Pub Date : 2024-04-21DOI: 10.1016/j.jms.2024.111906
George A. Pitsevich , Alex E. Malevich , Maksim Shundalau
Splitting of the ground state and some excited symmetric bending vibrational states due to inversion tunneling in the H3C− anion and H3Si radical is analyzed by numerically solving the vibrational Schrödinger equation of restricted (2D) dimensionality. We used the following two vibrational coordinates for the H3X structure (X = C, Si): the distance of the X atom from the plane of a regular triangle formed by three hydrogen atoms (1) and a symmetry coordinate composed of three distances between chemically non-bonded hydrogen atoms (2). The kinetic energy operator in this case takes the simplest form. The 2D potential energy surface (PES) in the given coordinates was calculated for H3C− at the CCSD(T)/aug-cc-pVTZ, CCSD(T)/aug-cc-pVQZ, CCSD(T)/aug-cc-pV5Z, CCSD(T)/CBS(TQ5), CCSD(T)/d-aug-cc-pVTZ, CCSD(T)/t-aug-cc-pVTZ, and CCSD(T)/q-aug-cc-pVTZ levels of theory, based on recommendations from recently published work [M.C. Bowman, B. Zhang, W.J. Morgan, H.F. Schaefer III, Mol.Phys., 117 (2019) 1069–1077]. The same 2D PES for the H3Si radical was calculated at the CCSD(T)/aug-cc-pVDZ CCSD(T)/aug-cc-pVTZ, CCSD(T)/aug-cc-pVQZ, and CCSD(T)/CBS(D,T,Q) as well as at the CCSD(T)/d-aug-cc-pVTZ, CCSD(T)/un-aug-cc-pVTZ, CCSD(T)/un-aug-cc-pVQZ levels of theory. The tunneling splittings for the D3C− anion and D3Si radical were calculated as well. The results of calculations demonstrate good agreement with available experimental data on umbrella vibration frequencies and inversion splittings for the title molecules.
通过数值求解限制维数(2D)的振动薛定谔方程,分析了 H3C- 阴离子和 H3Si 自由基中由于反向隧穿引起的基态和某些激发对称弯曲振动态的分裂。我们对 H3X 结构(X = C、Si)使用了以下两个振动坐标:X 原子到由三个氢原子组成的正三角形平面的距离 (1),以及由化学上不成键的氢原子之间的三个距离组成的对称坐标 (2)。在这种情况下,动能算子的形式最为简单。在给定坐标下计算了 H3C- 在 CCSD(T)/aug-cc-pVTZ、CCSD(T)/aug-cc-pVQZ、CCSD(T)/aug-cc-pV5Z 下的二维势能面(PES)、CCSD(T)/CBS(TQ5), CCSD(T)/d-aug-cc-pVTZ, CCSD(T)/t-aug-cc-pVTZ, and CCSD(T)/q-aug-cc-pVTZ levels of theory, based on recommendations from recent published work [M.C. Bowman, B. Zhang, W.J. Morgan, H.F. Schaefer III, Mol.Phys、117 (2019) 1069-1077].在 CCSD(T)/aug-cc-pVDZ、CCSD(T)/aug-cc-pVTZ、CCSD(T)/aug-cc-pVQZ 和 CCSD(T)/CBS(D,T,Q)以及 CCSD(T)/d-aug-cc-pVTZ、CCSD(T)/un-aug-cc-pVTZ、CCSD(T)/un-aug-cc-pVQZ 理论水平上计算了 H3Si 自由基的相同二维 PES。同时还计算了 D3C- 阴离子和 D3Si 自由基的隧道分裂。计算结果证明,标题分子的伞状振动频率和反转分裂与现有的实验数据十分吻合。
{"title":"The tunneling splittings of the ground state and some excited vibrational states for the inversion motion in H3C− anion and H3Si radical","authors":"George A. Pitsevich , Alex E. Malevich , Maksim Shundalau","doi":"10.1016/j.jms.2024.111906","DOIUrl":"10.1016/j.jms.2024.111906","url":null,"abstract":"<div><p>Splitting of the ground state and some excited symmetric bending vibrational states due to inversion tunneling in the H<sub>3</sub>C<sup>−</sup> anion and H<sub>3</sub>Si<sup><img></sup> radical is analyzed by numerically solving the vibrational Schrödinger equation of restricted (2D) dimensionality. We used the following two vibrational coordinates for the H<sub>3</sub>X structure (X = C, Si): the distance of the X atom from the plane of a regular triangle formed by three hydrogen atoms (1) and a symmetry coordinate composed of three distances between chemically non-bonded hydrogen atoms (2). The kinetic energy operator in this case takes the simplest form. The 2D potential energy surface (PES) in the given coordinates was calculated for H<sub>3</sub>C<sup>−</sup> at the CCSD(T)/aug-cc-pVTZ, CCSD(T)/aug-cc-pVQZ, CCSD(T)/aug-cc-pV5Z, CCSD(T)/CBS(TQ5), CCSD(T)/d-aug-cc-pVTZ, CCSD(T)/<em>t</em>-aug-cc-pVTZ, and CCSD(T)/q-aug-cc-pVTZ levels of theory, based on recommendations from recently published work [M.C. Bowman, B. Zhang, W.J. Morgan, H.F. Schaefer III, Mol.Phys., 117 (2019) 1069–1077]. The same 2D PES for the H<sub>3</sub>Si<sup><img></sup> radical was calculated at the CCSD(T)/aug-cc-pVDZ CCSD(T)/aug-cc-pVTZ, CCSD(T)/aug-cc-pVQZ, and CCSD(T)/CBS(D,T,Q) as well as at the CCSD(T)/d-aug-cc-pVTZ, CCSD(T)/un-aug-cc-pVTZ, CCSD(T)/un-aug-cc-pVQZ levels of theory. The tunneling splittings for the D<sub>3</sub>C<sup>−</sup> anion and D<sub>3</sub>Si<sup><img></sup> radical were calculated as well. The results of calculations demonstrate good agreement with available experimental data on umbrella vibration frequencies and inversion splittings for the title molecules.