Open Access

This article has an erratum: [https://doi.org/10.1051/0004-6361/202141096e]


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
disk disk accretion rate

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