The covariant loop-quantum-gravity black hole exhibits mass inflation at its Cauchy horizon, and in de Sitter spacetime its quasinormal modes satisfy the Strong Cosmic Censorship bound beta < 1/2.
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Mass inflation and strong cosmic censorship conjecture in the covariant quantum black hole
The covariant loop-quantum-gravity black hole exhibits mass inflation at its Cauchy horizon, and in de Sitter spacetime its quasinormal modes satisfy the Strong Cosmic Censorship bound beta < 1/2.