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arXiv · 2412.01881

High-energy interactions of charged black holes in full general relativity II: Near-extremal merger remnants and universality with the irreducible mass

M A. M. Smith·Vasileios Paschalidis·Gabriele Bozzola
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Abstract

In a previous paper, arXiv:2411.11960 [gr-qc], we initiated a study of high-energy interactions of charged binary black holes near the scattering threshold, focusing on zoom-whirl orbits. In this second paper in our series, we focus on merger remnant properties and energetics with new simulations of equal-mass, equal-charge, nonspinning binary black holes with variable impact parameter. We find near-extremal merger remnants with Kerr-Newman parameter reaching $\Upsilon_f = 0.97$, and observe that the maximum $\Upsilon_f$ increases monotonically with $\lambda$ for a fixed initial Lorentz factor. We find that binaries with larger $\lambda$ radiate less total energy despite having stronger electromagnetic emission. The maximum energy radiated by a binary in our study is $31\%$ of its gravitational mass. Increasing $\lambda$ has little effect on the maximum angular momentum radiated, which was $\approx 72\%$ of the spacetime total angular momentum for each $\lambda$ explored here. Lastly, we provide additional evidence for the universality with the irreducible mass that we discovered in arXiv:2411.11960 [gr-qc]. The black hole horizon areal radius determines a fundamental, gauge-invariant length scale governing BH interactions near the scattering threshold.

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M A. M. Smith, Vasileios Paschalidis, Gabriele Bozzola. 2024-12-02. High-energy interactions of charged black holes in full general relativity II: Near-extremal merger remnants and universality with the irreducible mass. https://arxiv.org/abs/2412.01881

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