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arXiv · 1304.7612

Mind the Resonances: Final stages of accretion into bumpy black holes

Georgios Lukes-Gerakopoulos·George Contopoulos
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Abstract

In 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.

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Georgios Lukes-Gerakopoulos, George Contopoulos. 2013-04-29. Mind the Resonances: Final stages of accretion into bumpy black holes. https://doi.org/10.1088/1742-6596/453/1/012005

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