Department of Chemistry, University of Basel, Klingelbergstrasse 80, 4056 Basel, Switzerland.
Phys Chem Chem Phys. 2014 Jan 21;16(3):1161-5. doi: 10.1039/c3cp54299h. Epub 2013 Nov 29.
Ultraviolet electronic transitions of the linear carbon chains C6, C7, C8, and C9 were measured in the gas phase by a mass-resolved 1 + 1 resonant two-photon ionization technique using a picosecond laser. Broad absorptions with band maxima at 230.2 and 259.0 nm are identified as N(3)Σ(u)(-) - X(3)Σ(g)(-) (N > 3) transition of C6 and C8, respectively. Based on calculated Franck-Condon intensities, the band maxima are identified as origin bands. An upper limit of 30 ps is determined for the N(3)Σ(u)(-) excited state lifetime of C6. The (1)Σ(u)(+)- X(1)Σ(g)(+) transition with band maximum at 238.5 nm was observed for C7 and at 279.0 nm for C9. The proposition that intramolecular processes in the excited electronic states of carbon chains can lead to broadening as in the diffuse interstellar absorptions is experimentally demonstrated.
采用皮秒激光的质量分辨 1 + 1 共振双光子电离技术,在气相中测量了线性碳链 C6、C7、C8 和 C9 的紫外电子跃迁。在 230.2nm 和 259.0nm 处的宽带吸收峰被确定为 C6 和 C8 的 N(3)Σ(u)(-) - X(3)Σ(g)(-)(N > 3)跃迁。基于计算出的 Franck-Condon 强度,这些带的最大值被确定为起源带。C6 的 N(3)Σ(u)(-)激发态寿命的上限为 30ps。在 238.5nm 处观察到 C7 的(1)Σ(u)(+)- X(1)Σ(g)(+)跃迁,在 279.0nm 处观察到 C9 的跃迁。实验证明,在激发电子态中,分子内过程可能导致类似弥漫星际吸收的展宽。