LINE INTENSITY MEASUREMENTS IN $^{14}N^{16}_{2}O$ AND THEIR TREATMENT USING THE EFFECTIVE OPERATOR APPROACH. II. THE 5200 TO $6400 CM^{-1}$ REGION

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2002

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Ohio State University

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This work continues a series of publications devoted to the application of the effective operators approach to the analysis and prediction of vibration-rotation spectra of linear triatomic molecules. In that frame, the present work aims at describing line intensities of cold and hot bands of 14N216O in its ground electronic state in the spectral range above 3600cm−1. In N2O, vibrational interacting levels group in polyads, identified by the so-called polyad number P=2V1+V2+4V3, as a result of the relation 2ω14ω2ω3 existing between the harmonic frequencies. The absorption spectra of N2O, at room temperature, have been recorded in Brussels over the whole range between 3600 and 11000cm−1 using a Bruker IFS120HR Fourier transform spectrometer. The measurement and analysis of absolute line intensities in the region between 4300 and 5200cm−1, involving bands associated with transitions corresponding to ΔP=7,8 and 9, was done recently.a We are now measuring absolute line intensities for cold and hot bands associated with transitions corresponding to ΔP=10 and 11, observed in the range from 5200 to 6400cm−1. Using wavefunctions previously determined from a global fit of an effective hamiltonian to about 18000 line positions,b parameters of a corresponding effective dipole moment are then fitted to these experimental intensities. Results will be presented and discussed.

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aL. Daumont, J. Vander Auwera, J-L. Teffo, V. I. Perevalov and S. A. Tashkun, J. Mol. Spectrosc. 208, 281-291 (2001). bA. Camparque, G. Weirauch, S. A. Tashkun, V. I. Perevalov, and J-L. Teffo, J. Mol. Spectrosc. 209, 198-206 (2001).


Author Institution: Laboratoire de Chimie Physique Mol'{e}culaire C. P. 160/09, Universit'{e} Libre de Bruxelles; Groupe de Spectrom'{e}trie Mol'{e}culaire et Atmosph'{e}rique, ESA CNRS 6089, Universit'{e} de Reims, Facult'{e} des Sciences, Moulin de la Housse; Institute of Atmospheric Optics, Russian Academy of Sciences, Siberian Branch; Laboratoire de Physique Mol'{e}culaire et Applications, CNRS, bo^{i}te 76, Universit'e Pierre et Marie Curie

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