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• W2005487886 abstract "When a classical black hole is perturbed, its relaxation is governed by a set of quasinormal modes with complex frequencies $ensuremath{omega}={ensuremath{omega}}_{R}+i{ensuremath{omega}}_{I}$. We show that this behavior is the same as that of damped harmonic oscillators whose real frequencies are $({ensuremath{omega}}_{R}^{2}+{ensuremath{omega}}_{I}^{2}{)}^{1/2}$, rather than simply ${ensuremath{omega}}_{R}$. Since, for highly excited modes, ${ensuremath{omega}}_{I}ensuremath{gg}{ensuremath{omega}}_{R}$, this observation changes drastically the physical understanding of the black hole spectrum and forces a reexamination of various results in the literature. In particular, adapting a derivation by Hod, we find that the area of the horizon of a Schwarzschild black hole is quantized in units $ensuremath{Delta}A=8ensuremath{pi}{l}_{mathrm{Pl}}^{2}$, in contrast with the original result $ensuremath{Delta}A=4mathrm{log}(3){l}_{mathrm{Pl}}^{2}$." @default.
• W2005487886 created "2016-06-24" @default.
• W2005487886 creator A5053252993 @default.
• W2005487886 date "2008-04-08" @default.
• W2005487886 modified "2023-10-16" @default.
• W2005487886 title "Physical Interpretation of the Spectrum of Black Hole Quasinormal Modes" @default.
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• W2005487886 doi "https://doi.org/10.1103/physrevlett.100.141301" @default.
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