Abstract

The reactions of the first-row transition metal cations, Sc+ (3D,1D), Ni+ (2D), Cu+ (1S), with NH3 have been studied by the multiconfigurational and multireference-based theories, to clarify the similarities and differences in the reactivity of early (Sc+) and late (Ni+, Cu+) transition metal cations. In all the cases, the ion–dipole complex, MNH3+, is initially formed with a C3v symmetry structure, which is the most stable complex in the respective potential energy surfaces except for Sc+ (1D). The M+–NH3 binding energy was evaluated as 42.4, 37.8, 50.9, and 48.1 kcal/mol for Sc+ (3D), Sc+ (1D), Ni+, and Cu+, respectively. In the second step, M+ is expected to activate one N–H bond of NH3, leading to the insertion complex, HMNH2+. In Sc+ (3D,1D), three different stationary points of HScNH2+, i.e., Cs (in-plane), Cs (out-of-plane), and C2v structures, were located, which correspond to a minimum point, a first-order saddle point, and a second-order saddle point, respectively. In these complexes, the singlet state originating from Sc+ (1D) is largely stabilized compared to the triplets. The singlet HScNH2+ (in-plane) is calculated to be the most stable compound. There are three dissociation channels from HScNH2+, i.e., →ScNH2++H, →ScH++NH2, and →ScNH++H2. The third dissociation occurs through the transition state of a four-centered structure, with a small activation barrier of 23 kcal/mol, in both singlet and triplet surfaces. As to the late transition metal cations Ni+ and Cu+, there is no intermediate complex of HMNH2+, thus, all the dissociations occur through highly vibrational excitations of MNH3+. The calculated results are consistent with experimental observations.

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