Methyl Isocyanate Formation from Oxygen Insertion in Methyl Cyanide Ices
Michelle R. Brann, Karin I. \"Oberg, Mahesh Rajappan

TL;DR
This study shows that oxygen atoms generated by UV photolysis can rapidly insert into methyl cyanide ices at cold temperatures, producing methyl isocyanate and other compounds, revealing a new pathway for chemical complexity in space.
Contribution
It demonstrates that oxygen atom insertion into methyl cyanide occurs efficiently at low temperatures, providing a novel mechanism for complex molecule formation in cold interstellar ices.
Findings
Oxygen atoms rapidly insert into methyl cyanide to produce methyl isocyanate.
The reaction occurs efficiently between 10 K and 40 K with no temperature dependence.
Formation of methyl isocyanate remains robust in different ice matrices, with some variation in yield.
Abstract
In cold molecular clouds, UV photolysis of icy grain mantles generates radicals that lead to new molecule formation. When radical diffusion is limited by low temperatures, oxygen atom addition and insertion reactions, enabled by photolysis of common ice components such as HO, CO, CO, and O, offer an alternative route to chemical complexity through the production of metastable, highly reactive O() atoms. We examine the reactivity of these oxygen atoms generated by UV photolysis of O with methyl cyanide (CHCN). These studies are conducted in an ultrahigh vacuum chamber at cryogenic and low-pressure conditions equipped with in situ infrared spectroscopy to monitor destruction and product formation in real time. We conclude that oxygen atoms rapidly insert into CHCN to produce primarily methyl isocyanate (CHNCO) in matrix free ices. Over the range from 10…
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