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October 20, 2025Open Access

Cauchy Horizon (In)Stability of Regular Black Holes

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Cauchy horizons in certain regular black holes demonstrate stability, differing from typical mass-inflation behavior.
The power-law growth of the mass function was shown to be generic for the Hayward solution and others.
Bardeen geometry and non-singular collapse models reveal unique mass dynamics at the Cauchy horizon.
The Misner-Sharp mass remains comparable to the black hole mass, with logarithmic growth highlighting distinct properties.

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This analysis demonstrates the stability of Cauchy horizons in regular black holes, suggesting novel implications in gravitational theories.

Bonanno et al. (2025) studied this question.

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This analysis demonstrates the stability of Cauchy horizons in regular black holes, suggesting novel implications in gravitational theories.