Dark matter halo dynamics in 2D Vlasov simulations - A self-similar approach

Open Access

Fig. 13.

Trends in residuals $(= \frac{1}{N} Σ (Δ r)^{2})$ $\left ({=}\frac {1}{N} \Sigma (\Delta r)^2\right )$ computed using r−q curves of Lagrangian slices along the x-axis with varying ϵ for the three cases: Q1D (left), ANI (middle), SYM (right).

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