Tiny Black Holes Don’t Warp the Cosmos express

Original: "Primordial black holes from inflation: on the decoupling between large and small scales"
· Laura Iacconi
arXiv:2605.04815v1 · 2026-05-06 · CC BY 4.0 · 1 min
The cosmic symphony fears no dark dwarfs: [tag:black_hole]primordial black holes[/tag] don’t drown out the echo of the [tag:big_bang]Big Bang[/tag].

Right after the Big Bang, the Universe expanded incredibly fast — this phase was called inflation. In some microscopic regions, matter randomly clumped so much that it collapsed into primordial black holes. They are tiny — the size of a proton, yet as massive as an iceberg.

Scientists were tormented by the question: wouldn’t these turbulent small-scale processes spoil the delicate picture of large-scale waves we observe in the cosmic microwave background? Alan Guth soothed: the basses and flutes in the cosmic symphony play at different frequencies and don’t interfere with each other. New calculations proved that any back-reaction is a thousand times weaker than the sensitivity threshold of our instruments. The melody of the cosmos remains pure.

Thus primordial black holes earned the right to be considered part of dark matter — the invisible substance that holds galaxies together. The irony is that, according to Stephen Hawking’s calculations, ordinary black holes evaporate, while these long-lived ones will exist forever.

A black hole the size of a proton has the mass of an iceberg.

Scientists
Stephen HawkingJacob BekensteinFritz ZwickyKarl SchwarzschildRalph AlpherSubrahmanyan Chandrasekhar
Concepts
early universe black holes primordial black hole mass inflation primordial gravitational waves bubble collision eternal inflation inflationary cosmology nuclear reaction mass gap critical collapse wave amplification big bang scalar perturbations quasi periodic eruptions early dark energy particle creation quantum cosmological inhomogeneities barrow entropy Penrose process Hawking radiation hawking radiation mechanism