</p></div>","PeriodicalId":16367,"journal":{"name":"Journal of Molecular Spectroscopy","volume":"402 ","pages":"Article 111906"},"PeriodicalIF":1.4,"publicationDate":"2024-04-21","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"140775401","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":4,"RegionCategory":"物理与天体物理","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}
Pub Date : 2024-04-18DOI: 10.1016/j.jms.2024.111905
Wlodzimierz Jastrzebski , Jacek Szczepkowski , Pawel Kowalczyk
The polarisation labelling spectroscopy technique was applied to study the C X band system in potassium dimer. About 1100 new rotationally resolved molecular lines were measured in the 22100–24100 cm−1 spectral range. Perturbations of the lowest vibrational levels of the C state were localised and their origin discussed. A set of Dunham coefficients was deduced to fit the unperturbed levels of the C state with and and the potential energy curve of the state was constructed.
{"title":"The C1Πu state of potassium dimer revisited: An extensive study by polarisation labelling spectroscopy method","authors":"Wlodzimierz Jastrzebski , Jacek Szczepkowski , Pawel Kowalczyk","doi":"10.1016/j.jms.2024.111905","DOIUrl":"https://doi.org/10.1016/j.jms.2024.111905","url":null,"abstract":"<div><p>The polarisation labelling spectroscopy technique was applied to study the C<span><math><mrow><msup><mrow></mrow><mrow><mn>1</mn></mrow></msup><msub><mrow><mi>Π</mi></mrow><mrow><mi>u</mi></mrow></msub></mrow></math></span> <span><math><mo>←</mo></math></span> X<span><math><mrow><msup><mrow></mrow><mrow><mn>1</mn></mrow></msup><msubsup><mrow><mi>Σ</mi></mrow><mrow><mi>g</mi></mrow><mrow><mo>+</mo></mrow></msubsup></mrow></math></span> band system in potassium dimer. About 1100 new rotationally resolved molecular lines were measured in the 22100–24100 cm<sup>−1</sup> spectral range. Perturbations of the lowest vibrational levels of the C state were localised and their origin discussed. A set of Dunham coefficients was deduced to fit the unperturbed levels of the C<span><math><mrow><msup><mrow></mrow><mrow><mn>1</mn></mrow></msup><msub><mrow><mi>Π</mi></mrow><mrow><mi>u</mi></mrow></msub></mrow></math></span> state with <span><math><mrow><mn>0</mn><mo>≤</mo><mi>v</mi><mo>≤</mo><mn>38</mn></mrow></math></span> and <span><math><mrow><mn>18</mn><mo>≤</mo><mi>J</mi><mo>≤</mo><mn>101</mn></mrow></math></span> and the potential energy curve of the state was constructed.</p></div>","PeriodicalId":16367,"journal":{"name":"Journal of Molecular Spectroscopy","volume":"402 ","pages":"Article 111905"},"PeriodicalIF":1.4,"publicationDate":"2024-04-18","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"140619247","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":4,"RegionCategory":"物理与天体物理","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}
Pub Date : 2024-03-01DOI: 10.1016/j.jms.2024.111899
A.J. Barclay , A.R.W. McKellar , A. Pietropolli Charmet , N. Moazzen-Ahmadi
We report spectroscopic observation and theoretical calculations of a new isomer of (CS2)3 as observed in the regions of the ν3 fundamental band of CS2 (6.5 μm) and the ν1 + ν3 combination band (4.5 μm), using tunable laser sources and a pulsed supersonic slit-jet. The previously observed CS2 trimer has a barrel-shaped structure with three equivalent monomers and D3 symmetry. The new isomer consists of a staggered parallel “dimer pair” of equivalent CS2 monomers with a third CS2 monomer sitting “on top”, similar to the known non-cyclic CO2 trimer. This structure has C2 rotational symmetry corresponding to the b inertial axis of the trimer, as proven by observed nuclear spin statistics. Ab initio calculations correctly give the two observed isomer structures and indicate that they lie very close in binding energy.
