Propargylimine (HC≡CH–CH=NH), detected toward the Galactic Center molecular cloud G+0.693‒0.027, is a potential a nitrogen-bearing 3C-atom species in prebiotic chemistry. In this study, we present a comprehensive computational investigation of its thermodynamics, reaction mechanism, electro-optical properties, global reactivity descriptors, and vibrational spectroscopic signatures. The formation of Z and E conformers of propargylimine was explored through radical-radical association pathway in the gas phase using density functional theory (M06-2X/aug-cc-pVTZ), and benchmarked with CCSD(T)/aug-cc-pVTZ single-point calculations. Thermodynamic parameters, electro-optical properties, global reactivity descriptors, and molecular electrostatic potential surfaces were evaluated to assess its chemical stability and detectability. The simulated IR spectrum provides characteristic vibrational markers, particularly the C=N stretch at 1691.9 cm‒1 and N–H stretching bands (~3430–3447 cm‒1), which may facilitate astronomical identification. UV absorption features and the electronic absorption properties of propargylimine were investigated using time-dependent density functional theory (TD-DFT). This work offers a theoretical framework for understanding its formation and spectroscopic features, reinforcing its role as a chemically robust molecule in the nitrogen-bearing chemistry and molecular complexity in Galactic Center molecular clouds.
Mishra et al. (Tue,) studied this question.
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