Formation of HNC and HCN isomers in molecular plasmas revealed by frequency comb and quantum cascade laser spectroscopy
Ibrahim Sadiek, Simona Di Bernardo, Uwe Macherius, Jean-Pierre H. van Helden

TL;DR
This study detects and quantifies HNC and HCN isomers in low-temperature plasmas, revealing significant kinetic differences from interstellar environments and highlighting HNC's role in plasma chemistry.
Contribution
First direct detection and quantification of HNC in molecular plasmas using advanced laser spectroscopy techniques, with insights into their formation mechanisms.
Findings
HNC/[HCN] ratio in plasmas is about 10^-4, much lower than in interstellar media.
Different formation and destruction kinetics of HNC and HCN in plasmas versus space environments.
HNC plays an overlooked role in plasma chemistry involving carbon, nitrogen, and hydrogen.
Abstract
Hydrogen cyanide (HCN) is a well-known product in combustion, astrophysical, and plasma environments, but its isomer, hydrogen isocyanide (HNC), remains unexplored in molecular plasmas. Here, we report on the detection and quantification of both HNC and HCN isomers in low-temperature plasmas generated from N/H/CH mixtures using quantum cascade laser and frequency comb absorption spectroscopy. The identification of HNC is confirmed by comparison with molecular spectroscopic databases. The observed [HNC]/[HCN] abundance ratio of is far lower than reported values in interstellar media, where ratios can reach unity. We attribute this stark difference to fundamentally different kinetics, dominated by an interplay between formation of vibrationally 'hot' intermediates (HCN* and HNC*) and their subsequent stabilization and destruction. This mechanism contrasts with…
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