Abstract
Bekenstein and others propose that the black hole area spectrum is discrete and equally spaced. We implement Kunstatter's method to derive the area spectrum for near extremal black 3-branes. The area spectrum of the event horizon is discrete but not equally spaced.
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Setare, M.R. Area Spectrum of Near Extremal Black Branes from Quasi-Normal Modes. Int J Theor Phys 44, 1365–1371 (2005). https://doi.org/10.1007/s10773-005-4771-1
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DOI: https://doi.org/10.1007/s10773-005-4771-1