Effects of Two Quantum Correction Parameters on Chaotic Dynamics of Particles near Renormalized Group Improved Schwarzschild Black Holes

Author:

Lu Junjie12,Wu Xin12ORCID

Affiliation:

1. School of Mathematics, Physics and Statistics, Shanghai University of Engineering Science, Shanghai 201620, China

2. Center of Application and Research of Computational Physics, Shanghai University of Engineering Science, Shanghai 201620, China

Abstract

A renormalized group improved Schwarzschild black hole spacetime contains two quantum correction parameters. One parameter γ represents the identification of cutoff of the distance scale, and another parameter Ω stems from nonperturbative renormalization group theory. The two parameters are constrained by the data from the shadow of M87* central black hole. The dynamics of electrically charged test particles around the black hole are integrable. However, when the black hole is immersed in an external asymptotically uniform magnetic field, the dynamics are not integrable and may allow for the occurrence of chaos. Employing an explicit symplectic integrator, we survey the contributions of the two parameters to the chaotic dynamical behavior. It is found that a small change of the parameter γ constrained by the shadow of M87* black hole has an almost negligible effect on the dynamical transition of particles from order to chaos. However, a small decrease in the parameter Ω leads to an enhancement in the strength of chaos from the global phase space structure. A theoretical interpretation is given to the different contributions. The term with the parameter Ω dominates the term with the parameter γ, even if the two parameters have same values. In particular, the parameter Ω acts as a repulsive force, and its decrease means a weakening of the repulsive force or equivalently enhancing the attractive force from the black hole. On the other hand, there is a positive Lyapunov exponent that is universally given by the surface gravity of the black hole when Ω≥0 is small and the external magnetic field vanishes. In this case, the horizon would influence chaotic behavior in the motion of charged particles around the black hole surrounded by the external magnetic field. This point can explain why a smaller value of the renormalization group parameter would much easily induce chaos than a larger value.

Funder

National Natural Science Foundation of China

Publisher

MDPI AG

Reference39 articles.

1. Akiyama, K. et al. [Event Horizon Telescope Collaboration] (2019). First M87 event horizon telescope results. I. The shadow of the supermassive black hole. Astrophys. J. Lett., 875, L1.

2. Akiyama, K. et al. [Event Horizon Telescope Collaboration] (2022). First Sagittarius A* Event Horizon Telescope results. I. The shadow of the supermassive black hole in the center of the Milky Way. Astrophys. J. Lett., 930, L12.

3. Beyond Einstein gravity: A survey of gravitational theories for cosmology and astrophysics;Faraoni;Fundam. Theor. Phys.,2010

4. f(R) theories of gravity;Sotiriou;Rev. Mod. Phys.,2010

5. Modified gravity and cosmology;Cliftona;Phys. Rep.,2012

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