福尔马林同素异形体 13CD2NOH 在 280-4000 cm-1 区域的振动波段以及利用傅立叶变换红外光谱对其 ν12 波段进行的振动分析

IF 1.4 4区 物理与天体物理 Q4 PHYSICS, ATOMIC, MOLECULAR & CHEMICAL
A. Jusuf, T.L. Tan
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引用次数: 0

摘要

傅立叶变换红外光谱(FTIR)在 500-4000 cm-1 区域的分辨率较低(0.50 cm-1),在 280-500 cm-1 区域的分辨率较高(0.00096 cm-1)。还测量了它们的相对红外(IR)波段强度。此外,还利用 13CD2NOH 在澳大利亚同步加速器上记录的高分辨率傅立叶变换红外光谱,对其 ν12 波段的红外跃迁进行了滚振分析。共分配了 1077 个 C 型 ν12 波段的红外跃迁,并使用 Ir 表示的 Watson's A 还原哈密顿进行拟合,首次推导出其波段中心和 v12 = 1 状态振荡常数,直至全部 5 个四元离心畸变项,均方根(rms)偏差为 0.00044 cm-1。13CD2NOH 的 ν12 波段中心为 391.054446(36) cm-1。通过拟合从 13CD2NOH ν12 波段分配的红外跃迁中得到的 407 个基态组合差(GSCDs),首次确定了直到全部 5 个四次项的基态振荡常数。GSCD 拟合的均方根偏差为 0.00040 cm-1。此外,为了与实验结果进行比较,我们在两个不同的理论水平(B3LYP 和 MP2,使用 cc-pVTZ 基集)上计算了 13CD2NOH 基态的全部 3 个旋转常数和 5 个四元离心畸变项,以及 v12 = 1 态的 3 个旋转常数。结果发现,13CD2NOH 的基态和 v12 = 1 态的振动常数计算值与实验值非常接近。利用 B3LYP 和 MP2 以及 cc-pVTZ 基集,还计算了 13CD2NOH 在 280-4000 cm-1 区域的 12 个基带的振动非谐波频率及其红外波段强度,并与相应的实验数据进行了比较。最后,计算了 13CD2NOH 顺式构象的基态旋转常数和 ν12 波段的波段中心,并将其与本研究中反式构象的基态旋转常数和 ν12 波段的波段中心进行了比较。
本文章由计算机程序翻译,如有差异,请以英文原文为准。

Vibrational bands of formaldoxime isotopologue 13CD2NOH in the 280–4000 cm−1 region and rovibrational analysis of its ν12 band by Fourier transform infrared (FTIR) spectroscopy

Vibrational bands of formaldoxime isotopologue 13CD2NOH in the 280–4000 cm−1 region and rovibrational analysis of its ν12 band by Fourier transform infrared (FTIR) spectroscopy

Vibrational bands of formaldoxime isotopologue 13CD2NOH in the 280–4000 cm−1 region and rovibrational analysis of its ν12 band by Fourier transform infrared (FTIR) spectroscopy

A total of 11 fundamental and 3 overtone bands of the formaldoxime isotopologue 13CD2NOH were identified using its Fourier transform infrared (FTIR) spectra which were recorded with a low resolution (0.50 cm−1) in the 500–4000 cm−1 region, and high resolution (0.00096 cm−1) in the 280–500 cm−1 region. Their relative infrared (IR) band intensities were also measured. Furthermore, a rovibrational analysis of the IR transitions of the ν12 band of 13CD2NOH was carried out using its high-resolution FTIR spectrum which was recorded at the Australian Synchrotron. A total of 1077 IR transitions of the C-type ν12 band were assigned and fitted using the Watson's A-reduced Hamiltonian in the Ir representation to derive its band center and the v12 = 1 state rovibrational constants up to all 5 quartic centrifugal distortion terms for the first time, with a root-mean-square (rms) deviation of 0.00044 cm−1. The band center of the ν12 band of 13CD2NOH were found to be 391.054446(36) cm−1. The ground state rovibrational constants up to all 5 quartic terms were determined for the first time by fitting 407 ground state combination differences (GSCDs) derived from the assigned IR transitions of the ν12 band of 13CD2NOH of this work. The rms deviation of the GSCD fit was 0.00040 cm−1. Additionally, all 3 rotational constants and 5 quartic centrifugal distortion terms of the ground state and 3 rotational constants of the v12 = 1 state of 13CD2NOH were computed from theoretical anharmonic calculations at two different levels of theory, B3LYP and MP2 with the cc-pVTZ basis set, for comparison with the experimental results. Close agreement was found for the calculated and experimental rovibrational constants of 13CD2NOH for both ground and v12 = 1 states. The vibrational anharmonic frequencies of the 12 fundamental bands of 13CD2NOH in the 280–4000 cm−1 region, and their IR band intensities were also calculated using B3LYP and MP2 with the cc-pVTZ basis set, and they were compared with the respective experimental data. Finally, the ground state rotational constants and the band center of the ν12 band of the cis conformer of 13CD2NOH were calculated and compared with those of the trans conformer of this work.

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来源期刊
CiteScore
2.70
自引率
21.40%
发文量
94
审稿时长
29 days
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.
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