When British physicist Roger Penrose suggested in 1969 that we could extract energy from a rotating black hole, it opened up a fascinating area of study. He theorized that within the ergosphere—a region just outside a black hole—particles could split. One part could fall into the black hole, taking negative energy with it, while the other part could escape, emerging with extra energy. It’s an idea that aligns well with general relativity. The energy absorbed from the black hole actually reduces its mass and rotation, allowing the escaping particle to gain energy without violating any physical laws.

Years later, Belarusian physicist Yakov Zel’dovich took this concept a step further. In 1971, he proposed that if a rotating metal cylinder could mimic this process, it could amplify waves similarly. The theory was that an incoming wave could gain strength by reflecting off a fast-spinning cylinder, effectively stealing energy from the cylinder’s rotation.
Zel’dovich’s prediction was bold. He imagined that if the cylinder had a mirror around it, it could amplify small signals into very powerful ones. This concept was later refined by other scientists, yet it remained unconfirmed in practice—until now.
Researchers from the University of Southampton, led by Hendrik Ulbricht, have made significant advancements. They created a rotating system using an aluminum cylinder and a three-phase magnetic field. This setup allowed them to stimulate conditions for amplifying electromagnetic waves.
By adding a resonant circuit around the cylinder, the scientists observed a remarkable phenomenon. Random background noise transformed into stronger electromagnetic waves, resembling what would happen near an actual black hole bomb. “We’re generating a signal from noise, mimicking the black hole bomb proposal,” Ulbricht explained.
This experiment is groundbreaking because it showcases how spontaneous amplification can occur, confirming theories about phenomena near rotating black holes.
The science behind the Zel’dovich effect is intriguing. When a rotating object spins faster than the incoming radiation frequency, the energy of those waves changes significantly. This shift is a variant of the Doppler effect—a familiar phenomenon that changes the pitch of a siren as an ambulance rushes by.
In past studies, the team explored this effect with sound waves. They reflected sound off a spinning disc, observing the predicted energy shift. But applying the same principle to electromagnetic waves was trickier.
The Southampton team spun the aluminum cylinder fast enough to cause incoming electromagnetic fields to become rotationally Doppler-shifted into negative frequencies. This negative frequency means negative absorption, effectively leading to amplification—a surprising and exciting result.
Vitor Cardoso, a physicist at the University of Lisbon, marveled at the implications. “You throw a low-frequency wave against a spinning cylinder, and who would think you get back more than what you threw in? It’s mind-boggling,” he shared.
The experiment’s implications extend even further. Physicists believe superradiance—the driving force behind the black hole bomb—could help detect new particles, including candidates for dark matter. “Superradiance is turning black holes into far better particle detectors than even CERN,” Cardoso noted.
If lightweight particles exist, they might cluster around spinning black holes, siphoning energy via superradiance. This could lead scientists to detect unusual gravitational waves or find that black holes spin down faster than expected.
The laboratory evidence for superradiant amplification boosts researchers’ confidence in searching for signs of these phenomena in real black hole systems in the universe.
In their study on arXiv, the Southampton team explained how the aluminum cylinder did more than simply amplify electromagnetic waves; it acted as a self-sustaining generator. Once noise initiated the amplification, the energy surged exponentially.
The results align with earlier theories predicting that a decrease in rotational energy would eventually halt the amplification, similar to what occurs with real black holes losing spin.
This experiment traces a line back to Penrose, Zel’dovich, and others, translating the complexities of black hole physics into something tangible in the lab. As scientists push boundaries, they aspire to observe spontaneous electromagnetic wave generation driven by quantum vacuum fluctuations—a challenging yet tantalizing goal.
The Southampton team is enthusiastic: “Based on our findings, this remains a technological challenge, but certainly an achievable one.”
With simple tools—a spinning cylinder, mirrors, and clever electromagnetic setups—researchers are uncovering the mysteries of the universe’s most extreme phenomena, all from the comfort of Earth.
For more detailed studies and digging deeper into the physics of this experiment, you can check the arXiv publication.
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