A perturbative model claims the inner horizon of a Reissner-Nordström black hole collapses inward under a massive scalar field, making the geometry tend toward Schwarzschild.
Change of relativistic collapse into anticollapse and kine matics of a charged sphere
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Nonlinear Dynamics of the Inner Horizon in Reissner-Nordstr\"om Black Holes: Insights into Mass Inflation
A perturbative model claims the inner horizon of a Reissner-Nordström black hole collapses inward under a massive scalar field, making the geometry tend toward Schwarzschild.