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The tunneling splittings of the ground state and some excited vibrational states for the inversion motion in H3C− anion and H3Si radical H3C- 阴离子和 H3Si 自由基中反转运动的基态和一些激发振动态的隧道分裂
IF 1.4 4区 物理与天体物理 Q3 Physics and Astronomy Pub Date : 2024-04-21 DOI: 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。
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引用次数: 0
The C1Πu state of potassium dimer revisited: An extensive study by polarisation labelling spectroscopy method 二聚酸钾的 C1Πu 状态再研究:极化标记光谱法的广泛研究
IF 1.4 4区 物理与天体物理 Q3 Physics and Astronomy Pub Date : 2024-04-18 DOI: 10.1016/j.jms.2024.111905
Wlodzimierz Jastrzebski , Jacek Szczepkowski , Pawel Kowalczyk

The polarisation labelling spectroscopy technique was applied to study the C1Πu X1Σg+ 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 C1Πu state with 0v38 and 18J101 and the potential energy curve of the state was constructed.

应用偏振标记光谱技术研究了二聚酸钾中的 C1Πu ← X1Σg+ 波段系统。在 22100-24100 cm-1 光谱范围内测量到了约 1100 条新的旋转分辨分子线。对 C 态最低振动级的扰动进行了定位并讨论了其起源。推导出了一组邓纳姆系数,用于拟合 C1Πu 态 0≤v≤38 和 18≤J≤101 的未扰动水平,并构建了该态的势能曲线。
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引用次数: 0
Spectroscopic observation and ab initio calculations of a new isomer of the CS2 trimer CS2 三聚体新异构体的光谱观测和 ab initio 计算
IF 1.4 4区 物理与天体物理 Q3 Physics and Astronomy Pub Date : 2024-03-01 DOI: 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.

我们报告了利用可调谐激光源和脉冲超音速狭缝喷射器在 CS2 的 ν3 基本波段(6.5 μm)和 ν1 + ν3 组合波段(4.5 μm)区域观测到的 (CS2)3 新异构体的光谱观测和理论计算结果。之前观测到的 CS2 三聚体具有桶状结构,有三个等效单体,对称性为 D3。新的异构体由等效 CS2 单体交错平行的 "二聚体对 "组成,第三个 CS2 单体位于 "顶部",与已知的非环状 CO2 三聚体类似。这种结构具有 C2 旋转对称性,与三聚体的 b 惯性轴相对应,这一点已被观察到的核自旋统计所证实。Ab initio 计算正确给出了观察到的两种异构体结构,并表明它们的结合能非常接近。
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引用次数: 0
A new look at N2+ electronic transitions: An experimental and theoretical study N2+ 电子跃迁新面貌:实验和理论
IF 1.4 4区 物理与天体物理 Q3 Physics and Astronomy Pub Date : 2024-03-01 DOI: 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 N2+ are investigated combining Fourier transform spectroscopy and ab initio methods. We have reanalyzed the First Negative band System (B2Σu+ X2Σg+) 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 22Πg-A2Πu band system. The 22Πg state (Te = 67,029 cm−1) has a dissociation energy of 24,787 cm−1 at Re = 2.7332 a0. The predicted lifetimes for the 22Πg-A2Πu emissions are of the order of 170 ns. The calculated transition probabilities A(v=0, v=0) for the B2Σu+-X2Σg+ and 22Π
由于不同倍率状态之间的耦合密度很大,中性和离子 N2 物种表现出丰富的光谱。在这个意义上,我们结合傅立叶变换光谱学和 ab initio 方法研究了分子离子 N2+ 的光谱。我们重新分析了第一负带系统(B2Σu+ → X2Σg+),包括以前未通过傅立叶光谱法报告的五个带。光谱记录的分辨率为 0.6 cm-1,精度为 0.005 cm-1。然后将这些结果与新的 MRCI+Q/AV6Z 计算结果进行比较。首次计算出了之前观测到的 22Πg-A2Πu 波段系统的过渡概率。22Πg 态(Te = 67,029 cm-1)在 Re = 2.7332 a0 时的解离能为 24,787 cm-1。22Πg-A2Πu 发射的预测寿命约为 170 ns。计算得出的 B2Σu+-X2Σg+ 和 22Πg-A2Πu 波段的转变概率 A(v′=0,v′′=0)分别为 1.156 × 107 和 1.716 × 103 s-1。讨论了自旋轨道(SO)矩阵元素在 N2+ 光谱数据中的作用,包括 SO 常数与 A2Πu 态振动水平函数的关系。我们的 SO 理论常数 A0(A2Πu) = -73.40 cm-1 很好地再现了实验值(-74.67 cm-1)。SO 计算还用于研究 N2+ 的自旋禁止跃迁。得到的 <A2Πu|HˆSO|a4Σu+>≈ 30 cm-1。根据自旋态总和(SOS)方法,X2Σg+ 和 B2Σu+ 态的自旋旋转常数γ0 的最佳估计值分别为 0.0096 和 0.0211 cm-1,与目前的实验数据 0.00917(36)和 0.0206(9)定量一致。
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引用次数: 0
Predicting the rotational dependence of line broadening using machine learning 利用机器学习预测线增宽的旋转依赖性
IF 1.4 4区 物理与天体物理 Q3 Physics and Astronomy Pub Date : 2024-03-01 DOI: 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.