{"title":"Spectroscopic observation and ab initio calculations of a new isomer of the CS2 trimer","authors":"A.J. Barclay , A.R.W. McKellar , A. Pietropolli Charmet , N. Moazzen-Ahmadi","doi":"10.1016/j.jms.2024.111899","DOIUrl":"https://doi.org/10.1016/j.jms.2024.111899","url":null,"abstract":"<div><p>We report spectroscopic observation and theoretical calculations of a new isomer of (CS<sub>2</sub>)<sub>3</sub> as observed in the regions of the ν<sub>3</sub> fundamental band of CS<sub>2</sub> (6.5 μm) and the ν<sub>1</sub> + ν<sub>3</sub> combination band (4.5 μm), using tunable laser sources and a pulsed supersonic slit-jet. The previously observed CS<sub>2</sub> trimer has a barrel-shaped structure with three equivalent monomers and <em>D</em><sub>3</sub> symmetry. The new isomer consists of a staggered parallel “dimer pair” of equivalent CS<sub>2</sub> monomers with a third CS<sub>2</sub> monomer sitting “on top”, similar to the known non-cyclic CO<sub>2</sub> trimer. This structure has <em>C</em><sub>2</sub> rotational symmetry corresponding to the <em>b</em> inertial axis of the trimer, as proven by observed nuclear spin statistics. <em>Ab initio</em> calculations correctly give the two observed isomer structures and indicate that they lie very close in binding energy.</p></div>","PeriodicalId":16367,"journal":{"name":"Journal of Molecular Spectroscopy","volume":"401 ","pages":"Article 111899"},"PeriodicalIF":1.4,"publicationDate":"2024-03-01","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"https://www.sciencedirect.com/science/article/pii/S0022285224000262/pdfft?md5=e2866be731d3b8c41008cac8033764e3&pid=1-s2.0-S0022285224000262-main.pdf","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"140103872","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":4,"RegionCategory":"物理与天体物理","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"OA","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}
Pub Date : 2024-03-01DOI: 10.1016/j.jms.2024.111902
Laiz R. Ventura, Ramon S. da Silva, Jayr Amorim, Carlos E. Fellows
Neutral and ionic N2 species exhibit a rich spectrum as a result of the large density of couplings between states with different multiplicities. In this sense, spectra of the molecular ion N are investigated combining Fourier transform spectroscopy and ab initio methods. We have reanalyzed the First Negative band System (B X) including five bands not reported previously by Fourier spectroscopy. The spectra were recorded using a resolution of 0.6 cm−1 and accuracy of 0.005 cm−1. These results are then compared with new MRCI+Q/AV6Z calculations. For the first time, transition probabilities are computed for the previously observed 2-A band system. The 2 state ( = 67,029 cm−1) has a dissociation energy of 24,787 cm−1 at = 2.7332 a0. The predicted lifetimes for the 2-A emissions are of the order of 170 ns. The calculated transition probabilities A(=0, =0) for the B-X and 2
{"title":"A new look at N2+ electronic transitions: An experimental and theoretical study","authors":"Laiz R. Ventura, Ramon S. da Silva, Jayr Amorim, Carlos E. Fellows","doi":"10.1016/j.jms.2024.111902","DOIUrl":"10.1016/j.jms.2024.111902","url":null,"abstract":"<div><p>Neutral and ionic N<sub>2</sub> species exhibit a rich spectrum as a result of the large density of couplings between states with different multiplicities. In this sense, spectra of the molecular ion N<span><math><msubsup><mrow></mrow><mrow><mn>2</mn></mrow><mrow><mo>+</mo></mrow></msubsup></math></span> are investigated combining Fourier transform spectroscopy and <em>ab initio</em> methods. We have reanalyzed the First Negative band System (B<span><math><mrow><msup><mrow></mrow><mrow><mn>2</mn></mrow></msup><msubsup><mrow><mi>Σ</mi></mrow><mrow><mi>u</mi></mrow><mrow><mo>+</mo></mrow></msubsup></mrow></math></span> <span><math><mo>→</mo></math></span> X<span><math><mrow><msup><mrow></mrow><mrow><mn>2</mn></mrow></msup><msubsup><mrow><mi>Σ</mi></mrow><mrow><mi>g</mi></mrow><mrow><mo>+</mo></mrow></msubsup></mrow></math></span>) including five bands not reported previously by Fourier spectroscopy. The spectra were recorded using a resolution of 0.6 cm<sup>−1</sup> and accuracy of 0.005 cm<sup>−1</sup>. These results are then compared with new MRCI+Q/AV6Z calculations. For the first time, transition probabilities are computed for the previously observed 2<span><math><mrow><msup><mrow></mrow><mrow><mn>2</mn></mrow></msup><msub><mrow><mi>Π</mi></mrow><mrow><mi>g</mi></mrow></msub></mrow></math></span>-A<span><math><mrow><msup><mrow></mrow><mrow><mn>2</mn></mrow></msup><msub><mrow><mi>Π</mi></mrow><mrow><mi>u</mi></mrow></msub></mrow></math></span> band system. The 2<span><math><mrow><msup><mrow></mrow><mrow><mn>2</mn></mrow></msup><msub><mrow><mi>Π</mi></mrow><mrow><mi>g</mi></mrow></msub></mrow></math></span> state (<span><math><msub><mrow><mi>T</mi></mrow><mrow><mi>e</mi></mrow></msub></math></span> = 67,029 cm<sup>−1</sup>) has a dissociation energy of 24,787 cm<sup>−1</sup> at <span><math><msub><mrow><mi>R</mi></mrow><mrow><mi>e</mi></mrow></msub></math></span> = 2.7332 a<sub>0</sub>. The predicted lifetimes for the 2<span><math><mrow><msup><mrow></mrow><mrow><mn>2</mn></mrow></msup><msub><mrow><mi>Π</mi></mrow><mrow><mi>g</mi></mrow></msub></mrow></math></span>-A<span><math><mrow><msup><mrow></mrow><mrow><mn>2</mn></mrow></msup><msub><mrow><mi>Π</mi></mrow><mrow><mi>u</mi></mrow></msub></mrow></math></span> emissions are of the order of 170 ns. The calculated transition probabilities A(<span><math><msup><mrow><mi>v</mi></mrow><mrow><mo>′</mo></mrow></msup></math></span>=0, <span><math><msup><mrow><mi>v</mi></mrow><mrow><mo>′</mo><mo>′</mo></mrow></msup></math></span>=0) for the B<span><math><mrow><msup><mrow></mrow><mrow><mn>2</mn></mrow></msup><msubsup><mrow><mi>Σ</mi></mrow><mrow><mi>u</mi></mrow><mrow><mo>+</mo></mrow></msubsup></mrow></math></span>-X<span><math><mrow><msup><mrow></mrow><mrow><mn>2</mn></mrow></msup><msubsup><mrow><mi>Σ</mi></mrow><mrow><mi>g</mi></mrow><mrow><mo>+</mo></mrow></msubsup></mrow></math></span> and 2<span><math><mrow><msup><mrow></mrow><mrow><mn>2</mn></mrow></msup><msub><mrow><mi>Π</mi></mrow><mrow><mi>","PeriodicalId":16367,"journal":{"name":"Journal of Molecular Spectroscopy","volume":"401 ","pages":"Article 111902"},"PeriodicalIF":1.4,"publicationDate":"2024-03-01","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"140407162","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":4,"RegionCategory":"物理与天体物理","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}
Pub Date : 2024-03-01DOI: 10.1016/j.jms.2024.111901
Elizabeth R. Guest, Jonathan Tennyson, Sergei N. Yurchenko
Correct pressure broadening is essential for modelling radiative transfer in atmospheres, however data are lacking for the many exotic molecules expected in exoplanetary atmospheres. Here we explore modern machine learning methods to mass produce pressure broadening parameters for a large number of molecules in the ExoMol data base. To this end, state-of-the-art machine learning models are used to fit to existing, empirical air-broadening data from the HITRAN database. A computationally cheap method for large-scale production of pressure broadening parameters is developed, which is shown to be reasonably (69%) accurate for unseen active molecules. This method has been used to augment the previously insufficient ExoMol line broadening diet, providing air-broadening data for all ExoMol molecules, so that the ExoMol database has a full and more accurate treatment of line broadening. Suggestions are made for improved air-broadening parameters for species present in atmospheric databases.
