For spherically symmetric Einstein-Maxwell-scalar field solutions, higher-order derivatives of the scalar field decay along the event horizon, implying generic mass inflation.
Late-time tails and mode coupling of linear waves on Kerr spacetimes
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Late-time tails and mass inflation for the spherically symmetric Einstein-Maxwell-scalar field system
For spherically symmetric Einstein-Maxwell-scalar field solutions, higher-order derivatives of the scalar field decay along the event horizon, implying generic mass inflation.