  We consider the recent description of elementary particles in terms of
Quantum Mechanical Kerr-Newman Black Holes, a description which provides a
rationale for and at the same time reconciles the Bohm-hydrodynamical
formulation on the one hand and the Nelsonian stochastiic formulation on the
other. The Boson-Fermion divide is discussed, and it is pointed out that in
special situations, anomalous statistics, rather than Bose-Einstein or
Fermi-Dirac states, can be encountered.
