Istituto Nazionale di Astrofisica-Osservatorio Astrofisico di Catania, Via S. Sofia 78, 95123 Catania, Italy.
Spectrochim Acta A Mol Biomol Spectrosc. 2010 Dec;77(5):998-1004. doi: 10.1016/j.saa.2010.08.037. Epub 2010 Sep 21.
Oleum (fuming sulphuric acid), a well known superacid, was used as medium for the generation of the radical cation of a series of selected PAHs. The resulting radical cation spectra were studied by electronic absorption spectroscopy. Not only common PAHs like naphthalene, anthracene, tetracene, pentacene, perylene, pyrene, benzo[a]pyrene, phenanthrene and picene were studied but also the less common and very large PAHs relevant also for the astrochemical research, like coronene, hexabenzocoronene, quaterrylene, dicoronylene and a coronene oligomer. A correlation between the first ionization potential (IP1) of the PAHs studied and the energy to the so-called A-type band of the radical cations observed in oleum has led to the equation IP1=1.30EA+4.39 (in eV) which permits to estimate the energy of the PAHs radical cation transition (EA) in the VIS-NIR knowing the relative ionization potential or vice versa.
发烟硫酸(fuming sulphuric acid),一种众所周知的超强酸,被用作一系列选定多环芳烃(PAHs)的自由基阳离子生成的介质。通过电子吸收光谱法研究了所得自由基阳离子光谱。研究的不仅包括常见的多环芳烃,如萘、蒽、并四苯、苝、芘、苯并[a]芘、菲和苉,还包括不太常见且非常大的多环芳烃,这些多环芳烃也与天体化学研究有关,如蒄、六苯并蔻、苝四醇、二并苝和一个蒄的低聚物。研究的多环芳烃的第一电离势(IP1)与在发烟硫酸中观察到的自由基阳离子所谓 A 型带的能量之间存在相关性,得出了 IP1=1.30EA+4.39(以 eV 为单位)的方程,该方程允许在 VIS-NIR 中估算 PAHs 自由基阳离子跃迁的能量(EA),已知相对电离势或反之亦然。