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Table 1
Details of the planetesimal annuli: their final mass Mplts and radial extent (Rin and Rout), formed in runs with different underlying protoplanetary disk models, global solids-to-gas ratio Z, turbulence strength αt, and initial disk size Rdisk.
| Diska | Z | α t | R disk b | M plts c | R in b | R out b |
|
|
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| 0.01 | 10-3 | 100 | – | – | – | |
| 0.02 | 10-3 | 100 | 3.54 | 1.98 | 2.34 | |
| P-L | 0.03 | 10-3 | 100 | 24.28 | 1.93 | 2.99 |
| 0.04 | 10-3 | 100 | 62.76 | 1.89 | 3.90 | |
| 0.05 | 10-3 | 100 | 115.10 | 1.87 | 4.90 | |
|
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| 0.03 | 10-4 | 100 | 217.13 | 1.66 | 5.19 | |
| P-L | 0.03 | 3 × 10-4 | 100 | 128.79 | 1.81 | 3.44 |
| 0.03 | 3 × 10-3 | 100 | – | – | – | |
| 0.03 | 10-2 | 100 | – | – | – | |
|
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| 0.03 | 10-3 | 60 | 8.90 | 1.89 | 2.45 | |
| P-L | 0.03 | 10-3 | 80 | 16.73 | 1.91 | 2.75 |
| 0.03 | 10-3 | 140 | 38.52 | 1.94 | 3.50 | |
| 0.03 | 10-3 | 200 | 49.50 | 1.98 | 4.10 | |
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| 0.01 | 10-3 | 100 | 119.80 | 1.03 | 2.20 | |
| 0.02 | 10-3 | 100 | 371.37 | 0.98 | 4.08 | |
| N-IRR | 0.03 | 10-3 | 100 | 663.18 | 0.96 | 5.50 |
| 0.04 | 10-3 | 100 | 928.35 | 0.96 | 6.83 | |
| 0.05 | 10-3 | 100 | 1130.9 | 0.95 | 8.00 | |
|
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| 0.01 | 10-3 | 100 | – | – | – | |
| 0.02 | 10-3 | 100 | 3.32 | 2.12 | 4.33 | |
| IRR | 0.03 | 10-3 | 100 | 22.50 | 1.64 | 7.16 |
| 0.04 | 10-3 | 100 | 63.31 | 1.25 | 10.37 | |
| 0.05 | 10-3 | 100 | 129.93 | 1.06 | 16.99 | |
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