Yurchenko, Sergei N;
Owens, Alec;
Kefala, Kyriaki;
Tennyson, Jonathan;
(2024)
ExoMol line lists – LVII: High accuracy ro-vibrational line list for methane (CH4).
Monthly Notices of the Royal Astronomical Society
, 528
(2)
pp. 3719-3729.
10.1093/mnras/stae148.
Preview |
Text
stae148.pdf Download (1MB) | Preview |
Abstract
The MM ro-vibrational line list for methane (12CH4) is presented; MM covers wavelengths λ > 0.83 μm (wavenumbers up to 12 000 cm−1) and contains over 50 billion transitions between 9 155 208 states with total angular momentum J ≤ 60. MM was generated through solution of the nuclear motion Schrödinger equation using variational program TROVE for an empirically-derived potential energy surface (PES) and a new high-level ab initio dipole moment surface. The PES was constructed by fitting the ro-vibrational energies of CH4 to a set of highly accurate, experimentally-derived energies. Molecular states are classified using the Td(M) symmetry group and are fully assigned with rotation and vibration quantum numbers. The MM line list is adapted to high-resolution applications by replacing the calculated ro-vibrational energies with the experimentally-derived values where available, namely for 23 208 states with J ≤ 27 below 9986 cm−1. Doing so leads to over 1 000 000 experimentally-derived CH4 lines compared to approximately 330 000 lines of 12CH4 in the HITRAN database. The MM line list is shown to be more complete than the recent HITEMP methane line list. Methane spectra computed using MM across a broad range of temperatures and wavenumbers show excellent agreement with experiment. The MM line list supersedes the previous ExoMol methane line lists 10to10 and 30to10 both in terms accuracy and coverage. Together with the pre-computed ExoMolOP molecular atmospheric opacity tables, it is now the recommended CH4 dataset in the ExoMol database (www.exomol.com).
| Type: | Article |
|---|---|
| Title: | ExoMol line lists – LVII: High accuracy ro-vibrational line list for methane (CH4) |
| Open access status: | An open access version is available from UCL Discovery |
| DOI: | 10.1093/mnras/stae148 |
| Publisher version: | http://dx.doi.org/10.1093/mnras/stae148 |
| Language: | English |
| Additional information: | Copyright © The Author(s) 2024. Published by Oxford University Press on behalf of Royal Astronomical Society. This is an Open Access article distributed under the terms of the Creative Commons Attribution License (https://creativecommons.org/licenses/by/4.0/), which permits unrestricted reuse, distribution, and reproduction in any medium, provided the original work is properly cited. |
| Keywords: | Molecular data, exoplanets, stars: atmospheres, stars: low-mass |
| 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 UCL > Provost and Vice Provost Offices > UCL BEAMS > Faculty of Maths and Physical Sciences > London Centre for Nanotechnology |
| URI: | https://discovery.ucl.ac.uk/id/eprint/10186044 |
Archive Staff Only
 |
View Item |
