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In this work, we compute the precise late-time asymptotics for the scalar field in the interior of a non-static subextreme Kerr black hole, based on recent progress on deriving its precise asymptotics in the Kerr exterior region. This provides a new proof of the generic -inextendibility of the Kerr Cauchy horizon against scalar perturbations that is first shown by Luk–Sbierski (J. Func. Anal., 2016). The analogous results in Reissner–Nordström spacetimes are also discussed.

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