Eighty
three stationary points of MgC6H2 isomers
spanning from 0 to 215 kcal
mol–1 have been theoretically identified using density
functional theory at the B3LYP/6-311++G(2d,2p) level of theory. Among
them, four low-lying isomers lying within 23.06 kcal mol–1 (1 eV) have been further characterized in detail using high-level
coupled-cluster (CC) methods. The thermodynamically most stable isomer
turns out to be 1-magnesacyclohepta-4-en-2,6-diyne (1). The other three isomers, 3-magnesahepta-1,4,6-triyne (2), 1-magnesacyclohepta-2,3,4-trien-6-yne (3), and 1-magnesahepta-2,4,6-triyne
(4) lie 8.24, 19.76, and 21.36 kcal mol–1, respectively, above 1 at the ae-CCSD(T)/cc-pCVTZ level
of theory. All the four isomers are polar with a permanent electric
dipole moment (μ ≠ 0). Hence, they are potential candidates
for rotational spectroscopic studies. Considering the recent identification
of magnesium-bearing hydrocarbons such as, MgC2H and MgC4H in IRC+10216, it is believed that the current theoretical
data may be of relevance to laboratory molecular spectroscopic and
radioastronomical studies on MgC6H2 isomers.
The energetic and spectroscopic information gathered in this study
would aid the detection of low-lying MgC6H2 isomers
in the laboratory, which are indispensable for radioastronomical studies.
It is also noted here that neither the National Institute of Standards
and Technology Chemistry WebBook nor the Kinetic Database for Astrochemistry
lists any isomer of MgC6H2 at the moment. Therefore,
these isomers are studied here theoretically for the very first time.
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