Stability of pyruvic acid clusters upon slow electron attachment

Pyruvic acid represents a key molecule in prebiotic chemistry and it has recently been proposed to be synthesized on interstellar ices. In order to probe the stability of pyruvic acid in the interstellar medium with respect to decomposition by slow electrons, we investigate the electron attachment t...

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Veröffentlicht in:Physical chemistry chemical physics : PCCP 2021-02, Vol.23 (7), p.4317-4325
Hauptverfasser: Pysanenko, Andriy, Grygoryeva, Kateryna, Ko išek, Jaroslav, Kumar, Ragesh, Fedor, Juraj, On ák, Milan, Fárník, Michal
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Sprache:eng
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Zusammenfassung:Pyruvic acid represents a key molecule in prebiotic chemistry and it has recently been proposed to be synthesized on interstellar ices. In order to probe the stability of pyruvic acid in the interstellar medium with respect to decomposition by slow electrons, we investigate the electron attachment to its homomolecular and heteromolecular clusters. Using mass spectrometry, we follow the changes in the fragmentation pattern and its dependence on the electron energy for various cluster sizes of pure and microhydrated pyruvic acid. The assignment of fragmentation reaction pathways is supported by ab initio calculations. The fragmentation degree dramatically decreases upon clustering. This decrease is even stronger in the heteromolecular clusters of pyruvic acid with water, where the non-dissociative attachment is by far the strongest channel. In the homomolecular clusters, the dissociative channel leading to dehydrogenation is active over a larger electron energy range than in the isolated molecules. To probe the role of the self-scavenging effects, we explore the excited states of pyruvic acid. This has been done both experimentally, by using electron energy loss spectroscopy, and theoretically, by photochemical calculations. Data on both optically-allowed and forbidden states allow for the explanation of processes emerging upon clustering. Fragmentation of pyruvic acid upon slow electron attachment is investigated in relevance to its formation on ice grains in the interstellar medium.
ISSN:1463-9076
1463-9084
DOI:10.1039/d0cp06464e