Regular black hole's impact on the gravitational waveforms from periodic orbits

TL;DR

This paper explores how magnetic charge in regular black holes influences orbital dynamics and gravitational waveforms from extreme mass ratio inspirals, revealing potential observational signatures of such black holes.

Contribution

It introduces a semi-analytical model linking magnetic charge effects to orbital behavior and gravitational waveforms in regular black hole spacetimes.

Findings

Magnetic charge reduces the radii of MBOs and ISCOs.

Charge significantly alters zoom-whirl orbital dynamics.

Waveform structures are notably affected by the black hole's magnetic charge.

Abstract

In this paper, we investigate periodic orbits exhibiting zoom-whirl behavior around a magnetically charged black hole (MCBH) within the framework of the regular black hole. We examine how the magnetic charge influences orbital dynamics by modifying the background spacetime geometry, thereby affecting the energy and angular momentum of particles. In particular, we calculate the radii of the marginally bound orbits (MBOs) and innermost stable circular orbits (ISCOs), demonstrating that the magnetic charge parameter reduces both radii. This provides valuable insight into the role of the charge parameter in shaping orbital behavior and altering spacetime geometry. We model the complex motion of a stellar-mass object as a timelike particle, inspiraling into a supermassive black hole (SMBH) in the MCBH background, with its trajectory described using periodic geodesic orbits. Based on this analysis of such periodic orbits, we further analyze the gravitational waveforms generated by extreme mass ratio inspirals (EMRIs), in which the SMBH's spacetime dominates the dynamics of the stellar-mass object. By combining particle trajectory analysis with waveform modeling in a semi-analytical approach, we show that the charge parameter significantly alters the zoom-whirl orbital dynamics and induces notable changes in the waveform structure. These results illustrate that future gravitational wave (GW) observations may constrain the properties of MCBHs, thereby deepening our understanding of the gravitational imprint of regular black holes.