Abstract:Among the ice mixtures that can be found in our Universe, those involving ethylene are poorly studied even though ethylene reportedly exists in the presence of water in several astrochemical domains. Here we report about the chemistry of ethylene and water mixtures in both pressure (0-15 GPa) and temperature (300-370 K) ranges relevant to celestial bodies conditions. The behaviour of the binary mixture has been tracked starting from the ethylene clathrate hydrate and following its evolution through two differe… Show more
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