  The statistical mechanics of a gas of Einstein-Kalb-Ramond wormholes is
studied in this paper. The wormholes studied are the result of sewing together
two Reissner-Nordstrom-type black hole metrics at their horizons. By requiring
the stress-energy tensor associated with this geometry to be that of a
Kalb-Ramond field, we obtain the mass and Kalb-Ramond `charge` of the wormholes
in terms of the parameters describing the mass density, tension and pressure.
We investigate the statistical mechanics of this system of wormholes within the
context of the statistical bootstrap model. A gas of such wormholes is found to
obey the bootstrap condition only for an extreme, non-thermodynamic, energy and
`charge` distribution among the particles. We comment briefly on the scattering
of quantum wormholes.
