Weak cosmic censorship, dyonic Kerr-Newman black holes and Dirac fields

TL;DR

This paper extends previous work on weak cosmic censorship by analyzing how extremal dyonic Kerr-Newman black holes interact with massive Dirac fields, showing that such interactions can potentially violate the conjecture without contradiction.

Contribution

It generalizes the analysis to charged, rotating black holes with massive Dirac fields, and clarifies the role of the energy-momentum tensor and superradiance in these processes.

Findings

Dirac fields can convert extremal black holes into naked singularities.

The Dirac energy-momentum tensor does not satisfy the null energy condition.

The superradiant frequency range for Dirac fields partially overlaps with that of scalar fields.

Abstract

It was investigated recently, with the aim of testing the weak cosmic censorship conjecture, whether an extremal Kerr black hole can be converted into a naked singularity by interaction with a massless classical Dirac test field, and it was found that this is possible. We generalize this result to electrically and magnetically charged rotating extremal black holes (i.e. extremal dyonic Kerr-Newman black holes) and massive Dirac test fields, allowing magnetically or electrically uncharged or nonrotating black holes and the massless Dirac field as special cases. We show that the possibility of the conversion is a direct consequence of the fact that the Einstein-Hilbert energy-momentum tensor of the classical Dirac field does not satisfy the null energy condition, and is therefore not in contradiction with the weak cosmic censorship conjecture. We give a derivation of the absence of superradiance of the Dirac field without making use of the complete separability of the Dirac equation in dyonic Kerr-Newman background, and we determine the range of superradiant frequencies of the scalar field. The range of frequencies of the Dirac field that can be used to convert a black hole into a naked singularity partially coincides with the superradiant range of the scalar field. We apply horizon-penetrating coordinates, as our arguments involve calculating quantities at the event horizon. We describe the separation of variables for the Dirac equation in these coordinates, although we mostly avoid using it.