2026-07-072026-07-07http://salesiana.dossiersoluciones.com/handle/123456789/34651Motivated by novel results in the theory of black-hole quantization, we study {\it analytically} the quasinormal modes (QNM) of ({\it rotating}) Kerr black holes. The black-hole oscillation frequencies tend to the asymptotic value $ω_n=mΩ+i2πT_{BH}n$ in the $n \to \infty$ limit. This simple formula is in agreement with Bohr's correspondence principle. Possible implications of this result to the area spectrum of quantum black holes are discussed.4 pagesGeneral Relativity and Quantum CosmologyAstrophysicsCondensed MatterHigh Energy Physics - TheoryQuantum Physicstext