Dark photon superradiance quenched by dark matter

Abstract

Black-hole superradiance has been used to place very strong bounds on a variety of models of ultralight bosons such as axions, new light scalars, and dark photons. It is common lore to believe that superradiance bounds are broadly model independent and therefore pretty robust. In this work we show however that superradiance bounds on dark photons can be challenged by simple, compelling extensions of the minimal model. In particular, if the dark photon populates a larger dark sector and couples to dark fermions playing the role of dark matter, then superradiance bounds can easily be circumvented, depending on the mass and (dark) charge of the dark matter.

Probing ultralight isospin-violating mediators at GW170817

“…The presence of such interactions can potentially invalidate the BHSR constraints; see e.g., refs. [79,80] and also refs. [81][82][83] for BHSR constraints on self-interacting axions.…”