Abstract :
We consider the recent description of elementary particles in terms of quantum mechanical Kerr–Newman black holes (QMKMBH), a description which provides a rationale for and at the same time reconciles the Bohm-hydrodynamical formulation on the one hand and the Nelsonian stochastic 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.