{"title":"Predicting the rotational dependence of line broadening using machine learning","authors":"Elizabeth R. Guest, Jonathan Tennyson, Sergei N. Yurchenko","doi":"10.1016/j.jms.2024.111901","DOIUrl":"https://doi.org/10.1016/j.jms.2024.111901","url":null,"abstract":"<div><p>Correct pressure broadening is essential for modelling radiative transfer in atmospheres, however data are lacking for the many exotic molecules expected in exoplanetary atmospheres. Here we explore modern machine learning methods to mass produce pressure broadening parameters for a large number of molecules in the ExoMol data base. To this end, state-of-the-art machine learning models are used to fit to existing, empirical air-broadening data from the HITRAN database. A computationally cheap method for large-scale production of pressure broadening parameters is developed, which is shown to be reasonably (69%) accurate for unseen active molecules. This method has been used to augment the previously insufficient ExoMol line broadening diet, providing air-broadening data for all ExoMol molecules, so that the ExoMol database has a full and more accurate treatment of line broadening. Suggestions are made for improved air-broadening parameters for species present in atmospheric databases.</p></div>","PeriodicalId":16367,"journal":{"name":"Journal of Molecular Spectroscopy","volume":"401 ","pages":"Article 111901"},"PeriodicalIF":1.4,"publicationDate":"2024-03-01","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"https://www.sciencedirect.com/science/article/pii/S0022285224000286/pdfft?md5=bb9e0d35ca6f02e39044595f28bd089d&pid=1-s2.0-S0022285224000286-main.pdf","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"140180150","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":4,"RegionCategory":"物理与天体物理","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"OA","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}
Pub Date : 2024-03-01DOI: 10.1016/j.jms.2024.111904
P. Bryan Changala , Nadav Genossar-Dan , Joshua H. Baraban , Michael C. McCarthy
Recent advances in circumstellar metal chemistry and laser-coolable molecules have spurred interest in the spectroscopy and electronic properties of alkaline earth metal-bearing polyatomic molecules. We report the microwave rotational spectra of two members of this important chemical family, the linear magnesium-carbon chains MgCH and MgCN, detected with cavity Fourier transform microwave spectroscopy of a laser ablation-electric discharge expansion. The rotation, fine, and hyperfine parameters have been derived from the precise laboratory rest frequencies. These experimental results, combined with a theoretical quantum chemical analysis, confirm the recent identification of MgCH and MgCN in the circumstellar envelope of the evolved carbon-rich star IRC+10216. The spectroscopic data also provide insight into the structural and electronic properties that influence the metal-based optical cycling center in this unique class of laser-coolable polyatomics.
{"title":"Laboratory rotational spectroscopy of the magnesium-carbon chains MgC4H and MgC3N","authors":"P. Bryan Changala , Nadav Genossar-Dan , Joshua H. Baraban , Michael C. McCarthy","doi":"10.1016/j.jms.2024.111904","DOIUrl":"https://doi.org/10.1016/j.jms.2024.111904","url":null,"abstract":"<div><p>Recent advances in circumstellar metal chemistry and laser-coolable molecules have spurred interest in the spectroscopy and electronic properties of alkaline earth metal-bearing polyatomic molecules. We report the microwave rotational spectra of two members of this important chemical family, the linear magnesium-carbon chains MgC<span><math><msub><mrow></mrow><mrow><mn>4</mn></mrow></msub></math></span>H and MgC<span><math><msub><mrow></mrow><mrow><mn>3</mn></mrow></msub></math></span>N, detected with cavity Fourier transform microwave spectroscopy of a laser ablation-electric discharge expansion. The rotation, fine, and hyperfine parameters have been derived from the precise laboratory rest frequencies. These experimental results, combined with a theoretical quantum chemical analysis, confirm the recent identification of MgC<span><math><msub><mrow></mrow><mrow><mn>4</mn></mrow></msub></math></span>H and MgC<span><math><msub><mrow></mrow><mrow><mn>3</mn></mrow></msub></math></span>N in the circumstellar envelope of the evolved carbon-rich star IRC+10216. The spectroscopic data also provide insight into the structural and electronic properties that influence the metal-based optical cycling center in this unique class of laser-coolable polyatomics.</p></div>","PeriodicalId":16367,"journal":{"name":"Journal of Molecular Spectroscopy","volume":"401 ","pages":"Article 111904"},"PeriodicalIF":1.4,"publicationDate":"2024-03-01","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"140604833","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":4,"RegionCategory":"物理与天体物理","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}
Pub Date : 2024-03-01DOI: 10.1016/j.jms.2024.111900
Muhammad Osama Ishtiak , Orfeo Colebatch , Karine Le Bris , Paul J. Godin , Kimberly Strong
