CavityWidth
This parameter is specific to
a set of simulations performed to evaluate the efficiency of planet
trapping at a cavity edge. Unless you want to reproduce these
simulations, you should simply ignore this variable. If you use it, you
also have to define CavityRadius
and CavityRatio. CavityWidth is the radial distance,
expressed in disk pressure scale heights (H), over which the surface density
and viscosity transitions occur. More precisely, the log(viscosity) is an affine function of r between CavityRadius-CavityWidth*H and CavityRadius+CavityWidth*H. Note
that the surface density is only approximately initialized so as to
mimic the cavity, so the initial state is not a steady state. If you
want a steady state, you should allow your system to relax over a few
viscous timescales.