Chemical evolution library for galaxy formation simulation
Takayuki R.Saitoh

TL;DR
The paper introduces CELib, a comprehensive software library for simulating chemical evolution in galaxy formation, enabling flexible model selection and easy comparison of different chemical evolution scenarios.
Contribution
It provides a modular, ready-to-use library for chemical evolution simulations under the SSP approximation, compatible with various galaxy formation models.
Findings
Demonstrated one-zone and 3D galaxy simulations using CELib.
Showed easy comparison of chemical evolution impacts by changing models.
Validated the library's applicability across different simulation frameworks.
Abstract
We have developed a software library for chemical evolution simulations of galaxy formation under the simple stellar population (SSP) approximation. In this library, all of the necessary components concerning chemical evolution, such as initial mass functions, stellar lifetimes, yields from type II and Ia supernovae, asymptotic giant branch stars, and neutron star mergers, are compiled from the literature. Various models are pre-implemented in this library so that users can choose their favorite combination of models. Subroutines of this library return released energy and masses of individual elements depending on a given event type. Since the redistribution manner of these quantities depends on the implementation of users' simulation codes, this library leaves it up to the simulation code. As demonstrations, we carry out both one-zone, closed box simulations and three-dimensional…
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