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2022

Superradiant Production of Heavy Dark Matter from Primordial Black Holes

Bernal, Nicolás, Perez-Gonzalez, Yuber F., Xu, Yong

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Rotating black holes (BHs) can efficiently transfer energy to the surrounding environment via superradiance.

In particular, when the Compton length of a particle is comparable to the gravitational radius of a BH, the particle's occupation number can be exponentially amplified.
In this work, we investigate the effect of the primordial-black-hole (PBH) superradiant instabilities on the generation of heavy bosonic dark matter (DM) with mass above $\sim$ 1 TeV.
Additionally, we analyze its interplay with other purely gravitational and therefore unavoidable DM production mechanisms such as Hawking emission and the ultraviolet freeze-in.

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