A FULL IAM ANALYSIS OF TORSION IN THE GROUND STATE MILLIMETER WAVE SPECTRUM OF METHYL FORMATE.

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1993

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Ohio State University

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The rotational spectrum of methyl formate has been extensively measured and analysed by PAM methods up to high J $values^{(1,2)}$. We have re-analysed these results by an IAM technique not calling for large matrix $diagonalisation^{(3)}$ and carried out further measurements in the 140-160 GHz band. The Hamiltonian used utilises a planar rotation which transforms the quartic and sextic centrifugal distortion terms to an internal axes $system^{(4,5)}$. Our analysis gives comparable rms deviations with 10 fewer parameters, and leads to a 2.5\% smaller $\nu_{3}$ value of 391.592(168) $cm^{-1}$ with slight changes in the rotation and centrifugal constants.

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1)Plummer G.M., Herbst E., De Lucia F.C. and Blake G.A., Astrophys.J.Suppl.Ser., 55, 633-656 (1984). 2)Plummer G.M., Herbst E., De Lucia F.C. and Blake G.A., Astrophys.J.Suppl.Ser., 60, 949-961 (1986). 3)Nadgaran H., Baker J.G., ``47th International symposium on Molecular Spectroscopy'', Columbus, Ohio, USA, FD14 (1992). 4)Maes H., Wlodarczak G., Boucher D. and Demaison J.Z., Naturforsch, 42a, 97-102 (1987). 5)Nadgaran H., Baker J.G., ``Twelfth Colloquium on High Resolution Spectroscopy'', Dijon, France, J38 (1991).
Author Institution: c/o N.Riazi, Department of Physics, University of Shiraz; Schuster Laboratory., University of Manchester

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