  We investigate the black hole solution to (2+1)-dimensional gravity coupled
to topological matter, with a vanishing cosmological constant. We calculate the
total energy, angular momentum and entropy of the black hole in this model and
compare with results obtained in Einstein gravity. We find that the theory with
topological matter reverses the identification of energy and angular momentum
with the parameters in the metric, compared with general relativity, and that
the entropy is determined by the circumference of the inner rather than the
outer horizon. We speculate that this results from the contribution of the
topological matter fields to the conserved currents. We also briefly discuss
two new possible (2+1)-dimensional black holes.
