Water formation at low temperatures by surface O2 hydrogenation III: Monte Carlo simulation

Water is the most abundant molecule found in interstellar icy mantles. In space it is thought to be efficiently formed on the surfaces of dust grains through successive hydrogenation of O, O 2 and O 3 . The underlying physico-chemical mechanisms have been studied experimentally in the past decade an...

Ausführliche Beschreibung

Bibliographische Detailangaben

Veröffentlicht in:	Physical chemistry chemical physics : PCCP 2013-06, Vol.15 (21), p.8287-832
Hauptverfasser:	Lamberts, Thanja, Cuppen, Herma M, Ioppolo, Sergio, Linnartz, Harold
Format:	Artikel
Sprache:	eng
Schlagworte:	Chemistry Cold Temperature Computer Simulation Exact sciences and technology General and physical chemistry Hydrogen - chemistry Hydrogenation Ice - analysis Models, Chemical Monte Carlo Method Oxygen - chemistry Surface physical chemistry Water - chemistry
Online-Zugang:	Volltext
Tags:	Tag hinzufügen Keine Tags, Fügen Sie den ersten Tag hinzu!