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Uncertainties in Galactic Chemical Evolution Models

Galactic chemical evolution models allow to follow in time the contribution of multiple stellar populations on the production of all elements in a galaxy. Here we present the impact of input uncertainties, such as the initial mass function, on chemical evolution predictions.
Project summary
Monte Carlo study of the impact of input uncertainties on numerical predictions with simple galactic chemical evolution models.
About the simulation codes
We used OMEGA (part of NuPyCE) along with a home-made Monte Carlo code.
Link to the published paper