How fast the horizon turns
Here is the spin per unit mass. Without spin the horizon does not turn and no wave can gain energy.
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 is reflected stronger, and a trapped boson cloud grows.
Computed: the gain in this browser, the cloud rates from an offline grid. No observations.
Horizontal: . Vertical: percent of incoming energy gained (positive) or absorbed (negative), massless field.
Horizontal: coupling . The selected cloud has . This cloud grows: its frequency is below the horizon rotation.
Vertical: spin . The dotted drop marks where growth would stop; the spin-down path itself is not computed.
BackgroundA rotating black hole drags space around with it. Its horizon turns at the angular velocity . A wave with azimuthal number and frequency has a pattern that turns at .
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.
Here is the spin per unit mass. Without spin the horizon does not turn and no wave can gain energy.
The same conserved Wronskian is evaluated far away, with incoming amplitude and reflected , and at the horizon with transmitted . The sign of decides whether . The Lab checks this balance for every solve.
A field with mass 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.
Growth stops once the spin has fallen so far that . This is an ideal end point; the path there, including saturation, is not computed here.
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.
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.
Start from the default and watch the amber outgoing fronts and the flow arrows near the horizon.
What to observe: The gain is positive and the arrows point outward: the reflected wave carries more energy than came in.Drag the wavelength marker inward until the frequency exceeds the horizon rotation, or choose the absorbed preset.
What to observe: When the gain turns negative and part of the wave is absorbed.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.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 . A ten times heavier hole has a ten times longer e-fold time and a ten times lighter boson for the same curve.You are hereBlack Hole Superradiance and Boson Clouds
Spinning black holes and boson clouds · Reading path
Articles on this path that use this experiment, followed by the other experiments they suggest.