ExoMol line lists – LVII: High accuracy ro-vibrational line list for methane (CH4)

IF 4.7 3区 物理与天体物理 Q1 ASTRONOMY & ASTROPHYSICS Monthly Notices of the Royal Astronomical Society Pub Date : 2024-01-12 DOI:10.1093/mnras/stae148
Sergei N Yurchenko, Alec Owens, Kyriaki Kefala, Jonathan Tennyson
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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).
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ExoMol 谱线表 - LVII:甲烷 (CH4) 的高精度罗振谱线表
MM 涵盖波长 λ > 0.83 μm(波数高达 12 000 cm-1),包含总角动量 J ≤ 60 的 9 155 208 个状态之间的 500 多亿次跃迁。MM 是通过使用变分程序 trove 解决核运动薛定谔方程来生成的,该程序适用于根据经验得出的势能面(PES)和新的高级原子偶极矩面。势能面是通过将 CH4 的罗振能量与一组高精度的实验能量拟合而构建的。分子状态使用 Td(M)对称组进行分类,并完全分配了旋转和振动量子数。MM 线表适用于高分辨率应用,方法是将计算的旋转振动能量替换为可用的实验值,即 J ≤ 27 低于 9986 cm-1 的 23 208 个状态。这样就得到了超过 1,000,000 条实验得出的 CH4 线,而 HITRAN 数据库中的 12CH4 线约为 330,000 条。MM 线表比最近的 HITEMP 甲烷线表更加完整。在广泛的温度和波数范围内,使用 MM 计算的甲烷光谱与实验结果显示出极好的一致性。在精确度和覆盖范围方面,MM 甲烷谱线表分别以 10:10 和 30:10 的比例超越了之前的 ExoMol 甲烷谱线表。与预先计算的 ExoMolOP 分子大气不透明度表一起,它现在是 ExoMol 数据库(www.exomol.com)中推荐的 CH4 数据集。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
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来源期刊
CiteScore
9.10
自引率
37.50%
发文量
3198
审稿时长
3 months
期刊介绍: Monthly Notices of the Royal Astronomical Society is one of the world''s leading primary research journals in astronomy and astrophysics, as well as one of the longest established. It publishes the results of original research in positional and dynamical astronomy, astrophysics, radio astronomy, cosmology, space research and the design of astronomical instruments.
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