Abstract: | Both STO-3G ab initio and s-p separation-type-modified INDO semiempirical methods were applied to molecular-orbital calculation of the N20 molecule. From these two methods, the optimized bond distances between the nearest N atoms (dn-n) and the most calculated thermodynamic data are close to each other. The positive values of ΔHa° and ΔGa° for the atomization reaction in this work prove that N20 is stable. In contrast to conventional INDO and MINDO/3, but similar to former AMI and MNDO calculations, both ΔHr° and ΔGr° are positive in the formation reaction, which indicates that N20 belongs to the category of high-energy molecules. |