Mergers of Charged Black Holes: Gravitational Wave Events, Short Gamma-Ray Bursts, and Fast Radio Bursts

TL;DR

This paper proposes a model where charged black hole mergers produce electromagnetic signals like gamma-ray bursts and fast radio bursts, linking gravitational wave events with these high-energy phenomena and suggesting new ways to measure black hole charges.

Contribution

It introduces a novel model connecting black hole charges to observable electromagnetic counterparts during mergers, explaining potential coincident signals like GRBs and FRBs.

Findings

Charged black hole mergers can generate detectable gamma-ray bursts.

Magnetospheric activity during mergers may produce fast radio bursts.

The model explains the possible association of GW 150914 with a short GRB.

Abstract

The discoveries of GW 150914, GW 151226, and LVT 151012 suggest that double black hole (BH-BH) mergers are common in the universe. If at least one of the two merging black holes carries certain amount of charge, possibly retained by a rotating magnetosphere, the inspiral of a BH-BH system would drive a global magnetic dipole normal to the orbital plane. The rapidly evolving magnetic moment during the merging process would drive a Poynting flux with an increasing wind power. The magnetospheric activities during the final phase of the merger would make a fast radio burst (FRB) if the BH charge can be as large as a factor of $\hat q \sim (10^{-9}-10^{-8})$ of the critical charge $Q_c$ of the BH. At large radii, dissipation of the Poynting flux energy in the outflow would power a short duration high-energy transient, which would appear as a detectable short-duration gamma-ray burst (GRB) if the charge can be as large as $\hat q \sim (10^{-5}-10^{-4})$. The putative short GRB coincident with GW 150914 recorded by Fermi GBM may be interpreted with this model. Future joint GW/GRB/FRB searches would lead to a measurement or place a constraint on the charges carried by isolate black holes.