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Kerr-Newman black holes with stationary charged scalar clouds (1406.1179v2)
Published 4 Jun 2014 in gr-qc, astro-ph.HE, and hep-th
Abstract: It is shown that Kerr-Newman black holes can support linear charged scalar fields in their exterior regions. To that end, we solve analytically the Klein-Gordon wave equation for a stationary charged massive scalar field in the background of a near-extremal Kerr-Newman black hole. In particular, we derive a simple analytical formula which describes the physical properties of these stationary bound-state resonances of the charged massive scalar fields in the Kerr-Newman black-hole spacetime.
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