Figure 4.

Relative domain size $C\left(t\right)$ over time during the collapse at $\varphi =1.2$ of three-arm stars (a), 12-arm stars (b), flexible chains (c) and semiflexible chains (d). Different datasets correspond to different values of the parameters $r_{\mathrm{c}}$ and ${\rho }_{\min }$ used to construct the density field. The time t is normalized by ${\tau }_{0.5}$, defined as in Figure 3. Straight lines in all panels fit to a power-law time dependence (exponents are indicated).