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Black hole superradiance with dark matter accretion

Lam Hui
(
- Columbia U.
)
,
Y.T. Albert Law
(
- Columbia U. and
- Harvard U.
)
,
Luca Santoni
(
- ICTP, Trieste
)
,
Guanhao Sun
(
- Columbia U.
)
,
Giovanni Maria Tomaselli
(
- U. Amsterdam, GRAPPA
)

Aug 12, 2022

50 pages

Published in:

Phys.Rev.D 107 (2023) 10, 104018

Published: May 8, 2023

e-Print:

2208.06408 [gr-qc]

DOI:

10.1103/PhysRevD.107.104018 (publication)

View in:

ADS Abstract Service

reference search34 citations

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Abstract: (APS)

Studies of black hole superradiance often focus on the growth of a cloud in isolation, accompanied by the spin-down of the black hole. In this paper, we consider the additional effect of the accretion of matter and angular momentum from the environment. We show that, in many cases, the black hole evolves by drifting along the superradiance threshold, in which case the evolution of its parameters can be described analytically or semianalytically. We quantify the conditions under which accretion can serve as a mechanism to increase the cloud-to-black hole mass ratio, beyond the standard maximum of about 10%. This occurs by a process we call oversuperradiance, whereby accretion effectively feeds the superradiance cloud, by way of the black hole. We give two explicit examples: accretion from a vortex expected in wave dark matter and accretion from a baryonic disk. In the former case, we estimate the accretion rate by using an analytical fit to the asymptotic behavior of the confluent Heun function. Level transition, whereby one cloud level grows while the other shrinks, can be understood in a similar way.

Note:

30+21 pages, 14 figures

matter: accretion
black hole: spin
superradiance
cloud
dark matter
vortex
asymptotic behavior
mass ratio
angular momentum
baryon: matter

References(61)

Figures(14)

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