- qc / 0 41 21 17 v 3 1 2 Ja n 20 05 A quantum mass - spectrum of Kerr black hole : superstrings
نویسنده
چکیده
Using thermal quantization of geodesics confined under horizons and reasonable conjecture on massless modes, we evaluate quantum spectrum of Kerr black hole masses compatible with superstring symmetries.
منابع مشابه
ar X iv : g r - qc / 0 41 21 17 v 1 2 3 D ec 2 00 4 A quantum mass - spectrum of Kerr black hole : superstrings
Using thermal quantization of geodesics confined under horizons and reasonable conjecture on massless modes, we evaluate quantum spectrum of Kerr black hole masses compatible with superstring symmetries.
متن کاملr - qc / 0 41 21 17 v 2 4 J an 2 00 5 A quantum mass - spectrum of Kerr black hole : superstrings
Using thermal quantization of geodesics confined under horizons and reasonable conjecture on massless modes, we evaluate quantum spectrum of Kerr black hole masses compatible with superstring symmetries.
متن کاملar X iv : g r - qc / 0 01 20 66 v 2 3 1 Ja n 20 01 Spectrum of Charged Black Holes – The Big Fix Mechanism Revisited
Following an earlier suggestion of the authors(gr-qc/9607030), we use some basic properties of Euclidean black hole thermodynamics and the quantum mechanics of systems with periodic phase space coordinate to derive the discrete two-parameter area spectrum of generic charged spherically symmetric black holes in any dimension. For the Reissner-Nordstrom black hole we get A/4G¯ h = π(2n + p + 1), ...
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The massless scalar field in the higher-dimensional Kerr black hole (Myers-Perry solution with a single rotation axis) has been investigated. It has been shown that the field equation is separable in arbitrary dimensions. The quasi-normal modes of the scalar field have been searched in five dimensions using the continued fraction method. The numerical result shows the evidence for the stability...
متن کاملar X iv : g r - qc / 0 01 20 66 v 3 1 1 O ct 2 00 1 Spectrum of Charged Black Holes – The Big Fix Mechanism Revisited
Following an earlier suggestion of the authors (gr-qc/9607030), we use some basic properties of Euclidean black hole thermodynamics and the quantum mechanics of systems with periodic phase space coordinate to derive the discrete two-parameter area spectrum of generic charged spherically symmetric black holes in any dimension. For the Reissner-Nordstrom black hole we get A/4G¯ h = π(2n + p + 1),...
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