On the Penrose process for rotating black holes
Leon Heller

TL;DR
This paper critically examines proposed implementations of Penrose's energy extraction process from rotating black holes, revealing limitations and quantifying the maximum energy that can be extracted, which falls short of theoretical limits.
Contribution
It clarifies the conditions under which the Penrose process can occur and quantifies the maximum energy extractable from an extreme Kerr black hole.
Findings
Energy extraction is limited to about 9.7% for an extreme Kerr black hole.
Procedures with negative energy particles violate black hole area increase constraints.
Gradual exchange method can extract energy without decreasing the black hole to a Schwarzschild state.
Abstract
Penrose described a process that, in principle, could extract energy and angular momentum from a rotating black hole. Here we examine two procedures that were claimed to be capable of implementing the Penrose idea; both make use of a particle moving at the horizon. In one, the particle is swallowed, and in the other the particle and black hole gradually exchange energy and angular momentum. We show that if the particle has negative energy and negative angular momentum but no radial momentum both procedures violate the requirement that the area of a black hole not decrease. For the gradual exchange method, however, it appears that the Penrose process could proceed if the particle has positive energy and angular momentum, but nevertheless removes energy from the black hole. It does not, however, lead to a Schwarzschild black hole. For an extreme Kerr black hole it's mass decreases by at…
Peer Reviews
No public reviews on file for this paper yet. If you reviewed it on a platform where reviews are public (OpenReview, ICLR, NeurIPS, ICML), you can paste yours below so the community can read it here.
Videos
No videos yet. Explain this paper in a talk, walkthrough, or lecture? Add one.
Taxonomy
TopicsExperimental and Theoretical Physics Studies · Astrophysical Phenomena and Observations · Relativity and Gravitational Theory
