Fig. F.1.

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Total acceleration atot relative to the MOND-like acceleration for a galaxy with Mb = 2 × 1010 M⊙ for different model parameters m2 and fG but with the same boundary condition imposed at r = 0. This boundary condition is chosen such that the first maximum of
is 1.1 for m = 1 Mpc−1 and fG = 0.6. This illustrates that the total acceleration begins to oscillate at large radii. It also illustrates that the total acceleration depends only on the combination m2/fG but not on m2 and fG individually.
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