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• W2014053742 abstract "A new analytic method for the determination of quasinormal oscillations of a black hole is presented. It is based on a connection between the quasinormal modes and the bound states of the inverted black-hole potentials. With use of this method, the quasinormal frequencies of a Schwarzschild, a Reissner-Nordstrom, and a slowly rotating Kerr black hole are determined in the eikonal approximation, Moreover, we provide evidence for the stability of an extreme Kerr black hole." @default.
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• W2014053742 date "1984-04-16" @default.
• W2014053742 modified "2023-09-25" @default.
• W2014053742 title "Oscillations of a Black Hole" @default.
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• W2014053742 doi "https://doi.org/10.1103/physrevlett.52.1361" @default.
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