Ring formation from black hole superradiance through repeated particle production on bound orbits
Zhen-Hong Lyu, Rong-Gen Cai, Zong-Kuan Guo, Jian-Feng He, Jing Liu
TL;DR
BH superradiance converts rotational energy into a growing ultralight-boson cloud with a hydrogenlike spectrum. Introducing a second axion coupled by $V_{ m int}=\frac{1}{2}\lambda\phi\chi^2$ reveals a novel mechanism where resonant production of a heavier field $\chi$ occurs primarily at the cloud’s toroidal peak, and bound $\chi$ particles on quasi-circular orbits undergo repeated resonance crossings, leading to staircase amplification and the formation of a stable ring embedded in the cloud. The ring-saturation dynamics show that the final ring mass is set by the hierarchy $\mu_\phi\ll\mu_\chi$, giving $\frac{M_\chi}{M_{\rm cloud}}\approx 0.6\left(\frac{\mu_\phi}{\mu_\chi}\right)^2$, and that backreaction halts growth. The work highlights a bound-state production channel with potential observational consequences in gravitational waves and binary dynamics, distinct from scenarios with quartic couplings which instead produce an escaping flux.
Abstract
Ultralight bosonic fields around a rotating black hole can extract energy and angular momentum through the superradiant instability and form a dense cloud. We investigate the scenario involving two scalar fields, $φ$ and $χ$, with a coupling term $\frac{1}{2}λφχ^2$, which is motivated by the multiple-axion framework. The ultralight scalar $φ$ forms a cloud that efficiently produces $χ$ particles nonperturbatively via parametric resonance, with a large mass hierarchy, $μ_χ\gg μ_φ$. Rather than escaping the system as investigated by previous studies, these $χ$ particles remain bound, orbiting the black hole. Moreover, the particle production occurs primarily at the peak of the cloud's profile, allowing $χ$ particles in quasicircular orbits to pass repeatedly through resonant regions, leading to cumulative amplification. This selective process naturally forms a dense ring of $χ$ particles, with a mass ratio to the cloud fixed by $(μ_φ/μ_χ)^2$. Our findings reveal a novel mechanism for generating bound-state particles via parametric resonance, which also impacts the evolution of the cloud. This process can be probed through its imprint on binary dynamics and its gravitational-wave signatures.
