Tidal effects around higher-dimensional black holes
Richard Brito, Vitor Cardoso, Paolo Pani

TL;DR
This paper investigates tidal effects around higher-dimensional black holes, demonstrating that in dimensions greater than five, superradiance causes orbiting bodies to gain energy and spiral outward, supporting the conjecture of stronger tidal acceleration in higher dimensions.
Contribution
The study provides numerical and analytical evidence that tidal acceleration via superradiance dominates in higher-dimensional black holes, confirming the conjecture and revealing the occurrence of floating orbits.
Findings
Superradiance exceeds energy radiated to infinity in >5D.
Moons can outspiral due to tidal acceleration.
Floating orbits occur at specific frequencies.
Abstract
In four-dimensional spacetime, moons around black holes generate low-amplitude tides, and the energy extracted from the hole's rotation is always smaller than the gravitational radiation lost to infinity. Thus, moons orbiting a black hole inspiral and eventually merge. However, it has been conjectured that in higher-dimensional spacetimes orbiting bodies generate much stronger tides, which backreact by tidally accelerating the body outwards. This effect, analogous to the tidal acceleration experienced by the Earth-Moon system, would determine the evolution of the binary. Here, we put this conjecture to the test, by studying matter coupled to a massless scalar field in orbit around a singly-spinning rotating black hole in higher dimensions. We show that in dimensions larger than five the energy extracted from the black hole through superradiance is larger than the energy carried out to…
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