Classifying metal-poor stars with machine learning using nucleosynthesis calculations
Nicole Vassh, Yilin Wang, Richard M. Woloshyn, Michelle P. Kuchera, Maude Lariviere, Kayle Majic, Benoit Cote

TL;DR
This paper demonstrates that machine learning can effectively classify metal-poor stars' nucleosynthesis origins by training on theoretical calculations, achieving 87% accuracy in distinguishing between $s$ and $r$ process signatures and offering insights for observational follow-up.
Contribution
The study introduces a novel application of machine learning trained on nucleosynthesis simulations to classify metal-poor stars' enrichment processes, highlighting its potential and challenges.
Findings
ML classifies $s$ vs. $r$ process stars with 87% accuracy.
ML suggests reclassification of some $i$ process stars.
Method identifies stars needing further observational data.
Abstract
We apply the capabilities of machine learning (ML) to discern patterns in order to classify metal-poor stars. To do so, we train an ML model on a bank of nucleosynthesis calculations derived from hydrodynamic simulations for events such as neutron star mergers where the rapid () neutron capture process can take place. Likewise we consider a bank of calculations from simulations of the slow () neutron capture process and also consider a few calculations for the intermediate () neutron capture process. We demonstrate that the ML does well overall in recognizing the process from the process, and after training on theoretical calculations ML stellar assignments match conventional labels 87% of the time. We highlight that this method then points to stars that could benefit from additional observational measurements. We also demonstrate that the ML assigns some of the…
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Taxonomy
TopicsAstronomy and Astrophysical Research · Stellar, planetary, and galactic studies · Gamma-ray bursts and supernovae
