After n xA xA all ZZ tubes

8) and DHAn · PCn · Na+, ASP · PCn · Na+ and ASP · DHAn · Na+ (Fig. 9). It has also allowed us to determine the interaction energies of the net secondary productivity (NSP) complexes (Table 1 and Table 2). The most energetically favorable structures of the DHAn · PCn (geometry C) and ASP · DHAn (geometry B) complexes have similar interaction energies in vacuum and in polar solvents while for the cationized non-covalent complexes the close values of IE have the most energetically favorable structures of DHAn · PCn · Na+ (geometry C) and ASP · PCn · Na+ (geometry C).