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Table 1
Breakdown of the expressions and parameters involved in the pebble accretion efficiency.
Expr. | Dependence | Description and reference |
---|---|---|
or definition | ||
εset | ε2D, ε3D | settling efficiency, Eq. (40) |
ε2D | A2, Δvy, fset | settling efficiency in 2D limit, Eq. (39a) |
ε3D | A3, heff, fset | settling efficiency in 3D limit, Eq. (39b) |
fset | Δv, σP, v*, aturb | settling fraction, Eq. (35) |
Δvy | vcir, vecc | azimuthal approach velocity, Eq. (28) |
Δvz | ai | vertical approach velocity, Eq. (31) |
v* | ![]() |
critical settling velocity |
vcir | acir, ash | circular velocity, Eq. (29) |
vecc | ae | eccentric velocity, Eq. (30) |
heff | ip, hP | effective aspect ratio, Eq. (27) |
hP | αz, tcorr | pebble aspect ratio, Eq. (15) |
A2 | 0.32 | fit constant |
A3 | 0.39 | fit constant |
acir | 5.7 | fit constant |
ae | 0.76 | fit constant |
ai | 0.68 | fit constant |
aset | 0.5 | fit constant |
ash | 0.52 | fit constant |
aturb | 0.33 | fit constant |
αz | turbulent diffusivity | |
η | disk radial pressure gradient parameter, Eq. (6) | |
τs | tstopΩ | dimensionless stopping time |
σP | (σx, σy, σz) | pebble rms velocity (Eq. (33)) |
ep | planet eccentricity | |
hgas | Hgas∕r | disk aspect ratio |
ip | planet inclination | |
qp | Mpl∕M⋆ | planet-to-star mass ratio |
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