Article ID Journal Published Year Pages File Type
8191092 Physics Letters B 2012 4 Pages PDF
Abstract
The instability of rotating Kerr black holes due to massive scalar perturbations is investigated. It is well known that a bosonic field impinging on a Kerr black hole can be amplified as it scatters off the hole. This superradiant scattering occurs for frequencies in the range ω
Related Topics
Physical Sciences and Engineering Physics and Astronomy Nuclear and High Energy Physics
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