  Black hole spacetimes are semiclassically not static. For black holes whose
lifetime is larger than the age of the universe we compute, in leading order,
the power spectrum of deviations of the electromagnetic charge from it's
average value, zero. Semiclassically the metric itself has a statistical
interpretation and we compute a lowerbound on its variance. (1 figure, at end
in encapsulated postscript - to locate use 'find figs')
