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