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Massive charged scalar field in the Kerr-Newman background: Quasinormal modes, late-time tails and stability
So far analysis of the quasinormal spectrum of a massive charged scalar field in the black hole background has been limited by the regime of small $\ensuremath{\mu}M$ and $qQ$, where $\ensuremath{\mu}$, $q$ $(M,Q)$ are mass and charge of the field (black hole). Here we shall present a comprehensive picture of …