Visible-Light Photoionization of Aromatic Molecules in Water-Ice: Organic Chemistry across the Universe with Less Energy
Antti Lignell, Laura I. Tanalenda-Ossorio, and Murthy S. Gudipati

TL;DR
This study demonstrates that visible light can ionize polycyclic aromatic hydrocarbons in water-ice, revealing new low-energy pathways for organic chemistry in space and planetary environments.
Contribution
First evidence that visible photons can cause ionization of PAHs in water-ice, expanding understanding of astrochemical processes with lower energy requirements.
Findings
Visible photons cause ionization of PAHs in water-ice.
Ionization energy is reduced by 4.4 eV compared to gas phase.
Implications for organic chemistry in space environments.
Abstract
Ionization of gas-phase organic molecules such as polycyclic aromatic hydrocarbons (PAHs) requires vacuum ultraviolet photons at wavelengths shorter than 200 nm (~6-9 eV). We present here for the first time that visible photons - accessible through sunlight - can cause photoionization of trapped PAHs in cryogenic water-ice, accounting for 4.4 eV less ionization energy than in the gas phase. This finding opens up new reaction pathways involving low-energy ionization in many environments where water and organic matter coexist. This include the interstellar medium, molecular clouds, protoplanetary disks, and planetary surfaces and atmospheres (including Earth).
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