화학공학소재연구정보센터
Inorganic Chemistry, Vol.40, No.20, 5092-5096, 2001
Structure and bonding in Hartwig stretched eta(3)-hydridoborate sigma-complex of niobium(III)
Ab initio calculations at the SCF, MP2, CASSCF, and CASPT2 levels of theory with basis sets using atomic pseudopotentials have been carried out for the stretched eta (3)-hydridoborate sigma -complex of niobium, [Cl2Nb{H2B(OH)(2)}], in order to investigate the nature and energetics of the interaction between the transition metal and the eta (3)-hydridoborate ligand. The geometry of the complex [Cl2Nb{H2B(OH)(2)}] and its fragments [Cl2Nb](+) and [H2B(OH)(2)](-) were optimized at SCF and CASSCF levels. These results are consistent with [Cl2Nb{eta (3)-H2B(OH)(2)}] being a Nb(III) complex in which both hydrogen and boron of the [eta (3)-H2B(OH)(2)](-) ligand have a bonding interaction with the niobium preserving stretching B-H bond character. The calculated values of DEF (energy required to restore the fragment from the equilibrium structure to the structure it takes in the complex) for [Cl2Nb](+) are 5.35 kcal/mol at SCF, 3.27 kcal/mol at MP2, 4.80 kcal/mol at CASSCF, and 2.82 kcal/mol at CASPT2 and for [H2B(OH)(2)](-) 21.13 kcal/mol at SCF, 23.85 kcal/mol at MP2, 20.69 kcal/mol at CASSCF, and 23.48 kcal/mol at CASPT2. Values of INT (stabilization energy resulting from the coordination of distorted ligand to the metal fragment) for the complex [Cl2Nb{H2B(OH)(2)}] are -239.35 kcal/mol at SCF, -260.00 kcal/mol at MP2, -230.76 kcal/mol at CASSCF, and -252.60 kcal/mol at CASPT2. For the complex [(eta (5)-C5H5)(2)Nb{H2B(OH)2}], calculations at the SCF and MP2 levels were carried out. Values of INT for [(eta (5)-C5H5)(2)Nb{H2B(OH)(2)}] are -169.93 kcal/mol at SCF and -210.62 kcal/mol at MP2. The results indicate that the bonding of the [eta (3)-H2B(OH)(2)](-) ligand with niobium is substantially stable. The electronic structures of [Cl2Nb{H2B(OH)(2)}], [(eta (5)-C5H5)(2)Nb{H2B(OH)(2)}], and its fragments are analyzed in detail as measured by Mulliken charge distributions and orbital populations.