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On the Formation of Interstellar CH(–) Anions: Exploring Mechanism and Rates for CH(2) Reacting with H(–)
[Image: see text] We present accurate ab initio calculations on the structural properties of a gas-phase reaction of possible interest for Saturn’s outer atmosphere chemistry, in which the CH(2) molecule has been detected. In the present study, that molecule is made to react with the H(–) anion to f...
Guardat en:
| Publicat a: | J Phys Chem A |
|---|---|
| Autors principals: | , , , |
| Format: | Artigo |
| Idioma: | Inglês |
| Publicat: |
American Chemical
Society
2020
|
| Accés en línia: | https://ncbi.nlm.nih.gov/pmc/articles/PMC7322726/ https://ncbi.nlm.nih.gov/pubmed/32463233 https://ncbi.nlm.nih.govhttp://dx.doi.org/10.1021/acs.jpca.0c02412 |
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