Hudson Reggie L, Yarnall Yukiko Y, Coleman Falvia M
Astrochemistry Laboratory, NASA Goddard Space Flight Center, Greenbelt, MD 20771, USA.
Astrochemistry Laboratory, NASA Goddard Space Flight Center, Greenbelt, MD 20771, USA; NASA Postdoctoral Program, Universities Space Research Association, Columbia, MD 21046, USA.
Spectrochim Acta A Mol Biomol Spectrosc. 2020 Jun 5;233:118217. doi: 10.1016/j.saa.2020.118217. Epub 2020 Mar 3.
Laboratory astrochemists have generated infrared (IR) data for nearly all common classes of organic compounds, but ethers in the solid phase continue to be neglected despite detections of ethers in the interstellar medium by radio astronomers and uncertainty in how extraterrestrial ethers are formed. To address this paucity of data, here we present new mid-IR spectra of amorphous and crystalline dimethyl ether, (CH)O, the simplest member of its class. Spectral positions are tabulated and compared to previous results, but more importantly we also report IR band strengths and absorption coefficients, which we have not found in the literature and on which quantitative IR studies depend. Optical constants of amorphous and crystalline dimethyl ether also have been calculated. Some applications are described.
实验室天体化学家已经生成了几乎所有常见有机化合物类别的红外(IR)数据,但尽管射电天文学家在星际介质中检测到了醚,且外星醚的形成方式存在不确定性,但固相中的醚仍一直被忽视。为了解决这一数据匮乏问题,我们在此展示了最简单的醚类成员——无定形和结晶态二甲醚((CH₃)₂O)的新中红外光谱。我们列出了光谱位置并与先前结果进行比较,但更重要的是,我们还报告了红外波段强度和吸收系数,这些在文献中尚未发现,而定量红外研究却依赖于此。我们还计算了无定形和结晶态二甲醚的光学常数。文中描述了一些应用。