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Sandbox Physics

Black Hole Superradiance and Boson Clouds

How can a spinning black hole amplify a wave and grow a cloud of light particles? A wave that rotates around a spinning black hole more slowly than the horizon turns comes back stronger, because the hole gives up rotational energy. A trapped field of very light particles can then grow into a cloud, but this linear growth says nothing yet about where it stops.

Drag the black hole spin and the wave frequency. A wave with ω<mΩH\omega<m\Omega_H is reflected stronger, and a trapped boson cloud grows.

Interactive modelBlack Hole Superradiance and Boson Clouds
Horizon rotation mΩHMm\Omega_H M0.4340.434
Reflected-wave gain Z11Z_{11}0.366 %0.366\,\%
Cloud e-fold time420 s420\,\mathrm{s}
Boson rest energy mbc2m_b c^25.19×10−12 eV5.19\times10^{-12}\,\mathrm{eV}

Gain, cloud growth and where clouds grow

Computed: the gain in this browser, the cloud rates from an offline grid. No observations.

Reflected-wave gain Z11(ω)Z_{11}(\omega)
  • Kerr wave solution
  • Low-frequency formula
  • Threshold mΩHm\Omega_H

Horizontal: MωM\omega. Vertical: percent of incoming energy gained (positive) or absorbed (negative), massless field.

Cloud growth rate log⁡10(MωI)\log_{10}(M\omega_I)
  • Continued fraction at a/M=0.99a/M=0.99
  • Hydrogenic formula

Horizontal: coupling α=GMmb/(ℏc)\alpha=GMm_b/(\hbar c). The selected cloud has α=0.389\alpha=0.389. This cloud grows: its frequency is below the horizon rotation.

Where the cloud grows
  • Growing region, brighter is faster
  • Ideal switch-off astop/M=0.963a_{\mathrm{stop}}/M=0.963

Vertical: spin a/Ma/M. The dotted drop marks where growth would stop; the spin-down path itself is not computed.

How a spinning hole hands energy to a wave

BackgroundA rotating black hole drags space around with it. Its horizon turns at the angular velocity ΩH\Omega_H. A wave with azimuthal number mm and frequency ω\omega has a pattern that turns at ω/m\omega/m.

Why it mattersChange the spin and the frequency and watch whether the reflected wave comes back brighter or dimmer than the wave that went in.

One-sentence intuition
A wave pattern that turns more slowly than the horizon, ω<mΩH\omega<m\Omega_H, carries negative energy across the horizon, so the reflected wave carries out more than came in.

Core mathematical model

How fast the horizon turns

ΩH=a2Mr+,r+=M+M2−a2\Omega_H=\frac{a}{2Mr_+},\qquad r_+=M+\sqrt{M^2-a^2}

Here aa is the spin per unit mass. Without spin the horizon does not turn and no wave can gain energy.

Energy flux on both sides

ω(∣I∣2−∣R∣2)=(ω−mΩH) ∣T∣2\omega\left(|I|^2-|R|^2\right)=(\omega-m\Omega_H)\,|T|^2

The same conserved Wronskian is evaluated far away, with incoming amplitude II and reflected RR, and at the horizon with transmitted TT. The sign of ω−mΩH\omega-m\Omega_H decides whether ∣R∣>∣I∣|R|>|I|. The Lab checks this balance for every solve.

A cloud that keeps reflecting

MωI≈α948(aM−2αr+M),α=GMmbℏcM\omega_I\approx\frac{\alpha^9}{48}\left(\frac aM-2\alpha\frac{r_+}M\right),\qquad \alpha=\frac{GMm_b}{\hbar c}

A field with mass mbm_b is trapped by gravity, like an electron around a proton. This small-coupling formula is drawn dashed; the solid curve comes from an exact continued-fraction solution and is lower near the peak.

Where linear growth would stop

astopM=4mMωRm2+4M2ωR2\frac{a_{\mathrm{stop}}}{M}=\frac{4mM\omega_R}{m^2+4M^2\omega_R^2}

Growth stops once the spin has fallen so far that mΩH=ωRm\Omega_H=\omega_R. This is an ideal end point; the path there, including saturation, is not computed here.

Common difficulties

The energy does not come from inside the hole

Typical misconceptionLight or matter escapes from inside the horizon to make the wave stronger.

Better mental modelNothing crosses outward through the horizon. The transmitted wave carries negative energy inward as measured from far away, so the hole loses rotational energy while its area still grows.

Fast growth is not a particle detection

Typical misconceptionA short e-fold time means such a particle must exist, or that the cloud grows without limit.

Better mental modelThe Lab computes only linear growth for one mode. Bounds on real particles also need measured spins, the age of the system, self-interactions and the cloud’s own radiation, all of which depend on the model.

Run the experiment

  1. 01

    See the gain

    Start from the default and watch the amber outgoing fronts and the flow arrows near the horizon.

    What to observe: The gain Z11Z_{11} is positive and the arrows point outward: the reflected wave carries more energy than came in.
  2. 02

    Push past the threshold

    Drag the wavelength marker inward until the frequency exceeds the horizon rotation, or choose the absorbed preset.

    What to observe: When ω>mΩH\omega>m\Omega_H the gain turns negative and part of the wave is absorbed.
  3. 03

    Stop the spin

    Drag the spin dial back to zero and try several frequencies.

    What to observe: A non-rotating hole only absorbs. No frequency gives a positive gain.
  4. 04

    Compare the cloud curves

    Look at the growth chart, then change the black-hole mass in the advanced group.

    What to observe: The exact curve and the dashed hydrogenic one agree only at small α\alpha. A ten times heavier hole has a ten times longer e-fold time and a ten times lighter boson for the same curve.

Related experiments and articles

What this page links to directly

Spinning black holes and boson clouds · Reading path

From an amplified wave to a growing cloud

Articles on this path that use this experiment, followed by the other experiments they suggest.

  1. ArticleWhy can a spinning black hole make the waves around it ever stronger?
  2. ArticleWaves, spin and the scales of a Kerr black hole
  3. ArticleConserved flux, physical units and a first growth estimate
  4. ArticleSolving for the bound cloud's growth rate reproducibly
  5. ArticleRecomputing a published superradiance amplification table
  6. ArticleHow self-interactions change boson-cloud limits from spins and gravitational waves
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