Protoplanetary disks are composed of gas and dust from which planetary systems ultimately emerge, yet a long-standing puzzle is how small dust particles grow into larger bodies despite frequent destructive collisions. Here, we developed a MATLAB model to simulate the motion of dust particles embeded in the gas disk. In this multi-phase fluid, two parameters are of particular importance: the Stokes number and the Reynolds number. A fundamental review on this topic can be found through: https://doi.org/10.1146/annurev-astro-071221-052705
引用格式
Jiaru (2026). Gas-solid Coupling Model (https://ww2.mathworks.cn/matlabcentral/fileexchange/183321-gas-solid-coupling-model), MATLAB Central File Exchange. 检索时间: .
MATLAB 版本兼容性
创建方式
R2025b
兼容 R2014b 到 R2026a 的版本
平台兼容性
Windows macOS Linux标签
| 版本 | 已发布 | 发行说明 | |
|---|---|---|---|
| 1.0.0 |
