The formation of urea in space I. Ion-molecule, neutral-neutral, and radical gas-phase reactions
Flavio Siro Brigiano, Yannick Jeanvoine, Antonio Largo, Riccardo, Spezia

TL;DR
This study investigates potential gas-phase formation pathways of urea in space, focusing on low-energy reactions using quantum chemistry, and identifies a promising ion-molecule reaction that could explain urea's presence in the interstellar medium.
Contribution
It provides the first detailed quantum chemistry analysis of urea formation pathways, highlighting a specific ion-molecule reaction as a plausible low-energy synthesis route.
Findings
Most reactions have high activation energies.
The NH₂OH₂⁺ + formamide reaction has a low activation barrier.
This reaction could also produce isocyanic acid.
Abstract
Many organic molecules have been observed in the interstellar medium thanks to advances in radioastronomy, and very recently the presence of urea was also suggested. While those molecules were observed, it is not clear what the mechanisms responsible to their formation are. In fact, if gas-phase reactions are responsible, they should occur through barrierless mechanisms (or with very low barriers). In the past, mechanisms for the formation of different organic molecules were studied, providing only in a few cases energetic conditions favorable to a synthesis at very low temperature. A particularly intriguing class of such molecules are those containing one N--C--O peptide bond, which could be a building block for the formation of biological molecules. Urea is a particular case because two nitrogen atoms are linked to the C--O moiety. Thus, motivated also by the recent tentative…
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Taxonomy
TopicsMolecular Spectroscopy and Structure · Advanced Chemical Physics Studies · Astrophysics and Star Formation Studies
