Initial and final masses and half-mass radii of the clusters. The dotted lines represent when the timescales (t_coll and t_rx) are equal to τ = 4 Myr. The shaded regions indicate the parameter space where the respective timescales fall within the range 1 Myr ≤ τ ≤ 10 Gyr, highlighting different dynamical regimes: pink for two-body relaxation and gray for stellar collisions. Our clusters R0005N50k, R001N100k, R001N250k, R005N500k, and R005N750k evolve for 3.73, 3.81, 3.64, 3.80, and 3.87 Myr, respectively. We show their initial conditions with empty symbols and the final conditions with filled symbols, connected by arrows.