\begin{document}$a\rightarrow 0$\end{document} and the extremal limit \begin{document}$a\rightarrow M$\end{document}. Upon the Kerr/CFT correspondence, a central charge \begin{document}$c=12 M r_+$\end{document} can be associated with an arbitrary Kerr black hole. Moreover, the microstates of the Kerr black hole can be identified with the quantum states of this scalar field. From this identification, the number of microstates of the Kerr black hole can be counted, yielding the Bekenstein-Hawking area law for the entropy."> Microscopic states of Kerr black holes from boundary-bulk correspondence -
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