Perfluoro-n-propane, perfluorocyclobutane, perfluoro-n-butane, and perfluoro-n-pentane are non-ozone-depleting industrial alternatives to chlorofluorocarbons and hydrochlorofluorocarbons. However, these perfluoroalkanes have significant band strength in the atmospheric window from 800 to 1200 cm−1. Coupled with their millennial-scale atmospheric lifetimes, they can lead to significant long-term global warming. Infrared spectra are required to quantify the climate impacts. This work provides a set of high-temperature infrared absorption cross-sections in the range 298–350 K at 0.1 cm−1 resolution from 515 to 1500 cm−1 for each compound. Our cross-sections generally agree with literature measurements except for perfluoro-n-pentane. We use density functional theory to calculate the absorption cross-sections from 0 to 515 cm−1 using the B3LYP functional and several basis sets. The 6-31G(d,p) basis set provides the best results for linear perfluoroalkanes, while the def2-TZVP basis set provides the best results for cyclic perfluoroalkanes. Using experimental cross-sections, we calculate the radiative efficiency and global warming potential for each compound, utilizing the Pinnock curve from Shine and Myhre (2020) and atmospheric lifetimes from Hodnebrog et al. (2020). These quantities are found to be independent of temperature. The average 100-year global warming potential derived from all cross-sections is 9,610±1,260, 10,800±1,420, 10,100±1,330, and 9,380±1,230 for perfluoro-n-propane, perfluorocyclobutane, perfluoro-n-butane, and perfluoro-n-pentane, respectively. Combining the data in this work with our previous measurements reveals that the global warming potential for perfluoroalkanes with an increasing number of CF bonds depends on the ratio of radiative efficiency to molecular weight.
{"title":"Measurements of infrared absorption cross-sections for n-C3F8, c-C4F8, n-C4F10, and n-C5F12 from 298 to 350 K","authors":"Muhammad Osama Ishtiak , Orfeo Colebatch , Karine Le Bris , Paul J. Godin , Kimberly Strong","doi":"10.1016/j.jms.2024.111900","DOIUrl":"10.1016/j.jms.2024.111900","url":null,"abstract":"<div><p>Perfluoro-n-propane, perfluorocyclobutane, perfluoro-n-butane, and perfluoro-n-pentane are non-ozone-depleting industrial alternatives to chlorofluorocarbons and hydrochlorofluorocarbons. However, these perfluoroalkanes have significant band strength in the atmospheric window from 800 to 1200 cm<sup>−1</sup>. Coupled with their millennial-scale atmospheric lifetimes, they can lead to significant long-term global warming. Infrared spectra are required to quantify the climate impacts. This work provides a set of high-temperature infrared absorption cross-sections in the range 298–350 K at 0.1 cm<sup>−1</sup> resolution from 515 to 1500 cm<sup>−1</sup> for each compound. Our cross-sections generally agree with literature measurements except for perfluoro-n-pentane. We use density functional theory to calculate the absorption cross-sections from 0 to 515 cm<sup>−1</sup> using the B3LYP functional and several basis sets. The 6-31G(d,p) basis set provides the best results for linear perfluoroalkanes, while the def2-TZVP basis set provides the best results for cyclic perfluoroalkanes. Using experimental cross-sections, we calculate the radiative efficiency and global warming potential for each compound, utilizing the Pinnock curve from Shine and Myhre (2020) and atmospheric lifetimes from Hodnebrog et al. (2020). These quantities are found to be independent of temperature. The average 100-year global warming potential derived from all cross-sections is 9,610±1,260, 10,800±1,420, 10,100±1,330, and 9,380±1,230 for perfluoro-n-propane, perfluorocyclobutane, perfluoro-n-butane, and perfluoro-n-pentane, respectively. Combining the data in this work with our previous measurements reveals that the global warming potential for perfluoroalkanes with an increasing number of C<img>F bonds depends on the ratio of radiative efficiency to molecular weight.</p></div>","PeriodicalId":16367,"journal":{"name":"Journal of Molecular Spectroscopy","volume":"401 ","pages":"Article 111900"},"PeriodicalIF":1.4,"publicationDate":"2024-03-01","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"https://www.sciencedirect.com/science/article/pii/S0022285224000274/pdfft?md5=1606f942c2fb317c06570494fb3fba8f&pid=1-s2.0-S0022285224000274-main.pdf","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"140154167","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":4,"RegionCategory":"物理与天体物理","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"OA","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}
We produced aniline cations (–C6H5 NH2+) and their dehydro- (H-loss) cations inside helium droplets by electron ionization and observed their mass-selected vibrational spectra in the NH stretching region. We observed vibrational bands at m/q = 93 which were identified as aniline cations. These bands showed only a few cm−1 shifts from the symmetric and anti-symmetric NH stretching bands for the amino (NH2) group in the gas phase. For the H-loss cation at mass m/q = 92, the agreement of the observed NH band frequency with the result of DFT calculations suggests several candidate species, including a seven-membered ring structure, 4-monodehydro azepinylium (–C6NH6+). A new reaction pathway to this cation was discussed by considering large excess energy in the ionization process.
