Zak, EJ;
Tennyson, J;
Polyansky, OL;
Lodi, L;
Zobov, NF;
Tashkun, SA;
Perevalov, VI;
(2017)
Room temperature linelists for CO₂ asymmetric isotopologues with ab initio computed intensities.
Journal of Quantitative Spectroscopy and Radiative Transfer
, 203
10.1016/j.jqsrt.2017.01.037.
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Abstract
The present paper reports room temperature line lists for six asymmetric isotopologues of carbon dioxide: ¹⁶O¹²C¹⁸O (628), ¹⁶O¹²C¹⁷O (627), ¹⁶O¹³C¹⁸O (638), ¹⁶O¹³C¹⁷O (637), ¹⁷O¹²C¹⁸O (728) and ¹⁷O¹³C¹⁸O (738), covering the range 0–8000 cm⁻¹. Variational rotation-vibration wavefunctions and energy levels are computed using the DVR3D software suite and a high quality semi-empirical potential energy surface (PES), followed by computation of intensities using an ab initio dipole moment surface (DMS). A theoretical procedure for quantifying sensitivity of line intensities to minor distortions of the PES/DMS renders our theoretical model as critically evaluated. Several recent high quality measurements and theoretical approaches are discussed to provide a benchmark of our results against the most accurate available data. Indeed, the thesis of transferability of accuracy among different isotopologues with the use of mass-independent PES is supported by several examples. Thereby, we conclude that the majority of line intensities for strong bands are predicted with sub-percent accuracy. Accurate line positions are generated using an effective Hamiltonian, constructed from the latest experiments. This study completes the list of relevant isotopologues of carbon dioxide; these line lists are available to remote sensing studies and inclusion in databases.
Type: | Article |
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Title: | Room temperature linelists for CO₂ asymmetric isotopologues with ab initio computed intensities |
Open access status: | An open access version is available from UCL Discovery |
DOI: | 10.1016/j.jqsrt.2017.01.037 |
Publisher version: | http://dx.doi.org/10.1016/j.jqsrt.2017.01.037 |
Language: | English |
Additional information: | © 2017 The Author. Published by Elsevier Ltd. This is an open access article under the CC BY-NC-ND license (http://creativecommons.org/licenses/by-nc-nd/4.0/). |
UCL classification: | UCL UCL > Provost and Vice Provost Offices > UCL BEAMS UCL > Provost and Vice Provost Offices > UCL BEAMS > Faculty of Maths and Physical Sciences UCL > Provost and Vice Provost Offices > UCL BEAMS > Faculty of Maths and Physical Sciences > Dept of Physics and Astronomy |
URI: | https://discovery.ucl.ac.uk/id/eprint/1543005 |
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