Jiang Pan, Chi Xiaoping, Zhu Qihe, Cheng Min, Gao Hong
Beijing National Laboratory for Molecular Sciences (BNLMS), Institute of Chemistry, Chinese Academy of Sciences, Beijing, 100190, China.
University of Chinese Academy of Sciences, Beijing, 100049, China.
Nat Commun. 2019 Jul 18;10(1):3175. doi: 10.1038/s41467-019-11086-z.
Rare isotope (C, O and O) substitutions can substantially change absorption line positions, oscillator strengths and photodissociation rates of carbon monoxide (CO) in the vacuum ultraviolet (VUV) region, which has been well accounted for in recent photochemical models for understanding the large isotopic fractionation effects that are apparent in carbon and oxygen in the solar system and molecular clouds. Here, we demonstrate a strong isotope effect associated with the VUV photodissociation of CO by measuring the branching ratios of CO and CO in the Rydberg 4p(2), 5p(0) and 5s(0) complex region. The measurements show that the quantum yields of electronically excited C atoms in the photodissociation of CO are dramatically different from those of CO, revealing strong isotope effect. This isotope effect strongly depends on specific quantum states of CO being excited, which implies that such effect must be considered in the photochemical models on a state by state basis.
稀有同位素(碳、氧和氧)取代会显著改变一氧化碳(CO)在真空紫外(VUV)区域的吸收线位置、振子强度和光解离速率,这在最近用于理解太阳系和分子云中碳和氧明显的大同位素分馏效应的光化学模型中已有充分考虑。在此,我们通过测量里德堡4p(2)、5p(0)和5s(0)复合区域中CO和CO的分支比,证明了与CO的VUV光解离相关的强烈同位素效应。测量结果表明,CO光解离中电子激发的C原子的量子产率与CO的量子产率显著不同,揭示了强烈的同位素效应。这种同位素效应强烈依赖于被激发的CO的特定量子态,这意味着在光化学模型中必须逐态考虑这种效应。