{"title":"Vibrational spectroscopy of aniline cations and their H-loss cations in helium droplets","authors":"Arisa Iguchi , Amandeep Singh , Susumu Kuma , Hajime Tanuma , Toshiyuki Azuma","doi":"10.1016/j.jms.2024.111903","DOIUrl":"10.1016/j.jms.2024.111903","url":null,"abstract":"<div><p>We produced aniline cations (<span><math><mi>c</mi></math></span>–C<sub>6</sub>H<sub>5</sub> <img>NH<sub>2</sub><sup>+</sup>) and their dehydro- (H-loss) cations inside helium droplets by electron ionization and observed their mass-selected vibrational spectra in the N<img>H stretching region. We observed vibrational bands at <em>m/q</em> = 93 which were identified as aniline cations. These bands showed only a few cm<sup>−1</sup> shifts from the symmetric and anti-symmetric N<img>H stretching bands for the amino (<img>NH<sub>2</sub>) group in the gas phase. For the H-loss cation at mass <em>m/q</em> = 92, the agreement of the observed N<img>H band frequency with the result of DFT calculations suggests several candidate species, including a seven-membered ring structure, 4-monodehydro azepinylium (<span><math><mi>c</mi></math></span>–C<sub>6</sub>NH<sub>6</sub><sup>+</sup>). A new reaction pathway to this cation was discussed by considering large excess energy in the ionization process.</p></div>","PeriodicalId":16367,"journal":{"name":"Journal of Molecular Spectroscopy","volume":"401 ","pages":"Article 111903"},"PeriodicalIF":1.4,"publicationDate":"2024-03-01","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"140398430","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":4,"RegionCategory":"物理与天体物理","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}
Pub Date : 2024-02-01DOI: 10.1016/j.jms.2024.111886
Michael C. McCarthy, P. Bryan Changala, P. Brandon Carroll
The rotational spectra of two new silicon-bearing carbon chains, H2C3Si and HSiCCH have been detected by means of Fourier-transform microwave spectroscopy in a supersonic jet source equipped with an electrical discharge. On the basis of measurements between 10 and 42 GHz, precise spectroscopic constants have been determined for both molecules. Along with H29SiCCH and H30SiCCH, which were detected in natural abundance, several other rare isotopic species of HSiCCH were observed using samples enriched in carbon-13 and D. From this isotopic data, a precise semi-experimental equilibrium structure was derived and compared with a re-evaluated semi-experimental equilibrium structure of the parent silylene SiH2; the deuterium isotopic measurements also provide important clues as to the formation pathway of HSiCCH in our discharge. Because other small Si-bearing chains have been detected in the circumstellar envelope of the evolved carbon star IRC+10216, both chains may be of astronomical interest.
