Table 1
Predicted companion population around WDs for different model assumptions.
| 1000 planets simulation | af | ef | MWD | tWD | ttot | fsurv | fWD |
|---|---|---|---|---|---|---|---|
| (AU) | (M⊙) | (Gyr) | (Gyr) | ||||
| Villaver (Baseline) | ![]() |
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262/1000 | 1.3% |
| Rasio (Baseline) | ![]() |
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123/1000 | 0.6% |
| No Tidal Forces | ![]() |
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652/1000 | 3.2% |
| Villaver (Pbreak=1500 days) | ![]() |
![]() |
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573/1000 | 2.8% |
| Rasio (Pbreak=1500 days) | ![]() |
![]() |
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386/1000 | 1.9% |
| Villaver (e=0) | ![]() |
0.00 | ![]() |
![]() |
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343/1000 | 1.7% |
| Rasio (e=0) | ![]() |
0.00 | ![]() |
![]() |
![]() |
170/1000 | 0.8% |
| Villaver (ηB = 0.7) | ![]() |
![]() |
![]() |
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579/1000 | 2.9% |
| Rasio (ηB = 0.7) | ![]() |
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405/1000 | 2.0% |
Notes. We tested the impact of the assumed mass-loss efficiency for stars on the AGB, the assumed strength of tidal forces, the adopted eccentricity and planet-mass distribution, as well as the age-metallicity relation assumed for the WD progenitor stars. Each entry shows the median value with the 16th and 84th percentiles. Columns correspond to final semimajor axis, final eccentricity, WD mass, WD age, total system age, survival rate, and predicted fraction of WDs hosting substellar companions, normalized to the total sample of 20 315 WDs.
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