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Neutrons, Rotating Black Holes, and a Galactic PeVatron at the Center of the Milky Way

A study asks if we can detect the Penrose process, where a spinning black hole loses energy through a twist in spacetime.

By mitch·5 min read
A black hole at the center of a galaxy emits energetic particles from its swirling accretion disk.

Black holes have a new job description: galactic mitochondria. That’s the comparison scientists are making, and it’s not a joke. Most of the energy these supermassive black holes produce comes from the material surrounding them, specifically superheated plasma in their accretion disks interacting with tremendous magnetic fields. But there’s a more direct way to extract energy from a black hole, and a new study is asking whether we can spot the signature of that process.

The method is called the Penrose process, a way of extracting energy from a spinning black hole through a clever twist in the fabric of spacetime itself. A new study asks whether we might detect evidence of this process happening naturally in the cosmos.

Black Holes As Powerhouses

The comparison to mitochondria is apt in a narrow sense. Mitochondria are the powerhouses of cells, converting energy from food into a form the cell can use. Galactic black holes are the powerhouses of galaxies, converting matter into light and radiation on a cosmic scale. The similarity holds at the level of function, even if the mechanism looks nothing like biology.

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Most of the energy a black hole produces comes from the material swirling around it. Accretion disks are made of superheated plasma, gas heated to millions of degrees by friction and gravity. Magnetic fields wrap around the disk, twisting and amplifying until they release energy in explosive bursts.

The Penrose Process

The Penrose process works differently. It doesn’t rely on surrounding material at all. Instead, it extracts energy directly from the black hole’s rotation. The idea is that particles falling toward the black hole can gain energy by borrowing some of the hole’s spin.

Here’s how it works in broad strokes:

  • A particle approaches the black hole along a path that carries it near the event horizon.
  • Some of the particle’s mass-energy is converted into extra kinetic energy.
  • The particle escapes with more energy than it had when it entered.
  • The black hole spins slightly slower as a result.

The trade is not free. The black hole loses angular momentum each time the process happens, and eventually the effect would slow the hole down. But over short timescales, the process can release a significant amount of energy.

Detecting The Signature

The new study asks whether we could detect a signature of this process in nature. The challenge is that the Penrose process is a subtle effect, and distinguishing it from the usual fireworks of an accretion disk is difficult. The study does not claim a detection, but it asks whether the signal exists and whether we have instruments sensitive enough to see it.

The signal would likely show up as a particular pattern in the light or gamma rays coming from a black hole. The exact shape of that pattern depends on the details of how particles move near the event horizon. Spotting it would require careful observation and sophisticated analysis.

A Galactic PeVatron

One of the most intriguing targets for this kind of search is the supermassive black hole at the center of the Milky Way. That black hole is a natural laboratory for studying these effects. It’s surrounded by a region of intense activity.

The galaxy’s core hosts a galactic PeVatron, a source of extremely high-energy particles. The central black hole is a prime suspect for producing these particles. The Penrose process could explain some fraction of those particles.

What The Study Asks

The study is not claiming a discovery. It is asking a question: can we find evidence that black holes are losing energy through the Penrose process? The answer is not yet known, and the study does not provide one.

What the study does offer is a framework for thinking about how we might look for such a signal. It asks whether we could discover a signature of the Penrose process.

Why This Matters

The Penrose process is a beautiful piece of theoretical physics, but it also has practical implications. If we can confirm that black holes lose energy this way, it changes our understanding of how these objects evolve over time. It also offers a natural mechanism for producing the highest-energy particles in the universe.

The comparison to mitochondria is a useful shorthand, but it’s not a complete picture. Black holes are not biological machines. They are regions of spacetime where the rules of physics behave in ways that seem strange to us. The fact that they share a functional role with cellular powerhouses is a reminder of how deeply connected the universe is, even across scales that seem utterly different.

The study is a reminder that the cosmos is full of surprises. Even a black hole, one of the most fearsome objects in existence, can be understood in terms of energy flows and conservation laws. The Penrose process shows that the universe is not wasteful. Energy extracted from a black hole’s spin is not lost forever; it simply moves elsewhere.

Whether we can detect that signal is an open question. The study asks whether we can spot a Penrose-process signature, and the answer will depend on whether our instruments are sharp enough to see it. For now, the comparison stands: black holes are the powerhouses of the galaxy, and we are only beginning to understand how they work.

Source material: “Neutrons, rotating black holes, and a galactic PeVatron at the center of the Milky Way,” Phys.org.

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