${session.getAttribute("locale")} 5 Galactic haloes in MONDian cosmological simulations 3 that can be readily ascribed to the low Ω0 value adopted. The agreement with ΛCDM at redshift z= 0 is driven by the more rapid structure evolution in MOND. Moreover, galaxy formation appears to be more strongly biased in MONDian cosmologies. Within the current implementation of MOND, density profiles of gravitationally bound objects at z= 0 can still be fitted by the universal Navarro, Frenk & White (NFW) profile, but MOND haloes are less clumpy.]]> Wed 18 Mar 2015 02:11:36 EST ]]>