ASCL Code Record
[ascl:2604.010]
DiscEvolution: Model the evolution of dust and gas in protoplanetary discs
DiscEvolution contains a set of modules to simulate the viscous evolution of protoplanetary discs over Myr time scales. The package includes modules to compute viscous evolution, grain growth, radial drift, thermal structure, transport of volatiles and planet formation.
- Code site:
- https://github.com/rbooth200/DiscEvolution
- Described in:
- https://ui.adsabs.harvard.edu/abs/2017MNRAS.469.3994B
- Bibcode:
- 2026ascl.soft04010B
Preferred citation method:
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