Table 2
Results of N-body simulations integrating the four or five giant planets initially in a resonant chain built in Sec. 2.
| Resonant chain | Name | Nsim | MD (M⊕) | A (%) | B (%) | C (C*) (%) | D; D* (%) | C∩D; C∩D* (%) | |
|---|---|---|---|---|---|---|---|---|---|
| Cold protoplanetary disc (h = (0.035) | |||||||||
| 200 | 30 | 7 | 0.5 | 0.5 (0.5) | 0; 0 | ||||
| (2:1, 3:2, 5:4) | C4 | 200 | 50 | 25.5 | 18 | 1 (4) | 3; 10 | 0; 1 | |
| (2:1, 3:2, 5:4, 4:3) | C5 | 200 | 30 | 9 | 4 | 1 (1) | 0; 0 | ||
| 200 | 50 | 21 | 13.5 | 1.5 (3) | 3; 4 | 0.5; 1.5 | |||
| Nominal protoplanetary disc (h = 0.05) | |||||||||
| (2:1, 3:2, 4:3) | N4 | 50 | 30 | 98 | 1 | 0 (0) | 0; 0 | ||
| 100 | 50 | 69 | 29 | 1 (2) | 2; 10 | 1; 0 | |||
| (2:1, 2:1, 4:3) | Nbis4 | 50 | 30 | 100 | 100 | 0 (0) | 0; 0 | ||
| 50 | 50 | 100 | 96 | 0 (0) | 0; 70 | ||||
| (2:1, 2:1, 4:3, 5:4) | Nbis5 | 100 | 30 | 19 | 10 | 0 (2) | 3; 0 | ||
| 100 | 50 | 4 | 3 | 0 (0) | 1; 1 | ||||
Notes. Column 1 – initial resonant chain. Column 2 – name of the hydrodynamical simulation. Column 3 – number of N-body simulations ran for the statistical study. Column 4 – mass of the planetesimal disc placed outside of the last planets’ orbit. Columns 5–9 – success rate of the criteria detailed in Sec. 3.2.
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