Some comments on gravitational clustering simulations of ''Ino'' dominated universes

Large-scale numerical simulations of universes dominated by collisionless elementary particles possess a number of ambiguities: (1) identification of the ''present'', (2) identification of the onset of galaxy formation, and (3) the relationship between simulation points and galaxies. It is possible to modify the interpretation of simulations in such a way as to make various alternatives more closely resemble the observed universe. Some statistical measures to favor so-called ''hot'' particles, while others favor ''cold'' particles. It seems that at this time neither can be ruled out