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Resumming Kerr Quasinormal-Mode Frequencies: Accuracy and Breakdown Near Extremality
Kerr black-hole quasinormal modes are usually computed with numerical methods, but analytic approximations remain useful for identifying the physics that controls different parts of the spectrum. In this paper, we ask whether the divergent, high-order Wentzel-Kramers-Brillouin (WKB) expansion about
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