Institute of Physical Chemistry of the Polish Academy of Sciences, Kasprzaka 44, 01-224 Warsaw, Poland.
J Chem Phys. 2010 Aug 21;133(7):074310. doi: 10.1063/1.3472978.
Electronic absorption and emission spectra have been investigated for cyanodiacetylene, HC(5)N, an astrophysically relevant molecule. The analysis of gas-phase absorption was assisted with the parallel rare gas matrix isolation experiments and with density functional theory (DFT) predictions concerning the excited electronic states. Mid-UV systems B (1)Delta<--X (1)Sigma(+) (origin at 282.5 nm) and A (1)Sigma(-)<--X (1)Sigma(+) (306.8 nm) were observed. Vibronic assignments have been facilitated by the discovery of the visible phosphorescence a (3)Sigma(+)<--X (1)Sigma(+) in solid Ar, Kr, and Xe. Phosphorescence excitation spectra, as well as UV absorption measurements in rare gas matrices, revealed the enhancement of A<--X transitions. The vibronic structure of dispersed phosphorescence spectra supplied new data concerning the ground state bending fundamentals of matrix-isolated HC(5)N. The experimental singlet-triplet splitting, 2.92 eV in Ar, closely matches the value of 3.0 eV predicted by DFT.
已研究了与天体物理相关分子氰基二乙炔(HC(5)N)的电子吸收和发射光谱。气相吸收分析得到了平行稀有气体基质隔离实验和关于激发电子态的密度泛函理论(DFT)预测的辅助。观察到了中紫外系统 B(1)Delta<--X(1)Sigma(+)(起源于 282.5nm)和 A(1)Sigma(-)<--X(1)Sigma(+)(306.8nm)。通过在固体 Ar、Kr 和 Xe 中发现可见磷光 a(3)Sigma(+)<--X(1)Sigma(+),促进了振子分配的确定。磷光激发光谱以及稀有气体基质中的 UV 吸收测量揭示了 A<--X 跃迁的增强。分散磷光光谱的振子结构提供了关于基质隔离 HC(5)N 基态弯曲基频的新数据。实验单重态-三重态分裂,在 Ar 中为 2.92eV,与 DFT 预测的 3.0eV 值非常吻合。