The project was initiated after the Building Blocks of Planets 2020 conference. The goal is to perform and compare simulations of the dust and gas drag instabilities in accretion disks. We aim to have a broad number of different methods and codes, including fluid and particle descriptions.
Stage 1 (active)
Collection of setup ideas. Brainstorming and open discussion. Please use the overleaf document below.
Stage 2
Simulation and performance of the setup. Comparing the different results and analysis.
Stage 3
Summarising of the results. Collecting the plots. Writing the publication.
Stage 1
We are currently in the stage of formulating the goal and framework of the test setups.
Please use the overleaf document. The current progress will be shown here.
Current Progress: Discussion of goals of the setup.