Table 1
Summary of our numerical models.
| Name | Planet mass [M⊕] | Stokes number (St) | Feedback |
|---|---|---|---|
| Mp0.03LR(a) | 0.03 | 0.0 | No |
| 2.8 × 10−5 | No | ||
| 2.8 × 10−5 | Yes | ||
| 0.0028 | Yes | ||
| 0.028 | Yes | ||
| 0.28 | Yes | ||
| Mp0.3AD | 0.3 | 0.0 | No |
| 0.001 | Yes | ||
| 0.1 | Yes | ||
| Mp0.3TD | 0.3 | 0.001 | Yes |
| 0.1 | Yes | ||
| Mp1.0AD | 1.0 | 0.001 | Yes |
| 0.01 | Yes | ||
| 0.1 | Yes | ||
| Mp1.0TD | 1.0 | 0.001 | Yes |
| 0.01 | Yes | ||
| 0.1 | Yes |
Notes. The first column shows the model name, here the capital letters in model names have the following meaning. LR: linear regime, AD: adiabatic disk, TD: thermal diffusivity. The second column shows the mass of the planet (in units of Earth masses). The third column shows the dimensionless Stokes number (see Eq. (10)). The fourth column shows the flag of the inclusion of the back-reaction force from the dust on gas. Note that models with feedback and the same value of the planet’s mass represent a two-fluid simulation. (a)Model in the local mesh approach.
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