DARKSKIES: A suite of super-sampled zoom-in simulations of galaxy clusters with self-interacting dark matter

Open Access

Fig. C.1.

Effective models simulated ( for a given halo mass at a z = 0 ), assuming relative particle velocities following $v \sim \sqrt{G M / r}$ $v\sim\sqrt{GM/r}$ . The stars show the velocity-independent models. The lines show how these can be recast into velocity-dependent models, assuming a constant asymptotic cross-section (top panel) or a constant turn over velocity (bottom panel).

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