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• W3100419685 abstract "In this paper, by using the quasi-normal frequencies for non-rotating BTZ black hole derived by Cardos and Lemos, also via Bohr-Sommerfeld quantization for an adiabatic invariant, $I=int {dEover omega(E)}$, which $E$ is the energy of system and $omega(E)$ is vibrational frequency, we leads to an equally spaced mass spectrum. The result for the area of event horizon is $A_{n}=2pi sqrt{frac{nm hbar}{Lambda}}$ which is not equally spaced, in contrast with area spectrum of black hole in higher dimension." @default.
• W3100419685 created "2020-11-23" @default.
• W3100419685 creator A5008350239 @default.
• W3100419685 date "2004-02-26" @default.
• W3100419685 modified "2023-09-23" @default.
• W3100419685 title "Non-rotating BTZ black hole area spectrum from quasi-normal modes" @default.
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• W3100419685 doi "https://doi.org/10.1088/0264-9381/21/6/012" @default.
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