Szczepaniak Urszula, Kołos Robert, Gronowski Marcin, Chevalier Michèle, Guillemin Jean-Claude, Turowski Michał, Custer Thomas, Crépin Claudine
Institut des Sciences Moléculaires d'Orsay, UMR8214, CNRS Univ. Paris-Sud, Université Paris-Saclay , F-91405 Orsay, France.
Institute of Physical Chemistry, Polish Academy of Sciences, Kasprzaka , 44/52, 01-224 Warsaw, Poland.
J Phys Chem A. 2017 Oct 5;121(39):7374-7384. doi: 10.1021/acs.jpca.7b07849. Epub 2017 Sep 25.
HCN is a molecule of astrochemical interest. In this study, it was produced in cryogenic Ar and Kr matrices from UV-photolyzed diacetylene/cyanodiacetylene mixtures. Its strong phosphorescence was discovered and served for the identification of the compound. Vibrationally resolved phosphorescence excitation spectra gave insight into excited singlet electronic states. Two electronic systems were observed around 26 000-34 000 cm and 35 000-50 000 cm. Energies of the second excited singlet and the lowest triplet state were derived from analysis of these systems. Vibrational and electronic spectroscopic features were assigned with the assistance of density functional theory calculations. Some trends concerning the electronic spectroscopy of HCN family molecules are presented.
HCN是一种具有天体化学研究价值的分子。在本研究中,它是由紫外光解的丁二炔/氰基丁二炔混合物在低温氩气和氪气基质中产生的。发现了其强烈的磷光,并用于该化合物的鉴定。振动分辨的磷光激发光谱深入研究了激发单重态电子态。在26000 - 34000厘米和35000 - 50000厘米附近观察到两个电子体系。通过对这些体系的分析得出了第二激发单重态和最低三重态的能量。借助密度泛函理论计算对振动和电子光谱特征进行了归属。还介绍了一些关于HCN族分子电子光谱的趋势。