Three-body effects greatly complicate stellar evolution. We model the
effects of encounters of binaries with single stars, based on paramete
rs chosen from conditions prevalent in the cores of globular clusters.
For our three-body encounters, we start with a population of primordi
al binaries, and choose incoming stars from the evolving single star p
opulations of paper I. In addition, we study the formation of new bina
ries through tidal capture among the single stars. In subsequent paper
s in this series, we will combine stellar evolution with the dynamics
of a full N-body system.