Abstract
The structure, vibrational frequencies, isomerization, and dissociation of CCNN were studied using the Hartree-Fock (HF), Moller-Plesset from second to fourth order (MP2, MP4SDQ, NP4SDTQ), configuration [CISD, QCSID, and QCISDT(T)] methods as well as the B3LYP and B3PW91 density functional theory methods. A schematic potential energy surface of the C2N2 was established at the QCISD(T)/6-311G(3df)//QCSIDT(T)/6-311G(d) single-point level. This enabled to compare the kinetic stability of CCNN with other C2N2 isomers. Finally, the possible formation of CCNN in laboratory and in interstellar space was confirmed.
| Original language | English |
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| Pages (from-to) | 1745-1754 |
| Number of pages | 10 |
| Journal | Journal of Chemical Physics |
| Volume | 113 |
| Issue number | 5 |
| DOIs | |
| Publication status | Published - Aug 2000 |
| Externally published | Yes |