M R Setare 2004 Class. Quantum Grav. 21 1453 doi:10.1088/0264-9381/21/6/012
Non-rotating BTZ black hole area spectrum from quasi-normal modes
M R Setare
Show affiliationsIn this paper, by using the quasi-normal frequencies for a non-rotating BTZ black hole derived by Cardos and Lemos, also via Bohr–Sommerfeld quantization for an adiabatic invariant, 
, where E is the energy of system and ω(E) is vibrational frequency, we are led to an equally spaced mass spectrum. The result for the area of the event horizon is 
which is not equally spaced, in contrast with the area spectrum of a black hole in higher dimension.
- PACS
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04.70.Dy Quantum aspects of black holes, evaporation, thermodynamics
- MSC
- Subjects
- Dates
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Issue 6 (21 March 2004)
Received 13 August 2003
Published 23 February 2004
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Non-rotating BTZ black hole area spectrum from quasi-normal modes
M R Setare 2004 Class. Quantum Grav. 21 1453
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