Answers are grounded in this paper and cite their sources.
The electronic structure and energy curves of the 15Σ g + and 25Σ g + states of N2 have been analysed using the multi-configuration self-consistent-field (MC-SCF) method for calculating the wavefunctions and energies. The ab initio model curve for the 15Σ g + state obtains an r e of 1·69 Å and a D e of 825 cm-1. There is also a barrier with a maximum at 2·21 Å with a height of about 800 cm-1 which is a novel feature of this calculation. The potential supports two bound vibrational levels and two shape resonances for J=0. The calculated curve differs most from the semi-empirical curve of Carroll in having a larger r e by about 0·14 Å and a well depth smaller by 250 cm-1. The 5Σ g + curve is known experimentally to predissociate both the B 3Π g and a 1Π g vibration-rotation levels above the dissociation limit. Conversely, two-body radiative association of two N(4 S) atoms is known to occur through the interaction of the 15Σ g + and B and a states. The two-body radiative rates are analysed in terms of the likely spin-orbit interaction between the 15Σ g + and B and a states and the ratio of these rates is calculated under the assumption that the predissociation rate exceeds the radiative in both cases. The ratio of the two-body associative rates kB/ka is calculated to be roughly 20 which is to be compared to an experimental ratio of 32.
No takes yet. Share an insight, caveat, or question.
Krauss et al. (1976) studied this question.
Synapse has enriched 10 related papers. Consider them for comparative context: