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Electron Density of Transition Metal Complexes

The intermediate Hamiltonian Fock-space coupled-cluster calculations of Infante et al. [1146] were performed in an all-electron approach explicitly correlating 26 electrons and using large de ontracted basis sets. [Pg.625]

for the Ft complex, the scalar-relativistic DKH Hamiltonian and the spin-orbit ZORA-Hamiltonian recover relativistic effects on the electron density of the valence region found in four-component calculations. This is particularly remarkable since the DKH density has not been corrected for the picture-change error in these calculations. The difference density maps for the Ft complex clearly show the importance of the scalar-relativistic contraction of the inner shells, while spin-orbit effects can be neglected for this closed-shell complex (otherwise, the DKH results would deviate much more from the four omponent and ZORA data). In the case of the Ni system the spin-orbit-coupling-induced splitting of the d shell is small but noticeable. [Pg.628]

Knowledge of the accurate electron density is decisive especially for the development of chemical concepts that are based on the analysis of this observable. Such concepts are Gillespie s valence-shell electron-pair repulsion model [1149] or the ligand-induced charge concentrations [880,1150-1152] that are designed to predict molecular structures and even chemical reactivity. Both approaches can be related to Bader s theory of atoms in molecules [1153], for which relativistic generalizations have been discussed in the literature [1154,1155]. [Pg.628]


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