Table 1
Initial conditions for the five scenarios explored in this study.
| (a) | (b) | (c) | (d) | |
|---|---|---|---|---|
| Scenario 1 | 1 | 1 | 100.2 | 08 |
| Scenario 2 | 1 | 0 | 0 | 02 |
| Scenario 3 | 2 | 0 | 0 | 04 |
| Scenario 4 | 2 | 1 | 100.2 | 01 |
| Scenario 5 | 2 | 1 | 100.2 | 05 |
Notes. The multi-resonance configuration is the 3:2, 3:2, 2:1, 3:2, with the outermost planet at 20.18 au from the Sun. In all cases studied here, we used a disk of 40 M⊕. (a) Distance of the inner bound of the disk (au), (b) inclination of the disk with respect to the invariable plane (°), (c) node of the disk (°), and (d) running number, i.e., number of generations used.
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