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

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.

Top-down schematic of CPICE with labels in the RAIRS measurement configuration. –astro-ph.GA

Travis J. Hager, Bailey M. Moore, Quentin D. Borengasser, Kyle T. Renshaw, Rachel Johnson, Anudha C. Kanaherarachchi, Bernadette M. Broderick

Subjects: Astrophysics of Galaxies (astro-ph.GA); Instrumentation and Methods for Astrophysics (astro-ph.IM)
Cite as: arXiv:2505.09888 [astro-ph.GA] (or arXiv:2505.09888v1 [astro-ph.GA] for this version)
https://doi.org/10.48550/arXiv.2505.09888
Focus to learn more
Submission history
From: Bernadette Broderick
[v1] Thu, 15 May 2025 01:12:47 UTC (1,211 KB)
https://arxiv.org/abs/2505.09888

Astrobiology, Astrochemistry,