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Quantum tunneling during interstellar surface-catalyzed formation of water: the reaction H + H(2)O(2) → H(2)O + OH
The final step of the water formation network on interstellar grain surfaces starting from the H + O(2) route is the reaction between H and H(2)O(2). This reaction is known to have a high activation energy and therefore at low temperatures it can only proceed via tunneling. To date, however, no rate...
| Autores principales: | , , , |
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| Formato: | Online Artículo Texto |
| Lenguaje: | English |
| Publicado: |
Royal Society of Chemistry
2016
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| Materias: | |
| Acceso en línea: | https://www.ncbi.nlm.nih.gov/pmc/articles/PMC5317215/ https://www.ncbi.nlm.nih.gov/pubmed/27886292 http://dx.doi.org/10.1039/c6cp06457d |