Roger Penrose theorized that spinning cosmic black holes can act like giant power plants by boosting the energy of incoming light waves; quantum physicists simulated that exact black hole energy-theft mechanism on a laboratory tabletop using rotating light pulses. Published in Nature, this breakthrough observation validates Floquet rotational superradiance, providing the first table-top laboratory proof of Penrose black-hole physics.

In 1969, Nobel laureate Roger Penrose and Soviet physicist Yakov Zel'dovich predicted an extraordinary cosmic phenomenon: if a wave of light brushes against the outer edge of a spinning black hole, it does not get swallowed—instead, it robs rotational energy from the black hole and bounces back with more energy than it started with. For over fifty years, testing this relativistic prediction in deep space remained impossible.
Quantum physicists built an optical table-top simulator using Floquet physics. By firing laser beams into a synthetic spinning medium that mimics the swirling spacetime vortex around a black hole, they watched incoming light waves absorb energy from the rotation and emerge thirty percent brighter than when they entered.
This laboratory experiment confirmed fifty years of black-hole theory. By demonstrating how rotational energy can be extracted directly from spacetime vortices, by unlocking new methods to amplify laser signals without electronic power, and by advancing quantum gravity simulation, tabletop superradiance bridges astrophysics with quantum optics.
Observation of Floquet rotational super-radiance
Time-driven systems provide a framework for controlling waves through spatio-temporal modulation, which enables the synthesis of effective motion without mechanical displacement. Within this framework, travelling-wave modulations can emulate moving media and give rise to phenomena such as Doppler-induced non-reciprocity. A related effect is the extraction of energy from rotating media, which has been theoretically predicted to occur when waves experience sufficiently large rotational Doppler shifts. Experimental access to this regime has remained limited due to the extreme rotation speeds required in mechanically rotating systems. Here we show that Floquet-induced rotation enables access to such ultrafast rotational regimes using purely spatio-temporal modulation. When spinning at effective superluminal speeds, angular-momentum bandgaps emerge in the band structure of the underlying space-time crystal. These gaps host parametric processes that efficiently extract energy from the Floquet-rotating medium, resulting in angular-momentum-selective amplification of orbital waves within a dissipation-shaped spectral bandwidth. We realize this effect experimentally in a ring network of time-modulated resonators, where we observe a Floquet regime of rotational super-radiance mediated by non-Hermitian and parametric dynamics in space-time structured media. These results demonstrate a controllable platform for studying rotational energy transfer and angular-momentum-dependent wave amplification in space-time-modulated media.
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