正确的压力展宽对于大气中的辐射传递建模至关重要,然而,对于系外行星大气中的许多外来分子,却缺乏相关数据。在此,我们探索了现代机器学习方法,以大量生成 ExoMol 数据库中大量分子的压力展宽参数。为此,我们使用了最先进的机器学习模型来拟合来自 HITRAN 数据库的现有经验空气展宽数据。开发出了一种计算成本低廉的大规模生成压力展宽参数的方法,该方法对于未见过的活性分子具有相当高的准确度(69%)。这种方法被用来扩充以前不足的 ExoMol 线展宽数据,为所有 ExoMol 分子提供空气展宽数据,从而使 ExoMol 数据库对线展宽进行了全面和更准确的处理。建议改进大气数据库中存在的物种的空气展宽参数。
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引用次数: 0
Laboratory rotational spectroscopy of the magnesium-carbon chains MgC4H and MgC3N 镁碳链 MgC4H 和 MgC3N 的实验室旋转光谱分析
IF 1.4 4区 物理与天体物理 Q3 Physics and Astronomy Pub Date : 2024-03-01 DOI: 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 MgC4H and MgC3N, 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 MgC4H and MgC3N 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.

最近在星周金属化学和激光可冷却分子方面取得的进展激发了人们对含碱土金属多原子分子的光谱学和电子特性的兴趣。我们报告了这一重要化学家族的两个成员--线性镁碳链 MgC4H 和 MgC3N 的微波旋转光谱。旋转参数、精细参数和超细参数都是根据精确的实验室静止频率推导出来的。这些实验结果与理论量子化学分析相结合,证实了最近在富碳演化星 IRC+10216 的星周包层中发现的 MgC4H 和 MgC3N。光谱数据还让我们深入了解了影响这一类独特的激光可冷却多面体中金属基光学循环中心的结构和电子特性。
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引用次数: 0
Measurements of infrared absorption cross-sections for n-C3F8, c-C4F8, n-C4F10, and n-C5F12 from 298 to 350 K 正-C3F8、正-C4F8、正-C4F10 和正-C5F12 在 298 至 350 K 之间的红外吸收截面测量结果
IF 1.4 4区 物理与天体物理 Q3 Physics and Astronomy Pub Date : 2024-03-01 DOI: 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.

全氟正丙烷、全氟环丁烷、全氟正丁烷和全氟正戊烷是氯氟化碳和氯氟烃的非臭氧消耗工业替代品。然而,这些全氟烷烃在 800 至 1200 厘米的大气窗口中具有显著的带强度。再加上它们在大气中的千年寿命,它们会导致全球长期显著变暖。需要红外光谱来量化对气候的影响。这项研究为每种化合物提供了一组 298-350 K 范围内的高温红外吸收截面,分辨率为 0.1 厘米(从 515 厘米到 1500 厘米)。除全氟正戊烷外,我们的横截面与文献测量结果基本吻合。我们利用密度泛函理论,使用 B3LYP 函数和多个基集计算了 0 至 515 厘米的吸收截面。6-31G(d,p) 基集为线性全氟烷烃提供了最佳结果,而 def2-TZVP 基集则为环状全氟烷烃提供了最佳结果。通过实验截面,我们利用 Shine 和 Myhre(2020 年)的平诺克曲线以及 Hodnebrog 等人(2020 年)的大气寿命计算出了每种化合物的辐射效率和全球变暖潜势。研究发现,这些数值与温度无关。从所有横截面得出的全氟正丙烷、全氟环丁烷、全氟正丁烷和全氟正戊烷的 100 年平均全球升温潜能值分别为 9,610 ± 1,260 、10,800 ± 1,420 、10,100 ± 1,330 和 9,380 ± 1,230 。将这项工作中的数据与我们之前的测量结果相结合,可以发现 CF 键数量不断增加的全氟烷烃的全球变暖潜势取决于辐射效率与分子量之比。
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引用次数: 0
Vibrational spectroscopy of aniline cations and their H-loss cations in helium droplets 氦液滴中苯胺阳离子及其氢损阳离子的振动光谱学
IF 1.4 4区 物理与天体物理 Q3 Physics and Astronomy Pub Date : 2024-03-01 DOI: 10.1016/j.jms.2024.111903
Arisa Iguchi , Amandeep Singh , Susumu Kuma , Hajime Tanuma , Toshiyuki Azuma

