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 |