AN AB INITIO MOLECULAR ORBITAL STUDY ON THE STRUCTURE AND SPECTROSCOPIC PROPERTIES OF MAGNESIUM DICARBIDE

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1999

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Ohio State University

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A magnesium-bearing molecule MgC2 is one of the candidate to be found in the envelope of a carbon star. Element magnesium may be rich in astrophysical objects because the elemental cosmic abundance of magnesium and silicon is almost the same, while silicon containing molecules such as SiO,SiS,SiC,SiC2,SiC4,SiH4,SiN, have been found in interstellar space. Silicon dicarbide SiC2 was discovered in IRC+10216. Now, magnesium dicarbide, MgC2, is strongly expected to be observed. Since none of the experimental spectroscopic data on MgC2 has been reported in any frequency region, ab initio molecular orbital predicition has been requested for its identification. The MR-SDCI+Q calculations with augmented cc-pVQZ basis sets have predicted that the ground state MgC2(1A1) has T-shaped structure of C2v symmetry consisting of Mg cation and CC moiety with the dipole moment of 7.9 Debye. The CC and MgC distances have been found to be 1.275 and 2.012 \AA in its equilibrium geometry. The MR-SDCI+Q three-dimensional potential energy surface consisting of 497 points were analysed by the 2nd-order perturbation theory, predicting the rotational constants A0,B0, and C0 to be 51794.0,11493.9 and 9378.7 MHz, and the centrifugal distortion constants ΔJ,ΔJK,ΔK,δJ,δK to be 0.014,0.21,−0.023,0.0027,0.14MHz, respectively. The ν1(CCstretching),ν2(MgC2streching), and 3(bending) vibrational frequencies have been estimated to be 1704.2, 594.8 and 455.8cm−1, respectively. These results indicate that MgC2 molecule is a rigid molecule unlike the analogue SiC2, which is known as a molecule with large-amplitude motion. Toward the laser induced fluorescent spectroscopy, the vertical excitation energies for A¯1A1X~1A1 and B¯1B2 transitions have also been calculated to be 8334 and 13034cm−1, respectively, at the CAS-SCF level of theory.

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Author Institution: Department of Chemistry, Faculty of Science, Ochanomizu University; National Institute of Materials and Chemical Research, 1-1 Higashi; Hiroshima City University, 3-4-1 Ozukahigashi; Nobeyama Radio Obverservatory, Minamimaki

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