Hudson Reggie L, Ferrante Robert F
Astrochemistry Laboratory, NASA Goddard Space Flight Center, Greenbelt, MD 20771, USA.
Chemistry Department, U.S. Naval Academy, Annapolis, MD 21402, USA.
Spectrochim Acta A Mol Biomol Spectrosc. 2020 Jun 5;233:118206. doi: 10.1016/j.saa.2020.118206. Epub 2020 Feb 27.
The infrared (IR) spectrum of dipropargyl ether, (HC≡C-CH)O, has been reinvestigated for the compound's liquid, amorphous, and crystalline forms. The IR baseline changes and bandshape distortions seen in literature spectra have been considerably reduced by a different choice of conditions for preparing the crystalline solid, leading to the discovery of two crystalline phases of the ether. A spectrum of the liquid phase has been recorded and compared to that of the amorphous ether to check for possible procedural artifacts. To facilitate cross-laboratory comparisons, estimates are made for absorption coefficients of three IR peaks of the amorphous solid's spectrum. An interpretation is discussed for changes reported in spectral baselines and bandshapes on warming amorphous dipropargyl ether, and tests and predictions are described. The suggestion that the results from dipropargyl ether warming experiments might pose problems in applying Beer's Law to astronomical observations is addressed.
已针对二炔丙基醚(HC≡C-CH₂)O的液体、非晶态和晶态形式重新研究了其红外(IR)光谱。通过选择不同的条件制备结晶固体,文献光谱中出现的红外基线变化和谱带形状畸变已大幅减少,从而发现了该醚的两个晶相。已记录液相光谱并与非晶态醚的光谱进行比较,以检查是否存在可能的操作假象。为便于跨实验室比较,对非晶态固体光谱中三个红外峰的吸收系数进行了估算。讨论了对非晶态二炔丙基醚升温时光谱基线和谱带形状变化的解释,并描述了相关测试和预测。探讨了二炔丙基醚升温实验结果可能给将比尔定律应用于天文观测带来问题的这一观点。