On the single versus the repetitive Penrose process in a Kerr black hole
Remo Ruffini, Mikalai Prakapenia, Hernando Quevedo, Shurui Zhang

TL;DR
This paper revisits the original Penrose process in Kerr black holes, demonstrating energy extraction efficiency and addressing issues with repetitive decay models that could violate energy conservation.
Contribution
It provides a detailed analysis of the simplest Penrose process, quantifies energy extraction at specific radii, and critiques repetitive decay models proposing a non-linear approach to conserve energy.
Findings
Single decay processes can extract energy as expected by Penrose.
Repetitive decay sequences may theoretically extract 100% of the BH's rotational energy.
A non-linear model is proposed to avoid energy conservation violations.
Abstract
Extracting the rotational energy from a Kerr black hole (BH) is one of the crucial topics in relativistic astrophysics. Here, we give special attention to the Penrose ballistic process based on the fission of a massive particle into two particles and , occurring in the ergosphere of a Kerr BH. Bardeen et al. indicated that for the process to occur, some additional "hydrodynamical forces or superstrong radiation reactions" were needed. Wald and Chandrasekhar further expanded this idea. This animosity convinced T. Piran and collaborators to move from a simple three-body system characterizing the original Penrose process to a many-body system. This many-body approach was further largely expanded by others, some questionable in their validity. Here, we return to the simplest original Penrose process and show that the solution of the equations of motion, imposing the…
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Taxonomy
TopicsAstrophysical Phenomena and Observations
