The Formation of Urea in Space
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 observation of urea, we have considered the synthetic pathways responsible to its formation.
We have studied the possibility of forming urea in the gas phase via different kinds of bi-molecular reactions: ion-molecule, neutral, and radical. In particular we have focused on the activation energy of these reactions in order to find possible reactants that could be responsible for to barrierless (or very low energy) pathways.
We have used very accurate, highly correlated quantum chemistry calculations to locate and characterize the reaction pathways in terms of minima and transition states connecting reactants to products.
Most of the reactions considered have an activation energy that is too high; but the ion-molecule reaction between NH2OH+2 and formamide is not too high. These reactants could be responsible not only for the formation of urea but also of isocyanic acid, which is an organic molecule also observed in the interstellar medium.
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
(Submitted on 9 Nov 2017)
Comments: 9 pages + 8 pages of appendix
Subjects: Astrophysics of Galaxies (astro-ph.GA); Chemical Physics (physics.chem-ph)
MSC classes: 85-08
Cite as: arXiv:1711.03457 [astro-ph.GA] (or arXiv:1711.03457v1 [astro-ph.GA] for this version)
Submission history
From: Riccardo Spezia
[v1] Thu, 9 Nov 2017 16:24:10 GMT (4323kb,D)
https://arxiv.org/abs/1711.03457
Astrochemistry
Astrobiology
