Tiny Black Holes Warm the Universe Longer Than Thought express

Original: "Accretion Effects on Primordial Black Hole Reheating Constraints"
· Chenhuan Wang
arXiv:2605.15772 · 2026-05-15 · CC BY 4.0 · 2 min
Tiny black holes that might have filled the early universe gobbled up matter and grew, delaying their final heating.

📄 Showing the "Simple" version — "Popular" is not ready yet. Add it to favorites to help prioritize it.

A tiny black hole the size of an atomic nucleus but with the mass of a mountain emerged in the first moments after the Big Bang, when random clumps of energy collapsed into such objects. If enough of these holes existed, they could have temporarily become the universe's main content, then evaporated via Hawking radiation — the slow 'melting' of a black hole as it releases energy back into space.

But a black hole doesn't hang in a vacuum. It pulls in dust and gas like a whirlpool dragging in leaves. This is accretion — matter falling onto the hole. The new analysis shows that such 'feeding' not only inflates the hole but also stretches its reign. The universe stays under the sway of these invisible giants-in-miniature for longer.

A tiny black hole with the mass of an asteroid could evaporate over a time comparable to the universe's age, but accretion could extend its life severalfold.

When the holes finally vanish, their departure is not silent. The abrupt change in the gravitational field generates gravitational waves — ripples in spacetime itself, like the rings from a stone tossed into a pond. These waves, arising from density inhomogeneities, are called isocurvature. Their energy is limited by what we know about primordial nucleosynthesis — the epoch when the first atomic nuclei formed. Waves that are too strong would have disrupted this process.

Taking accretion into account significantly shifts the allowed bounds for primordial black holes: they must be lighter and rarer than previously thought. Even if black holes merge with each other to form larger ones, the constraints remain strict. Isocurvature gravitational waves turn out to be a more sensitive probe than the mergers themselves.

If a primordial black hole with the mass of Everest were in a room, it would evaporate in a fraction of a second, but before that, its gravity would tear everything around it into atoms.

So tiny black holes, barely born, manage to gain weight and delay their finale. And we, observing the ripple of space, can peer into that epoch when the universe was younger than a second.

A primordial black hole with a mass of 10¹⁵ grams (like a small asteroid) has the size of a proton, and its temperature is billions of times hotter than the Sun's core: it would shine brighter than a star, but only in gamma rays.

In Terry Pratchett's novel 'The Pillars of Creation', tiny black holes were used as an energy source — much like the scenario of heating the early universe.

Scientists
Stephen HawkingJacob BekensteinRoger PenroseHenri PoincaréFritz ZwickyKarl Schwarzschild
Concepts
black hole accretion winds black hole memory burden Accretion disk Hawking radiation wave amplification hawking radiation mechanism mass inflation logarithmic correction reheating Penrose process quasi periodic eruptions primordial gravitational waves nuclear reaction mass gap barrow entropy quasar feedback quantum corrections Bekenstein-Hawking entropy early dark energy gravitational wave echoes backreaction