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Electronic spectra of the C_(2n+1)H (n=2-4) radicals in the gas phase

机译:气相中C_(2n + 1)H(n = 2-4)自由基的电子光谱

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The visible electronic spectra of the linear l-C_(2n+1)H (n=2-4) radicals have been measured in the gas phase. These have been obtained by means of a mass-selective resonant two-color two-photon ionization technique coupled to a supersonic plasma source. The observed spectra are assigned to the A ~2#DELTA# implied by X ~2#PI#, B ~2(sum)~- implied by X ~2#PI#, and C ~2(sum)~- implied by X ~2#PI# electronic transitions arising from #sigma#->#pi# electron promotion. The assignments are based on ab initio calculations, wavelength dependence of the 0_0~0 transition on size, and isotopic substitution. The lifetime broadening of the bands and effects due to vibronic coupling are associated with the carbon skeleton bending modes. The detection of these carbon chains in the diffuse interstellar medium appears to be more favorable by radio astronomy rather than by electronic spectroscopy.
机译:线性1-C_(2n + 1)H(n = 2-4)自由基的可见电子光谱已在气相中进行了测量。这些是通过与超声等离子体源耦合的质量选择共振双色双光子电离技术获得的。观察到的光谱分配给X〜2#PI#隐含的A〜2#DELTA#,X〜2#PI#隐含的B〜2(sum)〜-和C〜2(sum)〜-隐含由#sigma#->#pi#电子促进产生的X〜2#PI#电子跃迁。分配基于从头算,0_0〜0跃迁的波长与尺寸的相关性以及同位素取代。碳带骨架的弯曲模式与能带的寿命变宽以及由于振动耦合引起的效应有关。通过射电天文学比通过电子光谱学更有利于在星际弥散介质中检测这些碳链。

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