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单氘代环氧乙烷(-CHDO)的高分辨率红外光谱以及820至950厘米之间两种基频的分析

High resolution infrared spectroscopy of monodeutero-oxirane (-CHDO) and analysis of two fundamentals between 820 and 950 cm.

作者信息

Albert Sieghard, Chen Ziqiu, Keppler Karen, Wichmann Gunther, Quack Martin, Stohner Jürgen, Schurig Volker, Trapp Oliver

机构信息

Department of Chemistry and Applied Biosciences, ETH Zürich, CH-8093 Zürich, Switzerland.

College of Chemistry and Chemical Engineering, Lanzhou University, Lanzhou 730000, China.

出版信息

Phys Chem Chem Phys. 2025 May 23. doi: 10.1039/d5cp00880h.

Abstract

We report the analysis of the infrared (IR) spectrum of monodeutero-oxirane (-CHCHDO), measured at room temperature at a self-apodized instrumental resolution of 0.0015 cm with the Bruker IFS 125 HR Zürich Prototype spectrometer (ZP 2001), in the range of the ring deformation fundamental centered at 896.025 cm and the wagging fundamental centered at 837.36 cm. A total of more than 1100 transitions were analyzed and fitted with an effective Hamiltonian which represents the data accurately, within 0.001 cm for and 0.004 cm for most transitions of . We also report calculations including parity violation and an extended analysis with a substantial number of further assigned lines in our previously measured pure rotational spectra in the GHz and far infrared range. In combination with ground state combination differences from the IR spectra and further available results, we provide a critical analysis and improved spectroscopic parameters for the vibrational ground state based on more than 3300 assigned rotational transitions. The results are discussed as they pertain to isotopic chirality, molecular parity violation and the astrophysical observation of this isotopomer.

摘要

我们报告了在室温下,使用布鲁克IFS 125 HR苏黎世原型光谱仪(ZP 2001),以0.0015 cm的自变迹仪器分辨率测量的单氘代环氧乙烷(-CHCHDO)的红外(IR)光谱分析,范围为以896.025 cm为中心的环变形基频和以837.36 cm为中心的摇摆基频。总共分析了1100多个跃迁,并使用有效哈密顿量进行拟合,该哈密顿量能准确表示数据,对于 ,在0.001 cm范围内,对于 的大多数跃迁,在0.004 cm范围内。我们还报告了包括宇称破坏的计算,以及对我们之前在GHz和远红外范围内测量的纯转动光谱中大量进一步指定谱线的扩展分析。结合红外光谱的基态组合差异和其他可用结果,我们基于3300多个指定的转动跃迁,对振动基态进行了批判性分析并改进了光谱参数。讨论了这些结果与同位素手性、分子宇称破坏以及该同位素异构体的天体物理观测的关系。

https://cdn.ncbi.nlm.nih.gov/pmc/blobs/5a00/12172156/6aa8260d24af/d5cp00880h-f1.jpg

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