Identifying new nitrogenated hydrocarbon molecules in
the interstellar
medium (ISM) is challenging because of the lack of comprehensive spectroscopic
data from experiments. In this computational work, we focus on investigating
the structures, relative energies, spectroscopic constants, and energy
landscape of the cyclic isomers of diazirine (c-CH2N2) using ab initio quantum chemical methods.
Density functional theory (DFT) methods and coupled cluster theory
with singles and doubles including perturbative triples [CCSD(T)]
and CCSD(T) with the explicitly correlated F12b correction [CCSD(T)-F12b]
were employed for this purpose along with large correlation consistent
cc-pVTZ, cc-pVQZ, and cc-pV5Z basis sets. Harmonic vibrational frequencies,
infrared vibrational intensities, rotational constants, and dipole
moments are reported. Anharmonic vibrational fundamentals along with
centrifugal distortion constants, and vibration–rotation interaction
constants are also reported for all the cyclic isomers. The energies
computed with the CCSD(T) and CCSD(T)-F12b methods were extrapolated
to the one-particle complete basis set (CBS) limit following a three-point
formula. At the CCSD(T)-F12b/CBS level of theory, the 3,3H-diazirine (c-CH2N2) is the lowest energy cyclic
isomer followed by 1,3H-diazirine, (E)-1,2H-diazirine, and (Z)-1,2H-diazirine, which are 20.1, 47.8, and 51.3 kcal mol–1 above the 3,3H-diazirine, respectively.
Accurate structures and spectroscopic constants that are reported
here could be useful for future identification of these cyclic nitrogenated
organic molecules in the interstellar medium or circumstellar disks.