Chaotic motion of particle in regular black hole supported by Galactic halo

TL;DR

This study explores how dark matter halos influence chaotic motion of particles around regular black holes, revealing that halos significantly induce chaos and could help detect dark matter properties through astrophysical observations.

Contribution

It demonstrates the role of galactic halos in driving chaos in regular black hole environments using Poincaré sections and Lyapunov exponents, highlighting a new method to probe dark matter.

Findings

Galactic halos significantly induce chaos in particle motion.

Chaos increases with the halo scale parameter $a$.

Dark matter halos leave observable signatures in particle dynamics.

Abstract

We investigate the chaotic dynamics of the massless test particles moving in the regular black hole supported by a Dehnen-type dark matter halo. By limiting the particle within a external harmonic potential, we employ Poincar\'e sections and Lyapunov exponents as diagnostic tools and analyze the transition from regular to chaotic motion as the halo scale parameter $a$ increase. These findings indicate that the galactic halo acts as a primary driver of chaos in this regular black hole geometry, significantly distorting the phase space structure near the potential center, acting as a primary driver of chaos. Crucially, our results elucidate the distinct imprint of dark matter halos on particle dynamics, suggesting that observing such chaotic signatures in astrophysical systems could provide a novel method for detecting and constraining the properties of dark matter in future observations.