Fraction of surviving planets with final mass in a certain mass interval. N_total is the sum of all surviving planets (n_surv) plus the planets lost in the central star. Final masses of the formed planets are separated into five mass bins (M < 1   M_⊕, 1 < M [M_⊕]  < 10, 10 < M [M_⊕]  < 100, 100 < M [M_⊕]  < 1000, M > 1000   M_⊕). The solid component of the planets grows by the accretion of 0.1 km planetesimals. Three different approaches in the treatment of the evolution of the eccentricities and inclinations of planetesimals are considered: equilibrium, and explicit calculation of the differential equations for a “hot” and “cold” initial conditions.