Gravitational and electromagnetic radiation from binary black holes with electric and magnetic charges: Circular orbits on a cone

TL;DR

This paper derives equations for dyonic black hole binaries with electric and magnetic charges, analyzing their orbits, radiation emissions, and merger times, revealing how charges influence binary evolution and potential observational signatures.

Contribution

It introduces a Newtonian framework including radiation reaction to study dyonic black hole binaries with electric and magnetic charges, providing new insights into their dynamics and emissions.

Findings

Electric and magnetic charges suppress merger times.

Radiation emission rates depend on charge configurations.

Orbits can be static on a cone with specific charge conditions.

Abstract

We derive the equations of motion of dyonic black hole binaries with electric and magnetic charges and explore features of static orbits. By using a Newtonian method with the inclusion of radiation reaction, we calculate the total emission rate of energy and angular momentum due to gravitational radiation and electromagnetic radiation for circular orbits. Moreover, we obtain the evolutions of orbits and calculate merger times of dyonic binaries. We show that electric and magnetic charges significantly suppress the merger times of dyonic binaries. Our results provide rich information about dyonic binaries and can be used to test black holes with magnetic charges.