Fig. 5
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Evolution of an isolated halo as a function of time for two different choices of Nngb. The upper panel gives the mass enclosed within 10 pc and the lower panel displays the energy conservation as a function of time. The choice of Nngb = 384 corresponds to twice the kernel size compared to the SIDM computations for Nngb = 48. Table A.1 gives the parameters employed for the displayed simulations J and K.
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