| タイトル | Branching ratios in the N + CH3 reaction - Formation of the methylene amidogen (H2CN) radical |
| 著者（英） | Stief, L. J.; Marston, G.; Nesbitt, F. L. |
| 著者所属（英） | NASA Goddard Space Flight Center |
| 発行日 | 1989-09-15 |
| 言語 | eng |
| 内容記述 | The discharge-flow mass spectrometer system described by Brunning and Stief (1986) and Nejad et al. (1988) is used to determine the branching ratios for the reaction N + CH3. The results are presented in extensive tables and graphs and characterized in detail, and the implications for HCN formation in the atmosphere of Titan are considered. It is found that the main reaction channel at room temperature is H2CN + H, with about 10 percent giving HCN + H2; no isotope effects are seen when CH3 is replaced with CD3, and the branching ratios appear to be temperature-independent. |
| NASA分類 | ATOMIC AND MOLECULAR PHYSICS |
| レポートNO | 89A53528 |
| 権利 | Copyright |
| URI | https://repository.exst.jaxa.jp/dspace/handle/a-is/361337 |
