Quantum mechanical simulations of the radical-radical chemistry on icy surfaces
Joan Enrique-Romero, Albert Rimola, Ceccarelli, Piero, Ugliengo, Nadia Balucani, Dimitrios Skouteris

TL;DR
This study uses quantum mechanical simulations to investigate radical reactions on icy surfaces, revealing complexities in interstellar molecule formation and identifying likely products and reaction pathways.
Contribution
It provides detailed quantum chemical insights into radical reactions on ice, challenging simplified assumptions and identifying specific feasible interstellar complex organic molecules.
Findings
Radical--radical reactions can be less straightforward than assumed.
Certain molecules like ethane and methylamine are likely products.
Some expected products, like acetaldehyde, are unlikely on grain surfaces.
Abstract
The formation of the interstellar complex organic molecules (iCOMs) is a hot topic in astrochemistry. One of the main paradigms trying to reproduce the observations postulates that iCOMs are formed on the ice mantles covering the interstellar dust grains as a result of radical--radical coupling reactions. We investigate iCOMs formation on the icy surfaces by means of computational quantum mechanical methods. In particular, we study the coupling and direct hydrogen abstraction reactions involving the CH + X systems (X = NH, CH, HCO, CHO, CHOH) and HCO + Y (Y = HCO, CHO, CHOH), plus the CHOH + CHOH and CHO + CHO systems. We computed the activation energy barriers of these reactions as well as the binding energies of all the studied radicals, by means of density functional theory (DFT) calculations on two ice water models, made of 33 and 18…
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