Xinchuan Huang (黄新川) , Sergey A. Tashkun , David W. Schwenke
{"title":"Accurate N2O IR line lists with consistent empirical line positions: ABG-IMRHT and Ames-2000K","authors":"Xinchuan Huang (黄新川) , Sergey A. Tashkun , David W. Schwenke","doi":"10.1016/j.jqsrt.2025.109502","DOIUrl":null,"url":null,"abstract":"<div><div>We report the second generation of Ames N<sub>2</sub>O IR line lists, ABG-IMRHT for room-temperature and Ames-2000K for high temperature applications. The ABG-IMRHT line list utilized a new potential energy surface (PES), B1b, refined from a refit of Schröder’s Comp I PES [10.1515/zpch-2015–0622] with σ<sub>rms</sub> = 0.006 cm<sup>-1</sup> for all reliable <sup>14</sup>N<sub>2</sub><sup>16</sup>O levels in HITRAN2020 [10.1016/j.jqsrt.2021.107949], and a new dipole moment surface (DMS) G10K carrying fitting σ<sub>rms</sub> = 6.1 × 10<sup>–7</sup> au up to 10,000 cm<sup>-1</sup>. Compared to the previous Ames-296K line list, the PES and DMS upgrades have significantly reduced the line position deviations (δ) and relative intensity deviations (δ %), and maintained consistent accuracy across isotopologues. The line positions of the new ABG (<strong>A</strong>mes <strong>B</strong>1b + <strong>G</strong>10K) line lists including 12 stable N<sub>2</sub>O isotopolouges are enhanced by ∼100,000 global EH model based <sup>14</sup>N<sub>2</sub><sup>16</sup>O levels from NOSL-296, and empirical levels determined from <strong>I</strong>AO, <strong>M</strong>ARVEL, <strong>R</strong>ITZ, <strong>H</strong>ITRAN, and JPL(<strong>T</strong>oth) datasets, hence denoted ABG-<strong>IMRHT.</strong> Simple 0<sup>th</sup>-2<sup>nd</sup> order corrections are determined for E<sub>NOSL</sub> of about 20 vibrational states above 10,000 cm<sup>-1</sup>, based on E<sub>NOSL</sub>, E<sub>RITZ</sub>, and E<sub>MARVEL</sub> comparison. Uncertainty estimates are given for upper and lower state energies (<em>E</em>' and <em>E</em>\"), line positions, and IR intensities. The Ames-2000K line list contains 3.4 billion IR transitions covering the 0–15,000 cm<sup>-1</sup> range with <em>J</em><sub>max</sub>=210 and <em>E</em>'/<em>E</em>\"=0.125 Hartree (above the PES minimum) for <sup>14</sup>N<sub>2</sub><sup>16</sup>O. It combines strengths of three components: “Ames-1″ computed using Ames-1 PES and a weighted DMS “G2d” for 12 isotopologues, “B1b” for <sup>14</sup>N<sub>2</sub><sup>16</sup>O computed using B1b PES and G10K DMS with <em>E</em>' < 16,000 cm<sup>-1</sup>; and ABG-IMRHT line list. Comparison with HITEMP [10.1016/j.jqsrt.2019.04.040] and UCL TYM (ExoMol) [10.1093/mnras/stae2201] line lists are presented and discussed at <em>T</em> > 1000 K. This study represents a higher level of experiment-model-theory synergy, and a “block” approach for hot IR line list construction. The line lists and related datafiles are available online [<span><span>10.5281/zenodo.14174306</span><svg><path></path></svg></span>].</div></div>","PeriodicalId":16935,"journal":{"name":"Journal of Quantitative Spectroscopy & Radiative Transfer","volume":"343 ","pages":"Article 109502"},"PeriodicalIF":2.3000,"publicationDate":"2025-04-29","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"0","resultStr":null,"platform":"Semanticscholar","paperid":null,"PeriodicalName":"Journal of Quantitative Spectroscopy & Radiative Transfer","FirstCategoryId":"101","ListUrlMain":"https://www.sciencedirect.com/science/article/pii/S0022407325001645","RegionNum":3,"RegionCategory":"物理与天体物理","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"Q2","JCRName":"OPTICS","Score":null,"Total":0}
引用次数: 0
Abstract
We report the second generation of Ames N2O IR line lists, ABG-IMRHT for room-temperature and Ames-2000K for high temperature applications. The ABG-IMRHT line list utilized a new potential energy surface (PES), B1b, refined from a refit of Schröder’s Comp I PES [10.1515/zpch-2015–0622] with σrms = 0.006 cm-1 for all reliable 14N216O levels in HITRAN2020 [10.1016/j.jqsrt.2021.107949], and a new dipole moment surface (DMS) G10K carrying fitting σrms = 6.1 × 10–7 au up to 10,000 cm-1. Compared to the previous Ames-296K line list, the PES and DMS upgrades have significantly reduced the line position deviations (δ) and relative intensity deviations (δ %), and maintained consistent accuracy across isotopologues. The line positions of the new ABG (Ames B1b + G10K) line lists including 12 stable N2O isotopolouges are enhanced by ∼100,000 global EH model based 14N216O levels from NOSL-296, and empirical levels determined from IAO, MARVEL, RITZ, HITRAN, and JPL(Toth) datasets, hence denoted ABG-IMRHT. Simple 0th-2nd order corrections are determined for ENOSL of about 20 vibrational states above 10,000 cm-1, based on ENOSL, ERITZ, and EMARVEL comparison. Uncertainty estimates are given for upper and lower state energies (E' and E"), line positions, and IR intensities. The Ames-2000K line list contains 3.4 billion IR transitions covering the 0–15,000 cm-1 range with Jmax=210 and E'/E"=0.125 Hartree (above the PES minimum) for 14N216O. It combines strengths of three components: “Ames-1″ computed using Ames-1 PES and a weighted DMS “G2d” for 12 isotopologues, “B1b” for 14N216O computed using B1b PES and G10K DMS with E' < 16,000 cm-1; and ABG-IMRHT line list. Comparison with HITEMP [10.1016/j.jqsrt.2019.04.040] and UCL TYM (ExoMol) [10.1093/mnras/stae2201] line lists are presented and discussed at T > 1000 K. This study represents a higher level of experiment-model-theory synergy, and a “block” approach for hot IR line list construction. The line lists and related datafiles are available online [10.5281/zenodo.14174306].
期刊介绍:
Papers with the following subject areas are suitable for publication in the Journal of Quantitative Spectroscopy and Radiative Transfer:
- Theoretical and experimental aspects of the spectra of atoms, molecules, ions, and plasmas.
- Spectral lineshape studies including models and computational algorithms.
- Atmospheric spectroscopy.
- Theoretical and experimental aspects of light scattering.
- Application of light scattering in particle characterization and remote sensing.
- Application of light scattering in biological sciences and medicine.
- Radiative transfer in absorbing, emitting, and scattering media.
- Radiative transfer in stochastic media.