Line mixing in Raman scattering spectra of CO2 modelled by a non-Markovian Energy-Corrected Sudden approach
Non-Markovian Energy-Corrected Sudden modelling of room-temperature CO 2 Raman scattering spectra up to the far wing is revisited and completed for gas densities between 1 and 45 amagat. The model parameters are fitted on an extended set of low-pressure isolated line widths including very high value...
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Published in | Molecular physics Vol. 110; no. 17; pp. 2077 - 2089 |
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Main Authors | , |
Format | Journal Article |
Language | English |
Published |
Abingdon
Taylor & Francis Group
01.09.2012
Taylor & Francis Ltd Taylor & Francis |
Subjects | |
Online Access | Get full text |
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Summary: | Non-Markovian Energy-Corrected Sudden modelling of room-temperature CO
2
Raman scattering spectra up to the far wing is revisited and completed for gas densities between 1 and 45 amagat. The model parameters are fitted on an extended set of low-pressure isolated line widths including very high values of the rotational quantum number J and well reproduce the decreasing of line broadening for the experimentally studied J-values. From calculations of the absolute-intensity rototranslational spectrum at 23 amagat, it is shown that the traditional adiabaticity factor of De Pristo gives a more coherent description of low-pressure line widths and high-pressure wing intensities than the two-parameter factor of Birnbaum-Cohen. A simple qualitative correction of the ECS-modelled intensities for the induced and cross allowed-induced scattering appears to be insufficient to match the experimental data in the spectral wing. Theoretical spectral shapes are also calculated for the O-Q-S branches of vibrotational ν
1
and 2ν
2
Raman bands and compared to experimental results in the density range 1-45 amagat. |
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ISSN: | 0026-8976 1362-3028 |
DOI: | 10.1080/00268976.2012.683458 |