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The final (close to the singularity) dynamical behavior of the metric insideblack holes with massive charged scalar or vector hair is analyzed for generalanisotropic and inhomogeneous initial conditions. These solutions are relevantto a holographic realization of superconductivity. It is shown that thedynamics falls within the scope of the "cosmological billiard" description andthat in both cases, the corresponding hyperbolic billiard region has infinitevolume so that the system ultimately settles down to a final Kasner regime. Formassive vector hair, the conclusion holds because the longitudinal mode playsthe same role as a scalar field. There exists, however, a measure-zero subsetof solutions characterized by vanishing longitudinal modes that exhibit achaotic behavior with an infinite number of BKL oscillations as one goes to thesingularity.

The final Kasner regime inside black holes with scalar or vector hair