Fig. 10
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Power spectra for several MOND interpolating functions and parameters (in coloured lines). In back solid line we show the Newtonian counterpart, while the black dashed line refers to a MOND run with the simple parametrisation using the code Phantom of RAMSES. For MOND simulations we use g0 = 10−10 m s−2 and N = 0. In PySCo, we use the multigrid solver in any case.
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