Abstract
This work emphasizes the stability of C 6 N linear carbon chains and carbon clusters containing three-body rings. C 6 N possesses at least 44 neutral isomers and 38 and 35 isomers with a negative or a positive charge. The lowest-energy structures, which can be candidates for laboratory and astrophysical detection, were studied with RCCSD(T)-F12 and MRCI/CASSCF, specifying properties for various electronic states. Neutral C 6 N displays two prominent equilibrium structures, a nitrogen-terminated linear form (X 2 Π) and a form (X 2 B 2 ) containing a three-carbon ring. They are separated by 0.21 eV. For the linear one, Renner–Teller and spin–orbit effects are expected. Its equilibrium spin–orbit constant ∣ ∣ was predicted to be 29.09 cm −1 , the dipole moment was computed to be 0.2059 D, and B e was computed to be 868.20 MHz, very close to the experimental value (B 0 (exp)-B e (calc) ∼ 4.9 MHz). The anion presents two stable forms, a linear triplet (X 3 Σ − ) and a (X 1 A 1 ) isomer, whereas for the cation most stable structures are both linear. For the linear anion and the two linear cations B 0 was estimated to be 870.05 MHz, 875.72 MHz, and 917.36 MHz and μ was estimated to be 4.4200 D, 4.2013D, and 0.7828D. For the neutral form, Ae = 45048.74 MHz, Be = 1062.78 MHz, Ce = 1038.30 MHz, and μ = 0.8840 D, whereas for the negative form, Ae = 40087.48 MHz, Be = 1067.35 MHz, Ce = 1039.67 MHz, and μ = 6.2854 D. Below the electron affinity of the most stable isomer (EA = −3.42 eV), the linear anion displays three probably existing electronic states. Detectability is discussed in terms of the symmetry and spin multiplicity of the ground electronic states.
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CITATION STYLE
Al-Mogren, M. M., & Senent, M. L. (2017). Theoretical Characterization of C 6 N, C 6 N − , and C 6 N +. The Astrophysical Journal, 842(2), 107. https://doi.org/10.3847/1538-4357/aa719f
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