chemcomp: Modeling the chemical composition of planets formed in protoplanetary disks
arxiv(2023)
摘要
Future observations of exoplanets will hopefully reveal detailed constraints
on planetary compositions. Recently, we have developed and introduced chemcomp
(Schneider Bitsch 2021a), which simulates the formation of planets in
viscously evolving protoplanetary disks by the accretion of pebbles and gas.
The chemical composition of planetary building blocks (pebbles and gas) is
traced by including a physical approach of the evaporation and condensation of
volatiles at evaporation lines. We have now open-sourced the chemcomp code to
enable comparisons between planet formation models and observational
constraints by the community. The code can be found at
https://github.com/AaronDavidSchneider/chemcomp, is easy to use (using
configuration files) and comes with a detailed documentation and examples.
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