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Long-lived black holes: how their slow boiling is heard in a radio signal from the past ⚡ экспресс

Original: "Probing memory-burdened Primordial Black Holes with global 21 cm signal"
· Priyanka Sarmah, Kingman Cheung
arXiv:2512.06941 · 2025-12-07 · CC BY · ⏱ 1 min · Cosmology HEP Phenomenology
Tiny black holes evaporate not in an explosion but in a long boil — and their heat can still be heard in the radio whisper of hydrogen from the early universe.
Abstract

Some black holes live longer than expected: the memory effect slows their evaporation, like sand jamming an hourglass. In the early Universe, such holes could have heated hydrogen and left a mark in the radio signal picked up by telescopes. This helps solve the dark matter puzzle. What whispers will the echo of the cosmic dawn bring?

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Tiny black holes, born in the first moments after the Big Bang, should have disappeared long ago according to Hawking's theory — evaporated like a puddle of water under the sun. But new calculations show evaporation isn't that fast. The hole seems to choke on its own radiation — like a boiling pot covered by a cloud of steam, slowing the boil. This 'memory burden' effect turns an instantaneous flash into a long, slow fading.

Such 'underboiled' holes spent eons warming the surrounding hydrogen in the young universe. Hydrogen atoms, feeling the heat, change their radio voice — 21-cm radiation. Astronomers catch this ancient signal and see it's too cold. If black holes were more than a tiny fraction, they would have heated the gas more, distorting the radio picture. So these objects cannot be dark matter — their number is less than one ten-millionth of the required amount.

🎯 The most sensitive tool for hunting dark matter isn't a giant underground detector, but an ordinary radio telescope listening to the echo of hydrogen from the time before the first stars lit up.

Scientists
Alan GuthAndrei LindeGeorges LemaîtreJames PeeblesAdam RiessBrian Schmidt
Tags
dark matter black hole hydrogen big bang
Laws
Friedmann equationsHubble's lawHawking radiationgravitational lensingBekenstein-Hawking entropyCoulomb's law
Original: arXiv:2512.06941 · CC BY · bridge42worlds