When two black holes crash together and merge, the newly formed black hole rings like a bell, sending out gravitational waves with specific frequencies that fade over time. This brief, fading pattern of waves is called ringdown, and it may hold secrets about what is hiding around black holes.
According to Einstein’s basic rules for the simplest kind of black hole, ringdown waves depend only on two things: a black hole’s mass and how fast it spins. But what if black holes have hidden matter around them? If so, this matter would also affect the characteristics of the ringdown waves. As a result, ringdown may hold information about hidden matter surrounding the black hole. In theoretical physics, this extra structure is often called “black hole hair.”
A team led by researchers from Nagoya University in Japan has found a way to check for hair using changes in ringdown waves. They found that hidden matter does not affect these waves uniformly; the frequency and fade-out speed of the waves respond differently. This difference may show whether hidden matter is present and how its pressure is arranged around a black hole.
For spinning black holes, hidden matter affects ringdown differently, depending on whether the waves move with or against the black hole’s spin. Published in the Journal of Cosmology and Astroparticle Physics, the study identifies a pattern in the gravitational wave signal that would be a clue that hidden hair is present and may help future observations tell a hairy black hole apart from an ordinary one.
If hairy black holes exist
Scientists continue testing whether Einstein’s theory of general relativity perfectly describes black holes and what deviations may exist.
Finding signs of black hole hair is difficult because different kinds of extra matter or new physics can change the ringdown in different ways. This study gives researchers a clearer idea of what patterns to look for in future ringdown data.
“Black hole hair may represent matter surrounding the black hole or deviations from the simplest kind of black hole predicted by general relativity. Because these may slightly change the ringdown signal, detecting or ruling out these changes could give us a new way to test gravity in this extreme region,” said first author Ariadna Uxue Palomino Ylla, a Ph.D. student from Nagoya University’s Graduate School of Science.
A black hole distorts spacetime so severely that it bends the paths of light and gravitational waves. If hidden matter or new physics affects gravity, the effects would be most pronounced exactly where gravity is strongest. This makes black holes the best place to find out whether hidden matter or unknown physics might be present.
To check for hair, the team relied on a known link. The way light would orbit near a black hole corresponds to the way its ringdown waves behave, so scientists can calculate one from the other. They added a small amount of hidden matter to standard black hole models and used Einstein’s equations to calculate how that matter changes the ringdown’s frequency and fade-out speed.
The researchers tested this approach on three well-known theoretical black holes. They also extended it to spinning black holes and studied light that orbits with the spin and light that orbits against it.
Hair affects frequency and fading speed differently
A key finding is that the frequency and fade-out speed of ringdown waves do not change in the same way. The difference between them depends on how much hidden matter is present and how its pressure is arranged around the black hole.
“The ringdown waves may not only show that something extra is affecting the black hole; the way the signal changes could also give us clues about what this hidden matter is actually like,” said Palomino Ylla.
The researchers included spinning black holes in their analysis. Rotation makes calculations more complex because light circling with the black hole’s spin behaves differently from light circling against it. Hidden matter also changes the ringdown’s frequency and fade-out speed differently, depending on the spin direction. The exact pattern depends on the type of hidden matter involved.
Instead of studying each possible type of black hole hair from scratch, the new method gives researchers a common way to predict how extra matter or new physics could change a black hole’s ringdown. While the results are early estimates, this method helps scientists know what to look for if they ever spot something strange in a real black hole’s signal. In the future, this approach may help researchers use these waves to learn about a black hole’s size, spin and any black hole hair nearby.
Publication details
Ringdown waves from hairy black holes, Journal of Cosmology and Astroparticle Physics (2026). On arXiv: arxiv.org/abs/2603.15979
Journal information:
arXiv
Key concepts
Provided by
Nagoya University
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Do black holes have hidden hair? Scientists find a new way to check (2026, September 7)
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