Trapping of waves and null geodesics for rotating black holes
We present dynamical properties of linear waves and null geodesics valid for Kerr and Kerr-de Sitter black holes and their stationary perturbations. The two are intimately linked by the geometric optics approximation. For the null geodesic flow the key property is the r-normal hyperbolicity of the t...
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Format: | Article |
Language: | English |
Published: |
American Physical Society,
2014-02-07T20:43:50Z.
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Subjects: | |
Online Access: | Get fulltext |