Table 4.
Parameter settings of the K2-MZ simulations for different planet formation scenarios.
Model name | Parameter settings |
Results |
||||
---|---|---|---|---|---|---|
M1 | M2 | ΔZacc | Zproto | MXY, lost | MZ, planet | |
[M⊙] | [M⊙] | [M⊙] | [M⊕] | |||
MZ1 | 0.90 | 0.92 | 0.06 | 0.0155 | 0 | 213 |
MZ2 | 0.95 | 0.97 | 0.06 | 0.0144 | 0.04 | 150 |
MZ3 | 0.88 | 0.92 | 0.03 | 0.0155 | 0 | 213 |
MZ4 | 0.88 | 0.92 | 0.06 | 0.0148 | 0.03 | 150 |
MZ5 | 0.9703 ( * ) | 0.9703 ( * ) | – | 0.0152 | 0 | 150 |
MZ6 | 0.86 | 0.92 | 0.02 | 0.0155 | 0 | 214 |
MZ7 | 0.86 | 0.92 | 0.06 | 0.0140 | 0.08 | 150 |
MZ8 | 0.91 | 0.97 | 0.06 | 0.0132 | 0.14 | 150 |
MZ9 | 0.92 | 0.94 | 0.06 | 0.0151 | 0.01 | 150 |
Notes. fovershoot = 0.01, A2 = 0.12, and tacc = 5 Myr (see Table 1). The MXY, lost and MZ, planet values were calculated using the optimized Zproto value (see text for details). ΔZacc = Zacc,max − Zproto. See Fig. 4 for the definitions of M1 and M2. ( * )In MZ5, we assumed that there is no pebble accretion phase (i.e., M1 = M2), MXY, lost = 0, and MZ, planet = 150 M⊕; thus, M1 was determined by Zproto (see Eq. (9)).
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