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在星际化学丙炔基醚冰中观察到的非晶态向晶态相变引起的红外衰减。

Infrared attenuation due to phase change from amorphous to crystalline observed in astrochemical propargyl ether ices.

机构信息

Physical Research Laboratory, Ahmedabad, India.

Indian Centre for Space Physics, Kolkata, India.

出版信息

Spectrochim Acta A Mol Biomol Spectrosc. 2020 Jan 5;224:117393. doi: 10.1016/j.saa.2019.117393. Epub 2019 Jul 17.

Abstract

Astrochemical ices are known to undergo morphological changes, from amorphous to crystalline, upon warming the ice from lower (10 K) to higher temperatures. Phase changes are mostly identified by the observation of significant changes in the InfraRed (IR) spectrum, where the IR bands that are broad in the amorphous phase are narrower and split when the ice turns crystalline. To-date all the molecules that are studied under astrochemical conditions are observed to follow such a behaviour without significant attenuation in the IR wavelength. However, in this paper we report a new observation when propargyl ether (CHOCH) is warmed from the amorphous phase, at 10 K, through the phase transition temperature of 170 K, the crystalline ice being found to strongly attenuate IR photons at the mid-IR wavelengths.

摘要

天体化学冰在升温时(从 10K 升温到更高温度)已知会经历形态变化,从无定形变为结晶。通过观察红外光谱中的显著变化,主要可以识别相变,其中在无定形相中宽的红外带在冰变成结晶时变窄并分裂。迄今为止,在天体化学条件下研究的所有分子都被观察到表现出这种行为,而在红外波长上没有明显衰减。然而,在本文中,我们报告了当炔丙基醚(CHOCH)从 10K 的无定形相升温通过 170K 的相变温度时的一个新观察结果,发现结晶冰强烈衰减中红外波长的红外光子。

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