Abstract
The vibrational energy distributions of HF and CO formed in the O(3P) + CF3C2H reaction have been measured by means of HF laser emission and CO laser resonance absorption methods. CO was found to be vibrationally excited to υ = 3 with a Boltzmann vibrational temperature of 2200 K. The observed CO distribution is consistent with those predicted by different statistical models, indicating the presence of a long-lived reaction intermediate (CF3CH=CO). The observed HF distribution (N1/N0 = 0.38 ± 0.06), however, was found to be twice as much as that predicted by these models, presumably due to the presence of other more exothermic secondary reactions, such as CF3CH + O and NO2, the photochemical source of the O atom.
| Original language | English |
|---|---|
| Pages (from-to) | 121-124 |
| Number of pages | 4 |
| Journal | Journal of physical chemistry |
| Volume | 82 |
| Issue number | 1 |
| DOIs | |
| State | Published - 1978 |
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