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2019

Ultralight boson cloud depletion in binary systems

Berti, Emanuele, Brito, Richard, Macedo, Caio F. B. et al.

Understand

Ultralight scalars can extract rotational energy from astrophysical black holes through superradiant instabilities, forming macroscopic boson clouds.

This process is most efficient when the Compton wavelength of the boson is comparable to the size of the black hole horizon, i.e.
when the "gravitational fine structure constant" $\alpha\equiv G \mu M/\hbar c\sim 1$.
If the black hole/cloud system is in a binary, tidal perturbations from the companion can produce resonant transitions between the energy levels of the cloud, depleting it by an amount that depends on the nature of the transition and on the parameters of the binary.