THE STRUCTURE OF Ne-HCN COMPARED WITH THOSE OF Ar-HCN AND Kr-HCN

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1992

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Ohio State University

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The J=0→1,1→2, and 2→3K=0 rotational transitions have been observed for several isotopic species of the Ne-HCN dimer. Rotational constants obtained by fitting the line centers are listed below. [FIGURE] χaa(21Ne), the hyperfine interaction constant for 21Ne, was found to be -0.246 MHz in the J=0→1 transition of 21NeHC15N. The value of χaa(14N) in 20NcHC14N is highly dependent on J being −0.982,−1.034, and −1.109 MHz for J=1,2,3 respectively. A number of KO transitions have also been observed including what appears to be inversion doubling of the 111→212 transition. The Stark effect has been observed for several transitions and differs from that predicted for a linear species. Our results indicate that Ne-HCN is even more highly nonrigid than ArHCN,1 with even stronger angular-radial coupling in the interaction potential.2,3 Kr-HCN, on the other hand, is more ``normal” than either.4.

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1K.R. Leopold, G.T. Fraser, F.J. Lin, D.D Nelson, JR., and W. Klemperer, J. Chem. Phys. 81 , 4922 (1984). 2T.D. Klots, C.E. Dykstra, and H.S. Gutowsky, J. Chem. Phys, 90 , 30 (1989). 3D.C. Clary, C.E. Dateo, and T. Stoecklin, J. Chem. Phys 93 , 7666(1990). 4T.C. Germann, T. Emisson, and H.S. Gutowsky, J. Chem. Phys. 95 6302 (1991).


Author Institution: Noyes Chemical Laboratory, University of Illinois

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