Mind the Resonances: Final stages of accretion into bumpy black holes [PDF]
Georgios Lukes-Gerakopoulos, George ContopoulosIn this article we discuss a possible way of testing the Kerr black hole hypothesis by taking advantage of phenomena correlated with chaotic motion in the final stages of an accretion disk around a bumpy black hole. We anticipate that these phenomena should have an imprint in the electromagnetic spectrum coming from the accretion disk.View original: http://arxiv.org/abs/1304.7612
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