The Rhythm of Black Holes from the Early Universe ✎ express

Original: "Cosmological discrete self-similarity in primordial black hole formation"
arXiv:2604.21520 · 2026-04-23 · arXiv non-exclusive · independent analysis · 1 min
The birth of primordial black holes follows a rhythm where the same mass jump repeats again and again, like an echo.

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Drops from a leaky faucet beat a clear rhythm. A similar rhythm, only on the scale of the universe, has been found by astrophysicists: the formation of primordial black holes — tiny objects born in the first moments after the Big Bang — also proceeds not chaotically, but in a strictly measured way. The mass of such a hole grows not smoothly, but in jumps, as if repeating the same pattern over and over, but each time on a smaller scale.

Previously, this "rhythmicity" was known only for an idealized, non-expanding universe. New modeling on the expanding universe — which is what our universe was like in the beginning — has confirmed that the stepped rhythm persists. This is critically important because primordial black holes are considered one of the main candidates for dark matter — the invisible framework holding galaxies together.

Because of the rhythmicity, future detectors of gravitational waves — ripples in spacetime — will be able to pick up not random noise, but an ordered "melody" played by merging holes. And here's an unexpected twist: these holes could be so small that, flying through Earth, they wouldn't touch a single atom, even though each one weighs as much as a mountain.

Primordial black holes, if they exist, can be the size of an atom but weigh as much as a mountain.

Scientists
Stephen HawkingJacob BekensteinHenri PoincaréFritz ZwickyKarl SchwarzschildJoseph Weber
Concepts
early universe black holes direct collapse black holes massless scalar field critical collapse cosmic string schwarzschild metric scalar perturbations anti de sitter space decoherence free subspace spontaneous scalarization non singular cosmology cosmic structure formation dark matter subhalo primordial black hole gravitational singularity Penrose singularity theorem quasinormal modes scalar particle