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Dark matter haloes from dwarf to massive galaxies: No systematic inner-density tension with ΛCDM hydrodynamical simulations
Two of the most prominent small-scale challenges to the standard cold dark matter (CDM) paradigm are the cusp--core and diversity-of-rotation-curves problems. The former concerns the shallow inner dark matter density profiles inferred for many galaxies compared with the cusps predicted by collisionless CDM simulations,...