Dust Drag Code Comparison

Dust/Gas Drag Instability Code Comparison Project


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.


Dust-drag code comparison meeting 2022

1.6-3.6.2022

 

Planets in the Desert - A Streaming Instability Code Comparison


Together with the TCAN collaboration we propose a first workshop to discuss the code comparison setup.

The meeting will include invited and contributed talks and a coding session. 


The talk sessions will start in the morning MST time and afternoon CET times at 8am/4pm MST/CET.


Venue:

O'Donnell Hall at NMSU Main Campus, in Las Cruces

Meeting at room OH 111

Coffee Breaks at 10am/3pm MDT


Recommended Hotel:

Marriott




The meeting will provide Zoom sessions and a Slack channel


Time (MDT - am)/(CET - pm) Wednesday Thursday Friday
8:00/4:00 Anders Johansen Andrew Youdin Urs Schäfer
8:30/4:30 Pablo Benitez-Llambay  Chao Chin Yang Daniel Carrera
9:00/5:00 Rixin Li Leonardo Krapp Orkan Umhurhan
9:30/5:30 Min-Kai Lin Debanjan Sengupta Mario Flock
10:00/6:00 -- Break -- -- Break -- -Break--
10:30/6:30 Joanna Drazkowska Jake Simon Discussion
11:00/7:00 Talk discussions Talk discussions Coding/Session
11:30/7:30 Benchmark/setup discussion Benchmark/setup Discussion
12:00/8:00 END END
TCAN TCAN TCAN

Stage 1 (active)

 Collection of setup ideas. Brainstorming and open discussion.

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. 
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