Black Holes Evaporate, but Gravitational Waves Remember express

Original: "Universal Suppression of Gravitational Waves from Black Hole Evaporation Dynamics"
arXiv:2606.09804 · 2026-06-08 · CC BY 4.0 · 2 min
As they evaporate, black holes leave a characteristic imprint on the gravitational-wave background that does not depend on their initial properties.

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A black hole is not an eternal vacuum cleaner. Left alone in the void, it slowly disappears, radiating energy like a puddle drying on asphalt. This process, predicted by Stephen Hawking, is called evaporation. The smaller the hole, the faster it melts, and the hotter its "breath."

The authors of the study looked not at a single hole but at a whole cloud of such objects — for example, primordial black holes that might have formed in the early universe. Their masses are not identical but spread over a range. It turns out that over time, this cloud inevitably changes its shape according to a single scenario dictated by evaporation. It's like a puddle leaving behind smaller puddles of different sizes, but all of them dry up according to a common law, and in the end only the smallest ones remain, vanishing last.

The lightest black holes evaporate fastest, so in an old cloud, objects with masses just above the threshold of complete disappearance dominate.

This redistribution of masses leaves a trace in gravitational waves — ripples in spacetime that such holes could have generated in the distant past. The spectrum of these waves (the frequency distribution) acquires a characteristic power-law decline at low frequencies — a universal signature of evaporation. Importantly, this signature does not depend on how the masses were initially distributed, whether by critical collapse or any other mechanism. Nature seems to stamp a label: "Hawking evaporation was at work here."

By observing the gravitational-wave background, we can peer into an era when the universe was less than a second old and test whether black holes existed then.

Original abstract

as written by the authors arXiv:2606.09804

Evaporating black holes can leave distinct imprints on gravitational wave (GW) backgrounds. We show that black hole populations with finite width mass distributions exhibit a universal late time evolution governed by the evaporation dynamics rather than the details of the initial mass distribution, leading to a characteristic power law suppression of the induced GWs. We demonstrate this for a broad class of mass functions in primordial black hole (PBH) scenarios featuring an early Universe matter-dominated era, and identify the suppression of PBH-induced GWs found for critical collapse distributions as a manifestation of this general phenomenon. Our results establish a direct connection between the asymptotic GW spectrum and the underlying law of black hole evaporation.

A black hole with the mass of a small asteroid would evaporate in a time billions of times shorter than the age of the universe, while a supermassive black hole at the center of a galaxy would take longer to melt than all the stars put together have existed.

In Dan Simmons's novel "Hyperion," evaporating black holes are used as weapons capable of destroying entire star systems — here, the same process, but on cosmological scales.

Scientists
Stephen HawkingJacob BekensteinJohn Archibald WheelerHenri PoincaréFritz ZwickyKarl Schwarzschild
Concepts
black hole evaporation black hole memory burden gravitational wave propagation accretion disk wind gravitational wave echoes information loss Law of Universal Gravitation hawking area law Hawking area theorem critical collapse remnant tidal disruption event no-hair theorem quantum corrections apparent horizon galactic dust winds backreaction quasar feedback gravastar quantum gravity effects