Building formamide and N-substituted formamides from isocyanates on hydrogenated water ices

Context. Many complex organic molecules (COMs) observed in the interstellar medium (ISM) are probably not formed in the gas phase. A large consensus has developed that it could be related to the icy surfaces in this environment. Aims. We investigate the process of building N-substituted formamides in the ISM by successive additions of atomic hydrogen to isocyanates. The key point is to see whether the pre-adsorption of the atomic hydrogen on the ice surface is a driving vector as it is for the formation of CH 3 OH from CO. Methods. We use quantum numerical simulations, namely density functional theory (DFT) and post Hartree–Fock (p-HF) methods derived from coupled-cluster implementations. Several chemical models are presented: the addition of H directly to the isocyanate in the gas phase, the addition of H to the isocyanate pre-adsorbed on ices, the addition of the isocyanate to the hydrogen pre-adsorbed on ices. These ices are successively simulated by a few water molecules up to full bi-layers of them. Results. The formation of formamide (NH 2 CHO) from the isocyanic acid (HNCO) is taken as a case study. Whatever the level of the calculation and the size of the water cluster supporting the adsorbed isocyanate, the addition of the incoming atomic hydrogen reveals no opportunity to eliminate the energy barrier found in the gas phase. By contrast, the formation of H 2 NCHO, as well as CH 3 NHCHO or C 2 H 5 NHCHO, is possible without any barrier on the same ice surfaces, with the express condition that the H atom to be added is already attached to the ice, prior to the attack by the isocyanate species. Conclusions. There is a way for the N-substituted formamides to be easily built by two successive hydrogenations on ices starting from the isocyanates HNCO, CH 3 NCO, and C 2 H 5 NCO. Some of those species are already detected; if not, they appear as strong candidates worth considering for future observation campaigns. Moreover, this suggests that other hydrogenation processes neglected to date, could be considered when similar pre-conditions are satisfied.

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Journal
Astronomy and Astrophysics
Published
2025-03-01
DOI
https://doi.org/10.1051/0004-6361/202450614
Primary Topic
Education, Safety, and Science Studies
Type
article
Field-Weighted Citation Impact
0.00

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article

Building formamide and N-substituted formamides from isocyanates on hydrogenated water ices

F. Pauzat, Y. Ellinger, Jean‐Claude Guillemin, Pilar Redondo et al.
3 links
Astronomy and Astrophysics
Education, Safety, and Science Studies
article

Building formamide and N-substituted formamides from isocyanates on hydrogenated water ices

F. Pauzat, Y. Ellinger, Jean‐Claude Guillemin, Pilar Redondo, Olivier Parisel, N. Tieppo
article en

Abstract

Context. Many complex organic molecules (COMs) observed in the interstellar medium (ISM) are probably not formed in the gas phase. A large consensus has developed that it could be related to the icy surfaces in this environment. Aims. We investigate the process of building N-substituted formamides in the ISM by successive additions of atomic hydrogen to isocyanates. The key point is to see whether the pre-adsorption of the atomic hydrogen on the ice surface is a driving vector as it is for the formation of CH 3 OH from CO. Methods. We use quantum numerical simulations, namely density functional theory (DFT) and post Hartree–Fock (p-HF) methods derived from coupled-cluster implementations. Several chemical models are presented: the addition of H directly to the isocyanate in the gas phase, the addition of H to the isocyanate pre-adsorbed on ices, the addition of the isocyanate to the hydrogen pre-adsorbed on ices. These ices are successively simulated by a few water molecules up to full bi-layers of them. Results. The formation of formamide (NH 2 CHO) from the isocyanic acid (HNCO) is taken as a case study. Whatever the level of the calculation and the size of the water cluster supporting the adsorbed isocyanate, the addition of the incoming atomic hydrogen reveals no opportunity to eliminate the energy barrier found in the gas phase. By contrast, the formation of H 2 NCHO, as well as CH 3 NHCHO or C 2 H 5 NHCHO, is possible without any barrier on the same ice surfaces, with the express condition that the H atom to be added is already attached to the ice, prior to the attack by the isocyanate species. Conclusions. There is a way for the N-substituted formamides to be easily built by two successive hydrogenations on ices starting from the isocyanates HNCO, CH 3 NCO, and C 2 H 5 NCO. Some of those species are already detected; if not, they appear as strong candidates worth considering for future observation campaigns. Moreover, this suggests that other hydrogenation processes neglected to date, could be considered when similar pre-conditions are satisfied.

Astronomy and AstrophysicsVol. 695
Universidad de Valladolid (ES), Centre National de la Recherche Scientifique (FR), Sorbonne Université (FR), Laboratoire de Chimie Théorique (FR), École Nationale Supérieure de Chimie de Rennes (FR), Université de Rennes (FR)
Centre National d’Etudes Spatiales, Centre National de la Recherche Scientifique
Openalex Percentile: Top 96%
Education, Safety, and Science Studies
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