  In this paper a series of high-resolution n-body simulations is presented in
which the equations of motion have been changed to account for MOdified
Newtonian Dynamics (MOND). It is shown that a low-Omega0 MONDian model with an
appropriate choice for the normalisation sigma8 can lead to similar clustering
properties at redshift z=0 as the commonly accepted (standard) LCDM model.
However, such a model shows no significant structures at high redshift with
only very few objects present beyond z>3 that can be readily ascribed to the
low Omega0 value adopted. The agreement with LCDM 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 NFW profile but MOND halos are less
clumpy.