{"title":"Rotational detection of the silicon-carbon chains H2C3Si and HSiCCH","authors":"Michael C. McCarthy, P. Bryan Changala, P. Brandon Carroll","doi":"10.1016/j.jms.2024.111886","DOIUrl":"10.1016/j.jms.2024.111886","url":null,"abstract":"<div><p>The rotational spectra of two new silicon-bearing carbon chains, H<sub>2</sub>C<sub>3</sub>Si and HSiCCH have been detected by means of Fourier-transform microwave spectroscopy in a supersonic jet source equipped with an electrical discharge. On the basis of measurements between 10 and 42<!--> <!-->GHz, precise spectroscopic constants have been determined for both molecules. Along with H<sup>29</sup>SiCCH and H<sup>30</sup>SiCCH, which were detected in natural abundance, several other rare isotopic species of HSiCCH were observed using samples enriched in carbon-13 and D. From this isotopic data, a precise semi-experimental equilibrium structure was derived and compared with a re-evaluated semi-experimental equilibrium structure of the parent silylene SiH<sub>2</sub>; the deuterium isotopic measurements also provide important clues as to the formation pathway of HSiCCH in our discharge. Because other small Si-bearing chains have been detected in the circumstellar envelope of the evolved carbon star IRC+10216, both chains may be of astronomical interest.</p></div>","PeriodicalId":16367,"journal":{"name":"Journal of Molecular Spectroscopy","volume":"400 ","pages":"Article 111886"},"PeriodicalIF":1.4,"publicationDate":"2024-02-01","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"139557719","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":4,"RegionCategory":"物理与天体物理","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}
Pub Date : 2024-02-01DOI: 10.1016/j.jms.2024.111887
Aaron I. Strom , Ibrahim Muddasser , Guntram Rauhut , David T. Anderson
The vibrational dynamics of diborane have been extensively studied both theoretically and experimentally ever since the bridge structure of diborane was established in the 1950s. Numerous infrared and several Raman spectroscopic studies have followed in the ensuing years at ever increasing levels of spectral resolution. In parallel, ab initio computations of the underlying potential energy surface have progressed as well as the methods to calculate the anharmonic vibration dynamics beyond the double harmonic approximation. Nevertheless, even 70 years after the bridge structure of diborane was established, there are still significant discrepancies between experiment and theory for the fundamental vibrational frequencies of diborane. In this work we use parahydrogen (pH2) matrix isolation infrared spectroscopy to characterize six fundamental vibrations of B2H6 and B2D6 and compare them with results from configuration-selective vibrational configuration interaction theory. The calculated frequencies and intensities are in very good agreement with the pH2 matrix isolation spectra, even several combination bands are well reproduced. We believe that the reason discrepancies have existed for so long is related to the large amount of anharmonicity that is associated with the bridge BH stretching modes. However, the calculated frequencies and intensities reported here for the vibrational modes of all three boron isotopologues of B2H6 and B2D6 are within ± 2.00 cm−1 and ± 1.44 cm−1, respectively, of the experimental frequencies and therefore a refined vibrational assignment of diborane has been achieved.
{"title":"Diborane anharmonic vibrational frequencies and Intensities: Experiment and theory","authors":"Aaron I. Strom , Ibrahim Muddasser , Guntram Rauhut , David T. Anderson","doi":"10.1016/j.jms.2024.111887","DOIUrl":"https://doi.org/10.1016/j.jms.2024.111887","url":null,"abstract":"<div><p>The vibrational dynamics of diborane have been extensively studied both theoretically and experimentally ever since the bridge structure of diborane was established in the 1950s. Numerous infrared and several Raman spectroscopic studies have followed in the ensuing years at ever increasing levels of spectral resolution. In parallel, <em>ab initio</em> computations of the underlying potential energy surface have progressed as well as the methods to calculate the anharmonic vibration dynamics beyond the double harmonic approximation. Nevertheless, even 70 years after the bridge structure of diborane was established, there are still significant discrepancies between experiment and theory for the fundamental vibrational frequencies of diborane. In this work we use parahydrogen (pH<sub>2</sub>) matrix isolation infrared spectroscopy to characterize six fundamental vibrations of B<sub>2</sub>H<sub>6</sub> and B<sub>2</sub>D<sub>6</sub> and compare them with results from configuration-selective vibrational configuration interaction theory. The calculated frequencies and intensities are in very good agreement with the pH<sub>2</sub> matrix isolation spectra, even several combination bands are well reproduced. We believe that the reason discrepancies have existed for so long is related to the large amount of anharmonicity that is associated with the bridge BH stretching modes. However, the calculated frequencies and intensities reported here for the vibrational modes of all three boron isotopologues of B<sub>2</sub>H<sub>6</sub> and B<sub>2</sub>D<sub>6</sub> are within ± 2.00 cm<sup>−1</sup> and ± 1.44 cm<sup>−1</sup>, respectively, of the experimental frequencies and therefore a refined vibrational assignment of diborane has been achieved.</p></div>","PeriodicalId":16367,"journal":{"name":"Journal of Molecular Spectroscopy","volume":"400 ","pages":"Article 111887"},"PeriodicalIF":1.4,"publicationDate":"2024-02-01","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"139733136","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":4,"RegionCategory":"物理与天体物理","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}