Star clusters with a high central density contain an ecological networ
k of evolving binaries, affected by interactions with passing stars, w
hile in turn affecting the energy budget of the cluster as a whole by
giving off binding energy, This is the first paper in a series aimed a
t providing the tools for increasingly realistic simulations of these
ecological networks. Here we model the core of a globular star cluster
. The two main approximations are: a density of stars constant in spac
e and time, and a purely single star population in which collisions be
tween the evolving stars are modeled. In future papers in this series,
we will relax these crude approximations. Here, however, they serve t
o set the stage before proceeding to the additional complexity of bina
ry star interactions, in paper Il, and background dynamical evolution,
in later papers.