Table A.1.
Explanations of variables related to the disk used in our model.
Parameter | Explanation |
---|---|
ν | alpha viscosity parameter |
cs | sound speed |
ΩK | Kepler angular velocity |
G | Gravitational constant |
M⋆ | Mass of central star |
r | radius coordinate of the disk |
kB | Boltzmann constant |
Tmid | Temperature of the midplane |
μ | mean molecular weight |
mp | proton mass |
Δv | sub-Keplerian azimuthal speed |
vK | Keplerian velocity |
vφ | azimuthal velocity of the gas |
P | Gas pressure |
Hgas | scale height of the disk |
St | Stokes number of a particle |
τf | stopping time of a particle |
a | particle size |
ρ• | density of a dust and pebble particle |
Σgas | Gas surface density |
uZ | general pebble/dust drift velocity |
ugas | gas diffusion velocity |
ϵ | solid to gas ratio |
ΣZ | total dust surface density (pebbles and dust) |
fm | mass fraction of pebbles |
Σpeb | surface density of pebbles |
Σdust | surface density of dust |
ûZ | mass averaged dust drift velocity (dust and pebbles) |
upeb | pebble drift velocity |
udust | dust drift velocity |
Y | molecular species |
t | time |
![]() |
source/sink term for viscous evolution |
M0 | initial disk mass |
R0 | scaling radius of the disk |
ψ | logarithmic gradient of the viscosity at the inner edge |
rin | radius at the inner edge of the disk |
ξ | normed time |
tν | viscous time |
![]() |
evaporation source term |
![]() |
condensation source term |
![]() |
source term due to the discount of accreted pebbles |
rice,Y | position of the evaporation line of species Y |
adust | dust size |
apeb | pebble size |
ϵp | pebble sticking efficiency |
μY | mass of species Y (in proton masses) |
![]() |
photoevaporation source term |
tevap | start of photoevaporation |
τdecay | decay timescale of the disk |
Ṁdisk | disk accretion rate |
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