A bound on energy extraction (and hairiness) from superradiance
Carlos A. R. Herdeiro, Eugen Radu, Nuno M. Santos

TL;DR
This paper establishes a new theoretical upper bound of approximately 10% on the energy extractable from a black hole via superradiance, refining previous thermodynamic limits and aligning with numerical simulation results.
Contribution
The authors derive a conservative upper bound on superradiant energy extraction efficiency, improving understanding of black hole hairiness limits and guiding future numerical studies.
Findings
Maximum superradiance efficiency is about 10%.
Numerical simulations align with the derived bound.
Predicts outcomes for scalar and vector fields in superradiance.
Abstract
The possibility of mining the rotational energy from black holes has far--reaching implications. Such energy extraction could occur even for isolated black holes, if hypothetical ultralight bosonic particles exist in Nature, leading to a new equilibrium state a black hole with synchronised bosonic hair whose lifetime could exceed the age of the Universe. A natural question is then: for an isolated black hole and at maximal efficiency, how large is the energy fraction that can be extracted from a Kerr black hole by the superradiant growth of the dominant mode? In other words, how hairy can the resulting black hole become? A thermodynamical bound for the total superradiance efficiency, (as a fraction of the initial black hole mass), has long been known, from the area law. However, numerical simulations exhibiting the growth of the dominant mode…
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