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Black hole superradiant instability from ultralight spin-2 fields · Around

2020

Black hole superradiant instability from ultralight spin-2 fields

Brito, Richard, Grillo, Sara, Pani, Paolo

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Ultralight bosonic fields are compelling dark-matter candidates and arise in a variety of beyond-Standard-Model scenarios.

These fields can tap energy and angular momentum from spinning black holes through superradiant instabilities, during which a macroscopic bosonic condensate develops around the black hole.
Striking features of this phenomenon include gaps in the spin-mass distribution of astrophysical black holes and a continuous gravitational-wave~(GW) signal emitted by the condensate.
So far these processes have been studied in great detail for scalar fields and, more recently, for vector fields.

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