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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...

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Detalles Bibliográficos
Autores principales:	Lamberts, Thanja, Samanta, Pradipta Kumar, Köhn, Andreas, Kästner, Johannes
Formato:	Online Artículo Texto
Lenguaje:	English
Publicado:	Royal Society of Chemistry 2016
Materias:	Chemistry
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

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