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A statistical and machine learning approach to the study of astrochemistry

Heyl, Johannes; Viti, Serena; Vermariën, Gijs; (2023) A statistical and machine learning approach to the study of astrochemistry. Faraday Discussions , 245 pp. 569-585. 10.1039/d3fd00008g. Green open access

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Abstract

In order to obtain a good understanding of astrochemistry, it is crucial to better understand the key parameters that govern grain-surface chemistry. For many chemical networks, these crucial parameters are the binding energies of the species. However, there exists much disagreement regarding these values in the literature. In this work, a Bayesian inference approach is taken to estimate these values. It is found that this is difficult to do in the absence of enough data. The Massive Optimised Parameter Estimation and Data (MOPED) compression algorithm is then used to help determine which species should be prioritised for future detections in order to better constrain the values of binding energies. Finally, an interpretable machine learning approach is taken in order to better understand the non-linear relationship between binding energies and the final abundances of specific species of interest.

Type: Article
Title: A statistical and machine learning approach to the study of astrochemistry
Location: England
Open access status: An open access version is available from UCL Discovery
DOI: 10.1039/d3fd00008g
Publisher version: https://doi.org/10.1039/D3FD00008G
Language: English
Additional information: This version is the author accepted manuscript. For information on re-use, please refer to the publisher's terms and conditions.
UCL classification: UCL
UCL > Provost and Vice Provost Offices > UCL BEAMS
UCL > Provost and Vice Provost Offices > UCL BEAMS > Faculty of Maths and Physical Sciences
UCL > Provost and Vice Provost Offices > UCL BEAMS > Faculty of Maths and Physical Sciences > Dept of Physics and Astronomy
URI: https://discovery-pp.ucl.ac.uk/id/eprint/10172206
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