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Fixing typo in paper
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stammler committed May 23, 2023
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# Statement of need

Since `DustPy` is based on the `Simframe` framework for scientific simulations [@stammler2022a], it is rather simple to interchange and modify every aspect of the software. Numerous peer-review publications already made use interchangeability of `DustPy` modules investigating a variety of open questions of protoplanetary disk evolution. For example the formation of planetesimals in density enhancements [@stammler2019; @miller2021], the permeability of gaps opened by planets [@stammler2023], the influence of dust particle size distributions on the gas ionization fraction and therefore on the magnetorotational instability [@delage2023], or the effect erosion on dust evolution on young protoplanetary disks [@xu2023].
Since `DustPy` is based on the `Simframe` framework for scientific simulations [@stammler2022a], it is rather simple to interchange and modify every aspect of the software. Numerous peer-review publications already made use of the interchangeability of `DustPy` modules investigating a variety of open questions of protoplanetary disk evolution. For example the formation of planetesimals in density enhancements [@stammler2019; @miller2021], the permeability of gaps opened by planets [@stammler2023], the influence of dust particle size distributions on the gas ionization fraction and therefore on the magnetorotational instability [@delage2023], or the effect erosion on dust evolution on young protoplanetary disks [@xu2023].

The purpose of `DustPyLib` is to provide a library of `DustPy` modifications and extensions that users can easily import and use in their own `DustPy` setups or which can help to reproduce previous results. `DustPyLib` is meant to be a community project, where users can contribute their own customizations making them available for others to be used in their own projects. In that sense it is similar to the `REBOUNDx` extension package [@tamayo2020] for the N-body solver `REBOUND` [@rein2012].

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