in THF, yielding the radical anions as charge-separated sodium salts. The series of main group radicals have been comprehensively characterized by EPR spectroscopy, X-ray crystallography and DFT analysis, which reveal that in all cases, the spin density of the unpaired electron almost exclusively resides in a p-orbital of π symmetry located on the Group 14 center.Entities:
Keywords: EPR Spectroscopy; Group 14 Elements; Main Group Elements; Radical Ions
Year: 2022 PMID: 35266609 PMCID: PMC9401049 DOI: 10.1002/anie.202201248
Source DB: PubMed Journal: Angew Chem Int Ed Engl ISSN: 1433-7851 Impact factor: 16.823
Figure 1Heavy monometallic Group 14 E(I) radical complexes.
Scheme 1Synthesis of the radical anions 2‐Ge, 2‐Sn and 2‐Pb.
Figure 2Molecular structures of 2‐Ge (left) and 2‐Sn (right) as determined by X‐ray crystallography. Hydrogen atoms and the [Na(THF)6]+ cations are omitted for clarity. Displacement ellipsoids set at the 50 % probability level. Key bond lengths [Å]; 2‐Ge: Ge−N 2.089(5), 2.072(6); Ge⋅⋅⋅O 2.641(4); 2‐Sn: Sn−N 2.260(11), 2.281(10); Sn⋅⋅⋅O 2.61(1).
Figure 3Singly occupied molecular orbitals (SOMOs) from DFT models (top) and experimental EPR spectra (bottom) of a) 2‐Ge; b) 2‐Sn ; and c) 2‐Pb. The SOMO is shown for each complex along with the “hinging” of the ligand's backbone (θ). Spin Hamiltonian simulations, offset from the data are shown in red and all parameters listed. * indicates an unidentified trace paramagnetic impurity.
Figure 4X‐band HYSCORE spectrum of 2‐Ge. 1H and 14N signals marked are consistent with hyperfine coupling constants of the order of 4 MHz. See Supporting Information for corresponding 2‐Sn and 2‐Pb data.