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Prediction of molecular infrared band and line intensitiesThe general problem of predicting infrared intensities is examined. The problem of predicting line intensities is discussed with attention focussed specifically on the problem of predicting vibrational strengths (or total band intensities). Two methods are considered: predictions based on ab initio quantum mechanical calculations, and predictions based on the transfer of atomic polar tensor parameters from small model molecules to the molecule of interest. Comparisons of predicted spectra with experimental spectra are shown for CH3OH, CH3OCH3, C2H5OH, and HOC2. It is suggested that the most important application of this work may be to the prediction of intensities for free radicals, ions, and reactive intermediates so that the infrared spectrum can be used in the quantitative analysis for these interesting species.
Document ID
19820017171
Acquisition Source
Legacy CDMS
Document Type
Conference Paper
Authors
Person, W. B.
(Florida Univ. Gainesville, FL, United States)
Date Acquired
August 10, 2013
Publication Date
April 1, 1982
Publication Information
Publication: NASA. Goddard Space Flight Center Vibrational-Rotational Spectry. for Planetary Atmospheres, Vol. 1
Subject Category
Lunar And Planetary Exploration
Accession Number
82N25047
Funding Number(s)
CONTRACT_GRANT: NSF CHE-78-18940
Distribution Limits
Public
Copyright
Work of the US Gov. Public Use Permitted.

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