A Quantum Chemical Investigation of Electro-Optical Properties, and Spectroscopic Features of Propargylimine
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.
Authors
- P. K. Tandon
- Aftab Ahmad (ORCID: https://orcid.org/0000-0003-0686-0987)
- Amritanshu Shukla (ORCID: https://orcid.org/0000-0001-9352-4193)
- Parmanand Pandey
- Pravi Mishra (ORCID: https://orcid.org/0009-0009-9263-0395)
- Rachana Singh
- A. Misra
- Shivani .
- Manisha Yadav
Institutions
- University of Lucknow (IN)
Publication Details
- Journal
- Canadian Journal of Chemistry
- Published
- 2026-03-17
- DOI
- https://doi.org/10.1139/cjc-2025-0198
- Primary Topic
- Astrophysics and Star Formation Studies
- Type
- article
- Field-Weighted Citation Impact
- 0.00