Table 1
Summary of all scenarios.
Scenario name | Nemb / Nplan | femb | Model | Arch. | Pla-Pla |
---|---|---|---|---|---|
SPH[01-05]-cJS-pp1 | 35 / 150 | 0.7 | SPH | cJS | Yes |
SPH[06-10]-cJS-pp0 | 35 / 150 | 0.7 | SPH | cJS | No |
SPH[11-15]-eJS-pp1 | 35 / 150 | 0.7 | SPH | eJS | Yes |
SPH[16-20]-eJS-pp0 | 35 / 150 | 0.7 | SPH | eJS | No |
PM[01-03]-cJS-pp1 | 35 / 150 | 0.7 | PM | cJS | Yes |
PM[04-06]-cJS-pp0 | 35 / 150 | 0.7 | PM | cJS | No |
PM[07-09]-eJS-pp1 | 35 / 150 | 0.7 | PM | eJS | Yes |
PM[10-12]-eJS-pp0 | 35 / 150 | 0.7 | PM | eJS | No |
EO-SPH[21-25]-cJS | 29 / 0 | 1.0 | SPH | cJS | Yes |
EO-SPH[26-30]-eJS | 29 / 0 | 1.0 | SPH | eJS | Yes |
EO-PM[13-15]-cJS | 29 / 0 | 1.0 | PM | cJS | N/a |
EO-PM[16-18]-eJS | 29 / 0 | 1.0 | PM | eJS | N/a |
Notes. Nemb and Nplan are the initial numbers of embryos andplanetesimals. femb gives the mass fraction of the disk in embryos. “SPH” indicates our collision model, while “PM” indicates that all collisions are resolved with perfect merging. “Pla-Pla” indicates whether planetesimal–planetesimal interactions are included (pp1 vs. pp0). The embryo-onlyruns in the lower part of the table are marked by an “EO” prefix.
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