Can quasi-circular mergers of charged black holes produce extremal black holes?

TL;DR

This paper explores whether quasi-circular mergers of charged black holes can produce extremal or naked singularity remnants, combining theoretical modeling with numerical simulations to assess the limits of black hole charge and spin.

Contribution

It extends a theoretical model to charged black hole mergers and validates it with simulations, showing extremal remnants are possible without violating cosmic censorship.

Findings

Naked singularities do not form from non-spinning charged mergers.

Remnants can approach the extremal limit arbitrarily closely.

Model agrees with simulations at the percent level.

Abstract

In contrast to energy and angular momentum, electric charge is conserved in mergers of charged black holes. This opens up the possibility for the remnant to have Kerr-Newman parameter $\chi^{2} + \lambda^{2}$ greater than 1 (with $\chi$ and $\lambda$ being the black hole dimensionless spin and dimensionless charge, respectively), which is forbidden by the cosmic censorship conjecture. In this paper, we investigate whether a naked singularity can form in quasi-circular mergers of charged binary black holes. We extend a theoretical model to estimate the final properties of the remnant left by quasicircular mergers of binary black holes to the charged case. We validate the model with numerical-relativity simulations, finding agreement at the percent level. We then use our theoretical model to argue that while naked singularities cannot form following quasi-circular mergers of non-spinning charged binary black holes, it is possible to produce remnants that are arbitrarily close to the extremal limit.