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Motivated by the recent work on a new physical interpretation of quasinormalmodes by Maggiore, we utilize this new proposal to the interesting case of Kerrblack hole. In particular, by modifying Hod's idea, the resulting black holehorizon area is quantized and the resulting area quantum is in full agreementwith Bekenstein's result. Furthermore, in an attempt to show that the areaspectrum is equally spaced, we follow Kunstatter's method. We propose a newinterpretation as a result of Maggiore's idea, for the frequency that appearsin the adiabatic invariant of a black hole. The derived area spectrum issimilar to that of the quantum-corrected Kerr black hole but it is not equallyspaced.

Area spectrum of rotating black holes via the new interpretation of quasinormal modes