The inner Cauchy horizon of axisymmetric and stationary black holes with surrounding matter in Einstein-Maxwell theory: study in terms of soliton methods

TL;DR

This paper employs soliton methods to analyze the interior of axisymmetric, charged black holes with matter, revealing a universal relation between horizon areas and conditions for a regular inner Cauchy horizon.

Contribution

It introduces a novel application of soliton techniques to Einstein-Maxwell black holes with matter, deriving explicit relations for the inner horizon and a universal area-charge-angular momentum relation.

Findings

Existence of a regular inner Cauchy horizon under certain conditions.

Explicit relation between inner and outer horizon metrics.

Universal relation $(8 ext{π}J)^2 + (4 ext{π}Q^2)^2 = A^+ A^-$.

Abstract

We use soliton methods in order to investigate the interior electrovacuum region of axisymmetric and stationary, electrically charged black holes with arbitrary surrounding matter in Einstein-Maxwell theory. These methods can be applied since the Einstein-Maxwell vacuum equations permit the formulation in terms of the integrability condition of an associated linear matrix problem. We find that there always exists a regular inner Cauchy horizon inside the black hole, provided the angular momentum $J$ and charge $Q$ of the black hole do not vanish simultaneously. Moreover, the soliton methods provide us with an explicit relation for the metric on the inner Cauchy horizon in terms of that on the event horizon. In addition, our analysis reveals the remarkable universal relation $(8\pi J)^2+(4\pi Q^2)^2=A^+ A^-$, where $A^+$ and $A^-$ denote the reas of event and inner Cauchy horizon respectively.