All Tables

Table 1: Summary of mass estimates for the inner 10 AU region, as derived from previous works.
Table 2: Numerical estimate of $\langle f_{i(k)}\rangle$ in the 5 AU region, for a swarm of grains produced in the whole 1-10 AU region, as a function of $\beta _k$ (see text for details). Note that for low $\beta$ , e_k might become lower than the average eccentricity for the parent bodies in the disc (see Sect. 2.1). In such a case, the radiation pressure effect is neglected for all $e_{k}<\langle e_{0}\rangle$ and the values of $\langle f_{i(k)}\rangle$ rescaled so that $\langle f_{i(k)}\rangle =1$ for $e_{k}=\langle e_{0}\rangle$ .
Table 3: Initial parameters for the nominal reference run (see text for details).
Table 4: This table sums up, for all objects within 3 different size ranges, the respective amount of mass that is removed by all cratering and all fragmenting impacts. These values are obtained in the steady state regime for the nominal case.