{"title":"Three-states model for calculating the X-X rovibrational transition intensities in hydroxyl radical","authors":"V.G. Ushakov , A. Yu. Ermilov , E.S. Medvedev","doi":"10.1016/j.jms.2024.111977","DOIUrl":null,"url":null,"abstract":"<div><div>The best available line list of OH [Brooke et al. JQSRT, 168 (2016) 142] contains the high-quality line frequencies, yet the line intensities need refinement because the model function used to interpolate the RKR potential and to extrapolate it into the repulsion region was not analytic [Medvedev et al. Mol. Phys. doi: 10.1080/00268976.2024.2395439], and also because the coupling between the ground <span><math><mrow><msup><mrow><mi>X</mi></mrow><mrow><mn>2</mn></mrow></msup><mi>Π</mi></mrow></math></span> and first excited <span><math><mrow><msup><mrow><mi>A</mi></mrow><mrow><mn>2</mn></mrow></msup><msup><mrow><mi>Σ</mi></mrow><mrow><mo>+</mo></mrow></msup></mrow></math></span> electronic states was treated by the perturbation theory. In this paper, we performed <em>ab initio</em> calculations of all necessary molecular functions at <span><math><mrow><mi>r</mi><mo>=</mo><mn>0</mn><mo>.</mo><mn>4</mn></mrow></math></span>-8.0 bohr, and then we construct fully analytic model functions entering the Hamiltonian. The model functions were fitted to both the <em>ab initio</em> data and the available experimental data on the line positions and energy levels, the relative line intensities, and the transition dipole moments derived from the measured permanent dipoles. The system of three coupled Schrödinger equations for two multiplet components of the <span><math><mi>X</mi></math></span> state plus the <span><math><mi>A</mi></math></span> state was solved to calculate the energy levels and the line intensities. The new set of the Einstein <em>A</em> coefficients permits to decrease the scatter of the logarithmic populations of the ro-vibrational levels derived from the observed radiation fluxes [Noll et al. Atmos. Chem. Phys. 20 (2020) 5269], to achieve better agreement with the measured relative intensities, and to obtain significant differences in the intensities of the <span><math><mi>Λ</mi></math></span> doublets for large <span><math><mi>v</mi></math></span> and <span><math><mi>J</mi></math></span> as observed by Noll et al. The <span><math><mi>X</mi></math></span>-<span><math><mi>A</mi></math></span> coupling fully modifies the Q-line intensities at high <span><math><mi>J</mi></math></span> by removing the well-known <span><math><msup><mrow><mi>J</mi></mrow><mrow><mo>−</mo><mn>2</mn></mrow></msup></math></span> dependence. A new line list is constructed where the transition frequencies are from Brooke et al. and the Einstein <span><math><mi>A</mi></math></span> coefficients are from the present study. However, not all the problems with the intensities were resolved, presumably due to the neglect of the interaction with the <span><math><mrow><msup><mrow></mrow><mrow><mn>4</mn></mrow></msup><msup><mrow><mi>Σ</mi></mrow><mrow><mo>−</mo></mrow></msup><msup><mrow><mo>,</mo></mrow><mrow><mn>2</mn></mrow></msup><msup><mrow><mi>Σ</mi></mrow><mrow><mo>−</mo></mrow></msup></mrow></math></span> and <span><math><mrow><msup><mrow></mrow><mrow><mn>4</mn></mrow></msup><mi>Π</mi></mrow></math></span> repulsive electronic terms.</div></div>","PeriodicalId":16367,"journal":{"name":"Journal of Molecular Spectroscopy","volume":"407 ","pages":"Article 111977"},"PeriodicalIF":1.4000,"publicationDate":"2025-01-01","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"0","resultStr":null,"platform":"Semanticscholar","paperid":null,"PeriodicalName":"Journal of Molecular Spectroscopy","FirstCategoryId":"101","ListUrlMain":"https://www.sciencedirect.com/science/article/pii/S0022285224001048","RegionNum":4,"RegionCategory":"物理与天体物理","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"Q4","JCRName":"PHYSICS, ATOMIC, MOLECULAR & CHEMICAL","Score":null,"Total":0}
引用次数: 0
Abstract
The best available line list of OH [Brooke et al. JQSRT, 168 (2016) 142] contains the high-quality line frequencies, yet the line intensities need refinement because the model function used to interpolate the RKR potential and to extrapolate it into the repulsion region was not analytic [Medvedev et al. Mol. Phys. doi: 10.1080/00268976.2024.2395439], and also because the coupling between the ground and first excited electronic states was treated by the perturbation theory. In this paper, we performed ab initio calculations of all necessary molecular functions at -8.0 bohr, and then we construct fully analytic model functions entering the Hamiltonian. The model functions were fitted to both the ab initio data and the available experimental data on the line positions and energy levels, the relative line intensities, and the transition dipole moments derived from the measured permanent dipoles. The system of three coupled Schrödinger equations for two multiplet components of the state plus the state was solved to calculate the energy levels and the line intensities. The new set of the Einstein A coefficients permits to decrease the scatter of the logarithmic populations of the ro-vibrational levels derived from the observed radiation fluxes [Noll et al. Atmos. Chem. Phys. 20 (2020) 5269], to achieve better agreement with the measured relative intensities, and to obtain significant differences in the intensities of the doublets for large and as observed by Noll et al. The - coupling fully modifies the Q-line intensities at high by removing the well-known dependence. A new line list is constructed where the transition frequencies are from Brooke et al. and the Einstein coefficients are from the present study. However, not all the problems with the intensities were resolved, presumably due to the neglect of the interaction with the and repulsive electronic terms.
期刊介绍:
The Journal of Molecular Spectroscopy presents experimental and theoretical articles on all subjects relevant to molecular spectroscopy and its modern applications. An international medium for the publication of some of the most significant research in the field, the Journal of Molecular Spectroscopy is an invaluable resource for astrophysicists, chemists, physicists, engineers, and others involved in molecular spectroscopy research and practice.