The thermal reactivity of HCN and NH3 in interstellar ice analogues
J. A. Noble, P. Theule, F. Borget, G. Danger, M. Chomat, F. Duvernay,, F. Mispelaer, and T. Chiavassa

TL;DR
This study investigates the thermal reaction between ammonia and hydrogen cyanide in interstellar ice analogues, revealing its kinetics, product properties, and implications for astrochemical processes.
Contribution
It provides the first detailed kinetic and spectroscopic characterization of the NH3 + HCN to NH4+CN- reaction in interstellar ice analogues, emphasizing its astrochemical significance.
Findings
Reaction occurs at low temperatures without non-thermal processing.
Reaction rate constant depends on temperature and reactant abundance.
NH4+CN- exhibits multilayer desorption kinetics.
Abstract
HCN is a molecule central to interstellar chemistry, since it is the simplest molecule containing a carbon-nitrogen bond and its solid state chemistry is rich. The aim of this work was to study the NH3 + HCN -> NH4+CN- thermal reaction in interstellar ice analogues. Laboratory experiments based on Fourier transform infrared spectroscopy and mass spectrometry were performed to characterise the NH4+CN- reaction product and its formation kinetics. This reaction is purely thermal and can occur at low temperatures in interstellar ices without requiring non-thermal processing by photons, electrons or cosmic rays. The reaction rate constant has a temperature dependence of k(T) = 0.016+0.010-0.006 s-1.exp((-2.7+-0.4 kJmol-1)/(RT)) when NH3 is much more abundant than HCN. When both reactants are diluted in water ice, the reaction is slowed down. We have estimated the CN- ion band strength to be…
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