2022
DOI: 10.1039/d2cp01535h
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Ozone production in electron irradiated CO2:O2 ices

Abstract: Various CO2:O2 ices were irradiated using 1 keV electrons at 20 K. The O3 formation efficiency of each ice was quantified and an analysis of its ν3 absorption band was carried out. Our results are applicable to outer Solar System ice astrochemistry.

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Cited by 5 publications
(3 citation statements)
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“…One striking difference is the size of the absorption band due to the asymmetric stretching mode of O 3 located at about 1,041 cm −1 (Chaabouni et al., 2000). In the 20 K spectrum (Figure 2), this band is very intense and is indicative of the efficient formation of O 3 in the irradiated CO 2 ice (Mifsud et al., 2022a, 2022b). In the 70 K spectrum (Figure 3), however, this band is significantly smaller, suggesting an inefficient O 3 formation pathway.…”
Section: Resultsmentioning
confidence: 99%
See 1 more Smart Citation
“…One striking difference is the size of the absorption band due to the asymmetric stretching mode of O 3 located at about 1,041 cm −1 (Chaabouni et al., 2000). In the 20 K spectrum (Figure 2), this band is very intense and is indicative of the efficient formation of O 3 in the irradiated CO 2 ice (Mifsud et al., 2022a, 2022b). In the 70 K spectrum (Figure 3), however, this band is significantly smaller, suggesting an inefficient O 3 formation pathway.…”
Section: Resultsmentioning
confidence: 99%
“…The raw spectroscopic data collected during experimentation is available on the Mendeley Data online repository: https://doi.org/10.17632/zr2mdbk5dt.1 (Mifsud et al., 2022c). Data analysis was performed using the OriginPro 2018 software: https://www.originlab.com/.…”
Section: Data Availability Statementmentioning
confidence: 99%
“…To this end, our research group has been active in characterising the mid-infrared spectra of various molecular ices relevant to astrochemistry, including CO 2 6,7 and O 3 . 8 In this paper, we build upon our previous work and present a thorough and systematic mid-infrared characterisation of pure SO 2 ice deposited at various cryogenic temperatures and thermally annealed to sublimation. The need for more spectroscopic data on sulphur-bearing astrophysical ice analogues was highlighted in a recent review, 9 and is reflective of our comparatively incomplete understanding of sulphur ice astrochemistry, particularly as it relates to solid SO 2 .…”
Section: Introductionmentioning
confidence: 99%