Is dark matter the remnant of evaporated black holes? express

Original: "Signatures of loop quantum gravity in primordial black hole cosmologies"
arXiv:2605.28953 · 2026-05-27 · CC BY 4.0 · 1 min
Dark matter might be made of minuscule remnants of evaporated primordial black holes — a conclusion drawn by physicists studying the early universe.

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The universe is filled with invisible dark matter. Just as a drop of water, as it evaporates, leaves behind a tiny salt crystal, so too can a black hole evaporate, leaving behind a minuscule stable remnant. This idea was developed by Stephen Hawking and Jacob Bekenstein.

New research examined whether such remnants of primordial holes, born right after the Big Bang, could have become dark matter. It turned out that if light holes were too abundant, their 'salt grains' overproduced — the cosmos would be oversaturated. But holes with a mass of around a thousand kilograms (like a small car) evaporate just in time for our era, heating the universe along the way, and their remnants perfectly match today's dark matter.

A black hole weighing a ton would shine hotter than the Sun's core and melt like a grain of salt on a scorching frying pan, leaving an invisible trace.

While these holes were evaporating, they amplified random density fluctuations, generating a powerful background of gravitational waves — ripples in spacetime. Ground-based and space detectors, which Kip Thorne helped develop, may pick up this echo. If the signal is confirmed, we’ll know that dark matter is a handful of 'salt' from ancient black holes.

Primordial black holes can weigh as much as a mountain yet be smaller than an atom.

Scientists
Stephen HawkingJacob BekensteinFritz ZwickyVera RubinKarl SchwarzschildSubrahmanyan Chandrasekhar
Concepts
early universe black holes primordial black hole remnant primordial gravitational waves hawking radiation anomalies hawking radiation mechanism dark matter subhalo planck mass axion dark matter quantum cosmological inhomogeneities cosmic dawn magnetic signatures relic neutrino heavy quark neutron star mass limit planck length gravitational atom black hole memory burden Bekenstein-Hawking entropy globular cluster primordial magnetic fields