A First Look at Galaxy Flyby Interactions: Characterizing the Frequency
  of Flybys in a Cosmological Context
  Hierarchical structure formation theory is based on the notion that mergers
drive galaxy evolution, so a considerable framework of semi-analytic models and
N-body simulations has been constructed to calculate how mergers transform a
growing galaxy. However, galaxy mergers are only one type of major dynamical
interaction between halos -- another class of encounter, a close flyby, has
been largely ignored. We analyze a 50 Mpc/h, $1024^3$ collisionless
cosmological simulation and find that the number of close flyby interactions is
comparable to, or even surpasses, the number of mergers for halo masses $\ga
10^{11}\,{h^{-1} M_\odot}$ at $z \la 2$. Halo flybys occur so frequently to
high mass halos that they are continually perturbed, unable to reach a
dynamical equilibrium. We also find tentative evidence that at high redshift,
$z \ga 14$, flybys are as frequent as mergers. Our results suggest that close
halo flybys can play an important role in the evolution of the earliest dark
matter halos and their galaxies, and can still influence galaxy evolution at
the present epoch.
