Towards a Semiclassical Seismology of Black Holes

Details Towards a Semiclassical Seismology of Black Holes Towards a Semiclassical Seismology of Black Holes

1993-12-15

arxiv.org/abs/hep-th/9312136v1

Phys.Rev.D50:3954-3960,1994

Physics

High Energy Physics

High Energy Physics - Theory

21 pages, 1 figure, MIT CTP#2226

Scientific paper

10.1103/PhysRevD.50.3954

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')

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