Table 1: A subset of the 3D models performed. From left to right, the columns give: class name; mean eccentricity; standard deviation of inclination; mean mass; standard deviation of mass; lower-mass cutoff; initial separations in mutual Hill radii; disc mass (normalised against fiducial value); number of protoplanets.
Set $\mu_{\rm e}$ $\sigma_{i}$ $\mu_{\rm m}$ $\sigma_{\rm m}$ Cutoff $\Delta_0$ $\Sigma$ Np

H1		 0.05 $2^{\circ}$ - - - 5 1 8
O1 0.05 $2^{\circ}$ - - - 5 1 10
O2 0.15 $2^{\circ}$ - - - 5 1 10
O3 0.05 $6^{\circ}$ - - - 5 1 10
O4 0.10 $4^{\circ}$ - - - 5 1 10
O5 0.05 $2^{\circ}$ - - - 4 1 10
O6 0.05 $2^{\circ}$ - - - 8 1 10
O7 0.05 $2^{\circ}$ - - - 5 0.5 10
O8 0.05 $2^{\circ}$ - - - 5 0.2 10
O9 0.05 $2^{\circ}$ - - - 5 1 5
R1 0.05 $2^{\circ}$ 10 7 0.2 5 1 10
R2 0.05 $2^{\circ}$ 10 5 2 5 1 10
R3 0.05 $2^{\circ}$ 10 3 2 5 1 10
R4 0.05 $2^{\circ}$ 7 3 2 5 1 10
R5 0.05 $2^{\circ}$ 7 5 0.2 5 1 10
R6 0.10 $2^{\circ}$ 10 5 2 5 1 10
R7 0.05 $4^{\circ}$ 10 5 2 5 1 10
R8 0.10 $4^{\circ}$ 10 5 2 5 1 10
R9 0.05 $2^{\circ}$ 10 5 2 4 1 10
R10 0.05 $2^{\circ}$ 10 7 0.2 6 1 10
R11 0.05 $2^{\circ}$ 5 3 0.2 8 1 10


Source LaTeX | All tables | In the text