Summary of the numerical simulations. Ref. is the reference number of the simulation, |$0.1\, {\rm mm}$| and |$0.5\, {\rm mm}$| refer to the large dust grain size we used, Mp is the planet mass, Rp its separation from the central star, hc is the disc aspect ratio at |$R_{\rm 0}=56 \, {\rm au}$| and finally Npart is the total number of particles. Simulations 7 and 8 are convergence tests that we performed with a larger number of particles.
| Ref. . | |$0.1\, {\rm mm}$| . | |$0.5\, {\rm mm}$| . | Mp . | Rp . | hc . | Npart . |
|---|---|---|---|---|---|---|
| 1 | x | |$3\, M_{\rm J}$| | |$20\, {\rm au}$| | 0.07 | 7.5 × 105 | |
| 2 | x | |$6\, M_{\rm J}$| | |$20\, {\rm au}$| | 0.10 | 7.5 × 105 | |
| 3 | x | |$9\, M_{\rm J}$| | |$20\, {\rm au}$| | 0.12 | 7.5 × 105 | |
| 4 | x | |$3\, M_{\rm J}$| | |$20\, {\rm au}$| | 0.07 | 7.5 × 105 | |
| 5 | x | |$6\, M_{\rm J}$| | |$20\, {\rm au}$| | 0.10 | 7.5 × 105 | |
| 6 | x | |$9\, M_{\rm J}$| | |$20\, {\rm au}$| | 0.12 | 7.5 × 105 | |
| 7 | x | |$9\, M_{\rm J}$| | |$20\, {\rm au}$| | 0.12 | 1.5 × 106 | |
| 8 | x | |$9\, M_{\rm J}$| | |$20\, {\rm au}$| | 0.12 | 2.2 × 106 |
| Ref. . | |$0.1\, {\rm mm}$| . | |$0.5\, {\rm mm}$| . | Mp . | Rp . | hc . | Npart . |
|---|---|---|---|---|---|---|
| 1 | x | |$3\, M_{\rm J}$| | |$20\, {\rm au}$| | 0.07 | 7.5 × 105 | |
| 2 | x | |$6\, M_{\rm J}$| | |$20\, {\rm au}$| | 0.10 | 7.5 × 105 | |
| 3 | x | |$9\, M_{\rm J}$| | |$20\, {\rm au}$| | 0.12 | 7.5 × 105 | |
| 4 | x | |$3\, M_{\rm J}$| | |$20\, {\rm au}$| | 0.07 | 7.5 × 105 | |
| 5 | x | |$6\, M_{\rm J}$| | |$20\, {\rm au}$| | 0.10 | 7.5 × 105 | |
| 6 | x | |$9\, M_{\rm J}$| | |$20\, {\rm au}$| | 0.12 | 7.5 × 105 | |
| 7 | x | |$9\, M_{\rm J}$| | |$20\, {\rm au}$| | 0.12 | 1.5 × 106 | |
| 8 | x | |$9\, M_{\rm J}$| | |$20\, {\rm au}$| | 0.12 | 2.2 × 106 |
Summary of the numerical simulations. Ref. is the reference number of the simulation, |$0.1\, {\rm mm}$| and |$0.5\, {\rm mm}$| refer to the large dust grain size we used, Mp is the planet mass, Rp its separation from the central star, hc is the disc aspect ratio at |$R_{\rm 0}=56 \, {\rm au}$| and finally Npart is the total number of particles. Simulations 7 and 8 are convergence tests that we performed with a larger number of particles.
| Ref. . | |$0.1\, {\rm mm}$| . | |$0.5\, {\rm mm}$| . | Mp . | Rp . | hc . | Npart . |
|---|---|---|---|---|---|---|
| 1 | x | |$3\, M_{\rm J}$| | |$20\, {\rm au}$| | 0.07 | 7.5 × 105 | |
| 2 | x | |$6\, M_{\rm J}$| | |$20\, {\rm au}$| | 0.10 | 7.5 × 105 | |
| 3 | x | |$9\, M_{\rm J}$| | |$20\, {\rm au}$| | 0.12 | 7.5 × 105 | |
| 4 | x | |$3\, M_{\rm J}$| | |$20\, {\rm au}$| | 0.07 | 7.5 × 105 | |
| 5 | x | |$6\, M_{\rm J}$| | |$20\, {\rm au}$| | 0.10 | 7.5 × 105 | |
| 6 | x | |$9\, M_{\rm J}$| | |$20\, {\rm au}$| | 0.12 | 7.5 × 105 | |
| 7 | x | |$9\, M_{\rm J}$| | |$20\, {\rm au}$| | 0.12 | 1.5 × 106 | |
| 8 | x | |$9\, M_{\rm J}$| | |$20\, {\rm au}$| | 0.12 | 2.2 × 106 |
| Ref. . | |$0.1\, {\rm mm}$| . | |$0.5\, {\rm mm}$| . | Mp . | Rp . | hc . | Npart . |
|---|---|---|---|---|---|---|
| 1 | x | |$3\, M_{\rm J}$| | |$20\, {\rm au}$| | 0.07 | 7.5 × 105 | |
| 2 | x | |$6\, M_{\rm J}$| | |$20\, {\rm au}$| | 0.10 | 7.5 × 105 | |
| 3 | x | |$9\, M_{\rm J}$| | |$20\, {\rm au}$| | 0.12 | 7.5 × 105 | |
| 4 | x | |$3\, M_{\rm J}$| | |$20\, {\rm au}$| | 0.07 | 7.5 × 105 | |
| 5 | x | |$6\, M_{\rm J}$| | |$20\, {\rm au}$| | 0.10 | 7.5 × 105 | |
| 6 | x | |$9\, M_{\rm J}$| | |$20\, {\rm au}$| | 0.12 | 7.5 × 105 | |
| 7 | x | |$9\, M_{\rm J}$| | |$20\, {\rm au}$| | 0.12 | 1.5 × 106 | |
| 8 | x | |$9\, M_{\rm J}$| | |$20\, {\rm au}$| | 0.12 | 2.2 × 106 |
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