Geodesic structure of a rotating regular black hole

被引：4

作者：

Bautista-Olvera, Brandon ^{[1
]}

Degollado, Juan Carlos ^{[1
]}

German, Gabriel ^{[1
]}

机构：

[1] Univ Nacl Autonoma Mexico, Inst Ciencias Fis, Ave Univ S-N,Postal 48-3, Cuernavaca 62210, Morelos, Mexico

来源：

GENERAL RELATIVITY AND GRAVITATION | 2023年 / 55卷 / 05期

基金：

欧盟地平线“2020”;

关键词：

Rotating black holes; Hayward black hole; Geodesics;

D O I：

10.1007/s10714-023-03114-7

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

We examine the dynamics of particles around a rotating regular black hole. In particular we focus on the effects of the characteristic length parameter of the spinning black hole on the motion of the particles by solving the equation of orbital motion. We have found that there is a fourth constant of motion that determines the dynamics of orbits out the equatorial plane similar as in the Kerr black hole. Through detailed analyses of the corresponding effective potentials for massive particles the possible orbits are numerically simulated. A comparison with the trajectories in a Kerr spacetime shows that the differences appear when the black holes rotate slowly for large values of the characteristic length parameter.

引用

页数：26

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