We produced aniline cations (c–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 (c–C6NH6+). A new reaction pathway to this cation was discussed by considering large excess energy in the ionization process.

我们在氦液滴内通过电子电离产生了苯胺阳离子(c-C6H5 NH2+)及其脱氢(H-loss)阳离子,并观察了它们在 NH 伸缩区域的质量选择振动光谱。我们观察到了 m/q = 93 处的振动带,这些振动带被确定为苯胺阳离子。这些频带与气相中氨基(NH2)基的对称和反对称 NH 伸缩频带相比,仅有几 cm-1 的偏移。对于质量为 m/q = 92 的氢损阳离子,观测到的 NH 带频率与 DFT 计算结果一致,这表明存在几种候选物种,其中包括一种七元环结构,即 4-monodehydro azepinylium (c-C6NH6+)。通过考虑电离过程中的大过剩能量,讨论了这种阳离子的新反应途径。
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引用次数: 0
Rotational detection of the silicon-carbon chains H2C3Si and HSiCCH 硅碳链 H2C3Si 和 HSiCCH 的旋转探测
IF 1.4 4区 物理与天体物理 Q3 Physics and Astronomy Pub Date : 2024-02-01 DOI: 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.

在配备有放电装置的超音速喷射源中,通过傅立叶变换微波光谱法探测到了两种新型含硅碳链 H2C3Si 和 HSiCCH 的旋转光谱。根据 10 至 42 GHz 的测量结果,确定了这两种分子的精确光谱常数。除了检测到自然丰度的 H29SiCCH 和 H30SiCCH 外,还利用富含碳-13 和氘的样品观测到了 HSiCCH 的其他几种稀有同位素种类。根据这些同位素数据,得出了精确的半实验平衡结构,并将其与母体硅烯 SiH2 的重新评估半实验平衡结构进行了比较;氘同位素测量结果还为我们放电中 HSiCCH 的形成途径提供了重要线索。由于在演化碳星 IRC+10216 的星周包层中也探测到了其他小型含硅链,这两种链可能都具有天文意义。
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引用次数: 0
Diborane anharmonic vibrational frequencies and Intensities: Experiment and theory 二硼烷非谐振动频率和强度:实验与理论
IF 1.4 4区 物理与天体物理 Q3 Physics and Astronomy Pub Date : 2024-02-01 DOI: 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.

自 20 世纪 50 年代确定二硼烷的桥式结构以来,人们对其振动动力学进行了广泛的理论和实验研究。在随后的几年里,人们又以越来越高的光谱分辨率进行了大量的红外光谱研究和一些拉曼光谱研究。与此同时,底层势能面的非初始计算以及双谐波近似之外的非谐波振动动力学计算方法也取得了进展。然而,即使在二硼烷的桥式结构确定 70 年后,实验与理论在二硼烷的基本振动频率方面仍存在显著差异。在这项工作中,我们使用对氢 (pH2) 基质隔离红外光谱法表征了 B2H6 和 B2D6 的六次基振,并将其与构型选择性振动构型相互作用理论的结果进行了比较。计算出的频率和强度与 pH2 基质分离光谱非常吻合,甚至几个组合带也得到了很好的再现。我们认为,长期存在差异的原因与桥 BH 拉伸模式的大量非谐波有关。不过,本文报告的 B2H6 和 B2D6 所有三种硼同素异形体的振动模式的计算频率和强度分别在实验频率的 ± 2.00 cm-1 和 ± 1.44 cm-1 范围内,因此二硼烷的振动赋值已经得到完善。
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Journal of Molecular Spectroscopy
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