VUV Processing of Nitrile Ice: Direct Comparison of Branching in Ice and TPD Spectra

TL;DR

This study combines infrared and rotational spectroscopy to compare the chemical branching of VUV-irradiated nitrile ices in both ice and gas phases, providing insights relevant to astrochemical observations.

Contribution

It introduces a combined spectroscopic approach to directly compare ice and gas phase chemical branching in irradiated nitrile ices, enhancing understanding of astrochemical processes.

Findings

Quantified nitrile ice photoproduct abundances.

Detected gas-phase isocyanides and HCN.

Proposed IR band strength correction for isocyanides.

Abstract

The interplay between radiation chemistry and sublimation dynamics of condensed organic compounds on cold grains is fundamental to describe observed gas-phase and ice-phase molecular abundances in the ISM. Infrared measurements are generally used to identify molecules synthesized in irradiated ices in lab experiments, while mass spectrometric techniques have been used to monitor the products following temperature programmed desorption. The IR measurements are often used quantitatively to monitor chemical transformation of ices during the course of irradiation, but the gas phase methods applied with TPD generally do not permit quantitative branching determination. Here we combine reflection-absorption infrared spectroscopy (RAIRS) of ices with broadband rotational spectroscopy of the sublimed products, to study the branching of photoproducts produced by the VUV irradiation of condensed CH3CN and CH3CH2CN ices. This permits direct comparison between the ice-phase and gas-phase branching following temperature programmed desorption. This comparison is analogous to astronomical observations of ices in protostellar disks such as by the James Webb Space Telescope employed in conjunction with ALMA observations in the corresponding warm-up regions of the same objects. In the condensed CH3CN VUV processed ices we quantified the HCN, CH3NC, CH2CCNH, CH3NH2, and CH4 abundances. The CH3CH2CN ices also readily produced the corresponding isocyanide and HCN in addition to a significant yield of CH2CHCN. The ethyl cyanide ice produced CH3CHNH rather than CH3NH2 and no CH4 formation was observed. In the gas phase we detected the isocyanides, HCN and vinyl cyanide. The ice and gas phase relative abundances could be brought into agreement if the unknown IR band strength of the isocyanides C-N stretch is assumed to be ~3 times larger than that of the cyanides.