  We calculate the intrinsic entropy of a Schwarzschild black hole in an
asymptotically antide Sitter space. The statistical calculation of the entropy
is based on a model for particle structure that leads to confinement. The
constituents of the particle are distinguishable quasiparticles. The entropy
(temperature) is less (greater) than the entropy of a Schwarzschild black hole
in an asymptotically flat space. The equilibrium thermodynamic states are
described by pure states, myriotic fields, and the distinguishability of the
internal microstates may provide a solution to the black hole information
paradox by suggesting a Bose-Einstein condensate whereby the zero mass state is
a limit point (or accumulation point) of condensates on the event horizon.
