Mass Inflation in a Rotating Charged Black Hole

Abstract

The structure of the Cauchy horizon of a charged rotating black hole is analyzed under the combined effect of an ingoing and outgoing flux of gravitational waves. In particular, by means of an axisymmetric realization of the Ori model, the growth of the mass parameter near the Cauchy horizon is studied in the slow rotation approximation. It is shown that the mass-parameter inflates, while the angular momentum per unit mass deflates, but initial deviations from spherical symmetry survive.

arXiv comment6 pages, REVTex, one uuencoded figure

References in corpus (4)

• Black hole singularities: a numerical approach
• Non-linear instability of Kerr-type Cauchy horizons
• Structure of the Spherical Black Hole Interior
• Structure of the Inner Singularity of a Spherical Black Hole

Cited by in corpus (8)

• Cosmology of the Planck Era from a Renormalization Group for Quantum Gravity
• Scalar Wave Falloff in Asymptotically Anti-de Sitter Backgrounds
• Quantum Gravity effects near the null black hole singularity
• Spherical Black Holes cannot Support Scalar Hair
• The late-time singularity inside non-spherical black holes
• Hairs on the cosmological horizon
• The interior structure of slowly rotating black holes
• Stability of degenerate Cauchy horizons in black hole spacetimes