多环芳烃的计算红外光谱:从早期到现在的状况

F. Pauzat
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引用次数: 3

摘要

在星际多环芳烃的漫长历史中,计算在实验和观测中一直扮演着重要的角色。从80年代末第一次计算小多环芳烃的红外光谱到最近的计算,与多环芳烃假说相关的研究的每一个方面都发生了巨大的变化:考虑的分子的大小和种类,使用的技术,天文观测的精度……最初的场景已经完全改变了,尽管探索仍然是一样的,那就是将ISM(星际介质)中普遍存在的所谓UIR波段光谱与化学分子家族——多环芳烃(PAHs)联系起来。本文将对这一探索的25年进行历史回顾,重点介绍计算部分。
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Computational IR Spectroscopy for PAHs: From the Early Years to the Present Status
In the long story of interstellar PAHs, computations have played and are still playing a fundamental role in connection with ex- periments and observations. From the very first calculations of the IR spectra of small PAHs in the late eighties to the more recent ones, ev- ery aspect of the research linked to the PAH hypothesis has evolved dramatically: the size and the variety of the molecules considered, the techniques used, the precision of the astronomical observations ...The initial landscape has completely changed though the quest is still the same, that is to correlate the so-called UIR bands spectra ubiquitous in the ISM (Inter Stellar Medium) with a chemical family of molecules, the PAHs. An historical review of the 25 years of this quest is presented here, focusing on the computational part.
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