Dianoga SIDM: Galaxy cluster self-interacting dark matter simulations

Open Access

Fig. 6.

Rescaled DM central density ${\hat{ρ}}_{c}$ $\hat{\rho}_{\mathrm{c}}$ as a function of rescaled time $β \hat{σ} \hat{t}$ $\beta\hat{\sigma}\hat{t}$ , for our FP SIDM (red circles) and DMO SIDM (grey stars) runs. We also overplot the model from Yang et al. (2023, black solid line). The red shaded area shows the mean value of the FP SIDM points with its one standard deviation, while the blue shaded area shows the same for collisionless FP runs.

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