Repetitive Penrose process in Konoplya-Zhidenko rotating non-Kerr black holes

Fuente: arXiv
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Main Authors: Zeng, Xiao-Xiong, Su, Dong-Ping, Wang, Ke
Format: Preprint
Published: 2026
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author Zeng, Xiao-Xiong
Su, Dong-Ping
Wang, Ke
author_facet Zeng, Xiao-Xiong
Su, Dong-Ping
Wang, Ke
contents This paper investigates the repetitive Penrose process in Konoplya-Zhidenko rotating non-Kerr black hole, exploring the influence of the deformation parameter on the repetitive Penrose process. After a brief review of the Konoplya-Zhidenko rotating non-Kerr black hole, we study the fundamental equations of the Penrose process in this spacetime, examine the iterative stopping conditions required for the repetitive Penrose process, and obtain the corresponding numerical results. It is concluded that, in addition to previously observed phenomena, under the same decay radius, a larger initial dimensionless deformation parameter $\hatη$ leads to greater values of the energy return on investment and energy utilization efficiency, particularly at higher decay radii. Furthermore, a smaller initial $\hatη$ results in a larger maximum value of the energy return on investment. For energy utilization efficiency, the initial $\hatη$ should take an intermediate value to maximize its peak. Additionally, we find that a larger initial $\hatη$ corresponds to a smaller maximum value of the extracted energy.
format Preprint
id arxiv_https___arxiv_org_abs_2603_16147
institution arXiv
publishDate 2026
record_format arxiv
spellingShingle Repetitive Penrose process in Konoplya-Zhidenko rotating non-Kerr black holes
Zeng, Xiao-Xiong
Su, Dong-Ping
Wang, Ke
General Relativity and Quantum Cosmology
This paper investigates the repetitive Penrose process in Konoplya-Zhidenko rotating non-Kerr black hole, exploring the influence of the deformation parameter on the repetitive Penrose process. After a brief review of the Konoplya-Zhidenko rotating non-Kerr black hole, we study the fundamental equations of the Penrose process in this spacetime, examine the iterative stopping conditions required for the repetitive Penrose process, and obtain the corresponding numerical results. It is concluded that, in addition to previously observed phenomena, under the same decay radius, a larger initial dimensionless deformation parameter $\hatη$ leads to greater values of the energy return on investment and energy utilization efficiency, particularly at higher decay radii. Furthermore, a smaller initial $\hatη$ results in a larger maximum value of the energy return on investment. For energy utilization efficiency, the initial $\hatη$ should take an intermediate value to maximize its peak. Additionally, we find that a larger initial $\hatη$ corresponds to a smaller maximum value of the extracted energy.
title Repetitive Penrose process in Konoplya-Zhidenko rotating non-Kerr black holes
topic General Relativity and Quantum Cosmology
url https://arxiv.org/abs/2603.16147