GALAXY CLUSTER BULK FLOWS AND COLLISION VELOCITIES IN QUMOND.

We examine the formation of clusters of galaxies in numerical simulations of a QUMOND cosmogony with massive sterile neutrinos. Clusters formed in these exploratory simulations develop higher velocities than those found in ACDM simulations. The bulk motions of clusters attain ~1000 km s-1 by low redshift, comparable to observations whereas ACDM simulated clusters tend to fall short. Similarly, high pairwise velocities are common in cluster-cluster collisions like the Bullet Cluster. There is also a propensity for the most massive clusters to be larger in QUMOND and to appear earlier than in ACDM, potentially providing an explanation for "pink elephants" like El Gordo. However, it is not obvious that the cluster mass function can be recovered. [ABSTRACT FROM AUTHOR]